Supernovae

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References

1 - Books

[1-1]
Neutrinos in particle physics, astronomy and cosmology, Zhi-zhong Xing, Shun Zhou, Zhejiang University Press, Hangzhou, 2011. ISBN: 978-7308080248. http://www.zjupress.com/en/redir.php?catalog_id=64&book_id=1446.
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[1-2]
Fundamentals of Neutrino Physics and Astrophysics, C. Giunti, C. W. Kim, Oxford University Press, Oxford, UK, 2007. ISBN 978-0-19-850871-7. http://www.oup.com/uk/catalogue/?ci=9780198508717.
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[1-3]
Stars as laboratories for fundamental physics: The astrophysics of neutrinos, axions, and other weakly interacting particles, G.G. Raffelt, University of Chicago Press, 1996. ISBN 0-226-70272-3. http://wwwth.mpp.mpg.de/members/raffelt/pages/mybook.html.
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[1-4]
Neutrino Astrophysics, J. N. Bahcall, Cambridge University Press, 1989.
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[1-5]
Black Holes, White Dwarfs, and Neutron Stars: the Physics of Compact Objects, S. L. Shapiro, S. A. Teukolsky, John Wiley, 1983.
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[1-6]
An Introduction to the Study of Stellar Structure, S. Chandrasekhar, University of Chicago Press, 1938.
[Chandrasekhar-1938]

2 - Reviews

[2-1]
Supernovae from massive stars, Marco Limongi, arXiv:1706.01913, 2017.
[Limongi:2017ggo]
[2-2]
Nucleosynthesis in thermonuclear supernovae, Ivo R. Seitenzahl, Dean M. Townsley, arXiv:1704.00415, 2017.
[Seitenzahl:2017ctl]
[2-3]
Combustion in thermonuclear supernova explosions, Friedrich K. Roepke, arXiv:1703.09274, 2017.
[Roepke:2017our]
[2-4]
Neutrino-driven Explosions, H.-Th. Janka, arXiv:1702.08825, 2017.
[Janka:2017vcp]
[2-5]
Neutrino Emission from Supernovae, H.-Th. Janka, arXiv:1702.08713, 2017.
[Janka:2017vlw]
[2-6]
Spectra of supernovae in the nebular phase, A. Jerkstrand, arXiv:1702.06702, 2017.
[Jerkstrand:2017ruq]
[2-7]
Supernova Remnants as Clues to Their Progenitors, Daniel Patnaude, Carles Badenes, arXiv:1702.03228, 2017.
[Patnaude:2017uyc]
[2-8]
Supernova of 1006 (G327.6+14.6), Satoru Katsuda, arXiv:1702.02054, 2017.
[Katsuda:2017rwh]
[2-9]
Thermal and non-thermal emission from circumstellar interaction, Roger A. Chevalier, Claes Fransson, arXiv:1612.07459, 2016.
[Chevalier:2016hzo]
[2-10]
The effects of supernovae on the dynamical evolution of binary stars and star clusters, Richard J. Parker, arXiv:1609.05908, 2016.
[1609.05908]
[2-11]
Massive Computation for Understanding Core-Collapse Supernova Explosions, Christian D. Ott, arXiv:1608.08069, 2016.
[Ott:2016rsr]
[2-12]
The Status of Multi-Dimensional Core-Collapse Supernova Models, B. Muller, Publ.Astron.Soc.Austral. 33 (2016) 48, arXiv:1608.03274.
[Muller:2016izw]
[2-13]
Shock breakout theory, Eli Waxman, Boaz Katz, arXiv:1607.01293, 2016.
[Waxman:2016qyw]
[2-14]
Frontiers in Nuclear Astrophysics, Carlos A. Bertulani, Toshitaka Kajino, Prog.Part.Nucl. Phys. 89 (2016) 56-100, arXiv:1604.03197.
[Bertulani:2016eru]
[2-15]
A review of the impact of sterile neutrino dark matter on core-collapse supernovae, MacKenzie Warren, Grant J. Mathews, Matthew Meixner, Jun Hidaka, Toshitaka Kajino, Int.J.Mod.Phys. A31 (2016) 1650137, arXiv:1603.05503.
[Warren:2016slz]
[2-16]
Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview, H.-Thomas Janka, Tobias Melson, Alexander Summa, Ann.Rev.Nucl.Part.Sci. 66 (2016) 341-375, arXiv:1602.05576.
[Janka:2016fox]
[2-17]
The Equation of State of Hot, Dense Matter and Neutron Stars, James M. Lattimer, M. Prakash, Phys.Rept. 621 (2016) 127-164, arXiv:1512.07820.
[Lattimer:2015nhk]
[2-18]
Supernova Neutrinos: Production, Oscillations and Detection, Alessandro Mirizzi et al., Riv. Nuovo Cim. 39 (2016) 1, arXiv:1508.00785.
[Mirizzi:2015eza]
[2-19]
Observational constraints on the progenitors of core-collapse supernovae : the case for missing high mass stars, S. J. Smartt, Publ.Astron.Soc.Austral. 32 (2015) e016, arXiv:1504.02635.
[Smartt:2015sfa]
[2-20]
Neutrino-nucleus reactions and their role for supernova dynamics and nucleosynthesis, K. G. Balasi, K. Langanke, G. Martinez-Pinedo, Prog. Part. Nucl. Phys. 85 (2015) 33-81, arXiv:1503.08095.
[Balasi:2015dba]
[2-21]
The explosion mechanism of core-collapse supernovae: progress in supernova theory and experiments, Thierry Foglizzo et al., Publ.Astron.Soc.Austral. 32 (2015) 9, arXiv:1501.01334.
[Foglizzo:2015dma]
[2-22]
Supernovae and the Galactic Ecosystem, Q. Daniel Wang, IAU Symp. 296 (2014) 273, arXiv:1401.6209.
[Wang:2014gpa]
[2-23]
Diverse, massive-star-associated sources for elements heavier than Fe and the roles of neutrinos, Yong-Zhong Qian, J. Phys. G41 (2014) 044002, arXiv:1310.4462.
[Qian:2013fsa]
[2-24]
Neutrinos in Cosmology and Astrophysics, A.B. Balantekin, G. M. Fuller, Prog.Part.Nucl. Phys. 71 (2013) 162-166, arXiv:1303.3874.
[Balantekin:2013gqa]
[2-25]
Neutrino astrophysics, Cristina Volpe, Ann.Phys.(Berlin) 525 (2013) 588-599, arXiv:1303.1681.
[Volpe:2013kxa]
[2-26]
Neutrino Astrophysics, W. C. Haxton, arXiv:1209.3743, 2012.
[Haxton:2012bk]
[2-27]
Explosion Mechanisms of Core-Collapse Supernovae, H.-Thomas Janka, Ann. Rev. Nucl. Part. Sci. 62 (2012) 407-451, arXiv:1206.2503.
[Janka:2012wk]
[2-28]
Supernova Neutrino Detection, Kate Scholberg, J. Phys. Conf. Ser. 375 (2012) 042036, arXiv:1205.6003.
[Scholberg:2012id]
[2-29]
Equation of State for Proto-Neutron Star, Gang Shen, arXiv:1202.5791, 2012.
[Shen:2012fq]
[2-30]
Massive Stars and their Supernovae, Friedrich-Karl Thielemann, Raphael Hirschi, Matthias Liebendorfer, Roland Diehl, Lect.Notes Phys. 812 (2011) 153, arXiv:1008.2144.
[Thielemann:2010ux]
[2-31]
Diffuse supernova neutrinos at underground laboratories, Cecilia Lunardini, Astropart.Phys. 79 (2016) 49-77, arXiv:1007.3252.
[Lunardini:2010ab]
[2-32]
The Diffuse Supernova Neutrino Background, John F. Beacom, Ann. Rev. Nucl. Part. Sci. 60 (2010) 439, arXiv:1004.3311.
[Beacom:2010kk]
[2-33]
Low energy neutrino scattering measurements at future Spallation Source facilities, R. Lazauskas, C. Volpe, J. Phys. G37 (2010) 125101, arXiv:1004.0310.
[Lazauskas:2010rh]
[2-34]
Collective Neutrino Oscillations, Huaiyu Duan, George M. Fuller, Yong-Zhong Qian, Ann. Rev. Nucl. Part. Sci. 60 (2010) 569-594, arXiv:1001.2799.
[Duan:2010bg]
[2-35]
Search for CP violation in the lepton sector, Cristina Volpe, Prog. Part. Nucl. Phys. 64 (2010) 325-333, arXiv:0911.4314.
[Volpe:2009tc]
[2-36]
Neutrino flavour transformation in supernovae, Huaiyu Duan, James P Kneller, J. Phys. G36 (2009) 113201, arXiv:0904.0974.
[Duan:2009cd]
[2-37]
The Gravitational Wave Signature of Core-Collapse Supernovae, Christian D. Ott, Class. Quant. Grav. 26 (2009) 063001, arXiv:0809.0695.
[Ott:2008wt]
[2-38]
The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries, M. Arnould, S. Goriely, K. Takahashi, Phys. Rept. 450 (2007) 97-213, arXiv:0705.4512.
[Arnould:2007gh]
[2-39]
Supernova neutrinos, from back of the envelope to supercomputer, Christian Y. Cardall, arXiv:astro-ph/0701831, 2007.
[Cardall:2007dy]
[2-40]
Theory of Core-Collapse Supernovae, H.-Th. Janka et al., Phys. Rept. 442 (2007) 38-74, arXiv:astro-ph/0612072.
[Janka:2006fh]
[2-41]
The Supernova - Gamma-Ray Burst Connection, S. E. Woosley, J. S. Bloom, Ann. Rev. Astron. Astrophys. 44 (2006) 507-556, arXiv:astro-ph/0609142.
[Woosley:2006fn]
[2-42]
The Physics of Core-Collapse Supernovae, S. Woosley, H.-T. Janka, Nature Phys. 1 (2006) 147-154, arXiv:astro-ph/0601261.
[Woosley:2006ie]
[2-43]
The physics of dense hadronic matter and compact stars, Armen Sedrakian, Prog. Part. Nucl. Phys. 58 (2007) 168-246, arXiv:nucl-th/0601086.
[Sedrakian:2006mq]
[2-44]
Six Years of Chandra Observations of Supernova Remnants, Martin C. Weisskopf, John P. Hughes, arXiv:astro-ph/0511327, 2005.
[Weisskopf:2005pf]
[2-45]
Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae, Kei Kotake, Katsuhiko Sato, Keitaro Takahashi, Rept. Prog. Phys. 69 (2006) 971, arXiv:astro-ph/0509456.
[Kotake:2005zn]
[2-46]
Supernovae: Explosions in the Cosmos, Paingalil Kunjan Suresh, V. H. Satheesh Kumar, Science Reporter 42 (2005) 20, arXiv:astro-ph/0504597.
[Suresh:2005zk]
[2-47]
Progenitors of Core-Collapse Supernovae, John J. Eldridge, arXiv:astro-ph/0502046, 2005.
[Eldridge:2005pv]
[2-48]
Type Ia Supernovae and Cosmology, Alexei V. Filippenko, Astrophys.Space Sci.Libr. 332 (2005) 97, arXiv:astro-ph/0410609.
[Filippenko:2004ub]
[2-49]
Relic neutrino background from cosmological supernovae, Shin'ichiro Ando, Katsuhiko Sato, New J. Phys. 6 (2004) 170, arXiv:astro-ph/0410061.
[Ando:2004hc]
[2-50]
The Physics of Neutron Stars, J.M. Lattimer, M. Prakash, Science 304 (2004) 536-542, arXiv:astro-ph/0405262.
[Lattimer:2004pg]
[2-51]
Astrophysical Neutrino Telescopes, A. B. McDonald et al., Rev. Sci. Instrum. 75 (2004) 293, arXiv:astro-ph/0311343.
[McDonald:2003xn]
[2-52]
Supernova Science at Spallation Neutron Sources, W. R. Hix, A. Mezzacappa, O. E. B. Messer, S. W. Bruenn, J. Phys. G29 (2003) 2523, arXiv:astro-ph/0310763.
[Hix:2003vv]
[2-53]
Advances in r-Process Nucleosynthesis, John J. Cowan, Christopher Sneden, arXiv:astro-ph/0309802, 2003.
[Cowan:2003ej]
[2-54]
The Accelerating Universe and Dark Energy: Evidence from Type Ia Supernovae, A. V. Filippenko, Lect. Notes Phys. 646 (2004) 191, arXiv:astro-ph/0309739.
[Filippenko:2003ta]
[2-55]
Supernova Neutrino-Nucleus Astrophysics, A. B. Balantekin, G. M. Fuller, J. Phys. G29 (2003) 2513, arXiv:astro-ph/0309519.
[Balantekin:2003ip]
[2-56]
Shocks and Particle Acceleration in Supernova Remnants: Observational Features, Jacco Vink, Adv.Space Res. 33 (2004) 356, arXiv:astro-ph/0304176.
[Vink:2003tz]
[2-57]
Optical Light Curves of Supernovae, Bruno Leibundgut, Nicholas B.Suntzeff, Lect.Notes Phys. (2003), arXiv:astro-ph/0304112.
[Leibundgut:2003cp]
[2-58]
Measuring Cosmology with Supernovae, Saul Perlmutter, Brian P. Schmidt, Lect. Notes Phys. 598 (2003) 195-217, arXiv:astro-ph/0303428.
[Perlmutter:2003kf]
[2-59]
The Historical Supernovae, D. A. Green, F. R. Stephenson, Lect.Notes.Phys. (2003), arXiv:astro-ph/0301603.
[Green:2003ir]
[2-60]
The Origin of the Heavy Elements: Recent Progress in the Understanding of the r-Process, Yong-Zhong Qian, Prog. Part. Nucl. Phys. 50 (2003) 153, arXiv:astro-ph/0301422.
[Qian:2003wd]
[2-61]
Physics of SNeIa and Cosmology, P. Hoeflich, C. Gerardy, E. Linder, H. Marion, Lect.Notes Phys. 635 (2003) 203, arXiv:astro-ph/0301334.
[Hoflich:2003bg]
[2-62]
Classification of Supernovae, Massimo Turatto, Lect.Notes Phys. 598 (2003) 21, arXiv:astro-ph/0301107.
[Turatto:2003np]
[2-63]
Explosion Mechanisms of Massive Stars, H.-Th. Janka et al., arXiv:astro-ph/0212314, 2002.
[Janka:2002eg]
[2-64]
Absolute values of neutrino masses: Status and prospects, S. M. Bilenky, C. Giunti, J. A. Grifols, E. Masso, Phys. Rep. 379 (2003) 69-148, arXiv:hep-ph/0211462.
[Bilenky:2002aw]
[2-65]
Neutrino-Matter Interaction Rates in Supernovae: The Essential Microphysics of Core Collapse, A. Burrows, T. A. Thompson, arXiv:astro-ph/0211404, 2002.
[Burrows:2002jv]
[2-66]
Supernova remnants and gamma-ray sources, Diego F. Torres, Gustavo E. Romero, Thomas M. Dame, Jorge A. Combi, Yousaf M. Butt, Phys. Rep. 382 (2003) 303, arXiv:astro-ph/0209565.
[Torres:2002af]
[2-67]
Observations and Theory of Supernovae, J. Craig Wheeler, Am. J. Phys. 71 (2003) 11, arXiv:astro-ph/0209514.
[Wheeler:2002gw]
[2-68]
The evolution and explosion of massive stars, S. E. Woosley, A. Heger, T. A. Weaver, Rev. Mod. Phys. 74 (2002) 1015-1071.
[Woosley-Heger-Weaver-RMP74-2002]
[2-69]
Element Synthesis in Stars, F. K. Thielemann et al., Prog. Part. Nucl. Phys. 46 (2001) 5-22, arXiv:astro-ph/0101476.
[Thielemann:2001rn]
[2-70]
Observational neutrino astrophysics, M. Koshiba, Phys. Rep. 220 (1992) 229-381.
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[2-71]
Neutrino astronomy, Y. Totsuka, Rept. Prog. Phys. 55 (1992) 377-430.
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Galactic and extragalactic supernova rates, S. van den Bergh, G. A. Tammann, Ann. Rev. Astron. Astrophys. 29 (1991) 363-407.
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[2-73]
Supernova mechanisms, H. A. Bethe, Rev. Mod. Phys. 62 (1990) 801-866.
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The number of neutrino species, D. Denegri, B. Sadoulet, M. Spiro, Rev. Mod. Phys. 62 (1990) 1.
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[2-75]
1987A: The greatest supernova since Kepler, V. Trimble, Rev. Mod. Phys. 60 (1988) 859-871.
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1987A: The greatest supernova since Kepler, V. Trimble, Rev. Mod. Phys. 60 (1988) 859-871.
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The Physics of supernova explosions, S. E. Woosley, T. A. Weaver, Ann. Rev. Astron. Astrophys. 24 (1986) 205.
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Supernovae. Part II: the aftermath, V. Trimble, Rev. Mod. Phys. 55 (1983) 511-563.
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Supernovae. Part I: the events, V. Trimble, Rev. Mod. Phys. 54 (1982) 1183-1224.
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The Weak Neutral Current and Its Effects in Stellar Collapse, Daniel Z. Freedman, David N. Schramm, David L. Tubbs, Ann. Rev. Nucl. Part. Sci. 27 (1977) 167-207.
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Synthesis of the Elements in Stars, E. Margaret Burbidge, G. R. Burbidge, William A. Fowler, F. Hoyle, Rev. Mod. Phys. 29 (1957) 547.
[Burbidge-Burbidge-Fowler-Hoyle-RMP29-547-1957]

3 - Reviews - Conference Proceedings

[3-1]
Supernovae in SuperK-Gd and other experiments, Lluis Marti-Magro, arXiv:1705.00675, 2017. NuPhys2016 (London, 12-14 December 2016).
[Marti-Magro:2017nbn]
[3-2]
The Core-Collapse Supernova Explosion Mechanism, B. Muller, arXiv:1702.06940, 2017.
[Muller:2017wgc]
[3-3]
Neutrino Astrophysics, Cristina Volpe, Acta Phys.Polon.Supp. 9 (2016) 769, arXiv:1609.06747. 52th Winter School of Theoretical Physics, Ladek Zdroj, 14-21 February 2016.
[Volpe:2016bkp]
[3-4]
Nuclear Physics and Astrophysics of Neutrino Oscillations, A.B. Balantekin, JPS Conf.Proc. 14 (2017) 010701, arXiv:1609.02207. NIC 2016.
[Balantekin:2016ndb]
[3-5]
Detection of Supernova Neutrinos, Ines Gil-Botella, arXiv:1605.02204, 2016. NuPhys2015 (London, 16-18 December 2015).
[Gil-Botella:2016sfi]
[3-6]
Supernova Neutrinos: Theory, Irene Tamborra, arXiv:1604.07332, 2016. NuPhys2015 (London, 16-18 December 2015).
[Tamborra:2016lpf]
[3-7]
Neutrino astrophysics : recent advances and open issues, Cristina Volpe, J. Phys. Conf. Ser. 631 (2015) 012048, arXiv:1503.01355. DISCRETE 2014.
[Volpe:2015yya]
[3-8]
Recent advances in neutrino astrophysics, Cristina Volpe, PoS FFP14 (2016) 127, arXiv:1411.6533. Frontiers of Fundamental Physics 2014, July 15-18, Marseille.
[Volpe:2014rca]
[3-9]
Current and Future Liquid Argon Neutrino Experiments, Georgia Karagiorgi, AIP Conf.Proc. 1663 (2015) 100001, arXiv:1304.2083. NuInt'12.
[Karagiorgi:2013cwa]
[3-10]
Review of Multi-messenger observations of neutron rich matter, C. J. Horowitz, arXiv:1212.6405, 2012. Xth Quark Confinement and the Hadron Spectrum, Munich.
[Horowitz:2012za]
[3-11]
Core-Collapse Supernovae, Neutrinos, and Gravitational Waves, C. D. Ott et al., Nucl. Phys. Proc. Suppl. 235-236 (2013) 381-387, arXiv:1212.4250. Neutrino 2012, Kyoto, Japan.
[Ott:2012jq]
[3-12]
Neutrino flavour conversion and supernovae, Cristina Volpe, AIP Conf.Proc. 1560 (2013) 306-313, arXiv:1210.0176. CIPANP 2012, May 29 to June 3, Florida.
[Volpe:2013cua]
[3-13]
Neutrinos and the stars, Georg Raffelt, Proc.Int.Sch.Phys.Fermi 182 (2012) 61-143, arXiv:1201.1637. ISAPP School 'Neutrino Physics and Astrophysics', 26 July-5 August 2011, Villa Monastero, Varenna, Italy.
[Raffelt:2012kt]
[3-14]
Neutrinos and core-collapse supernovae, Cristina Volpe, arXiv:1108.6285, 2011. XIV International Workshop on 'Neutrino Telescopes', March 15-18, 2011, Venice.
[Volpe:2011ff]
[3-15]
Physics and Astrophysics Opportunities with Supernova Neutrinos, Basudeb Dasgupta, PoS ICHEP2010 (2010) 294, arXiv:1005.2681. Electroweak Session of Rencontres de Moriond 2010.
[Dasgupta:2010gr]
[3-16]
Significance of neutrino cross-sections for astrophysics, A.B. Balantekin, AIP Conf. Proc. 1189 (2009) 11-15, arXiv:0909.0226. NUINT2009 (6th International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region), May 18-22, 2009, Sitges, Barcelona, Spain.
[Balantekin:2009qq]
[3-17]
Massive stars as thermonuclear reactors and their explosions following core collapse, Alak Ray, arXiv:0907.5407, 2009. Kodai School on Synthesis of Elements in Stars.
[Ray:2009xa]
[3-18]
Opportunities for Neutrino Physics at the Spallation Neutron Source (SNS), Yu Efremenko, W R Hix, J. Phys. Conf. Ser. 173 (2009) 012006, arXiv:0807.2801. 2008 Carolina International Symposium on Neutrino Physics.
[Efremenko:2008an]
[3-19]
Physics of Supernovae: theory, observations, unresolved problems, D. K. Nadyozhin, arXiv:0804.4350, 2008. Baikal Young Scientists' International School (BAYSIS), 17-22 September 2007, Irkutsk, Russia.
[Nadyozhin:2008is]
[3-20]
Neutrinos from a core collapse supernova, Amol Dighe, AIP Conf. Proc. 981 (2008) 75-79, arXiv:0712.4386. NuFact07.
[Dighe:2007ks]
[3-21]
Neutrino-driven explosions twenty years after SN1987A, H. -Th. Janka, A. Marek, F. -S. Kitaura, AIP Conf. Proc. 937 (2007) 144-154, arXiv:0706.3056. Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.
[Janka:2007yu]
[3-22]
Supernova neutrinos, Christian Y. Cardall, Nucl. Phys. Proc. Suppl. 168 (2007) 96-102, arXiv:astro-ph/0703334. NOW2006, Conca Specchiulla, Italy, September 9-16, 2006.
[Cardall:2007ha]
[3-23]
Supernova neutrino observations: What can we learn?, Georg G. Raffelt, Nucl. Phys. Proc. Suppl. 221 (2011) 218-229, arXiv:astro-ph/0701677. ]Neutrino 2006.
[Raffelt:2007nv]
[3-24]
Supernova neutrino detection, K. Scholberg, Nucl. Phys. Proc. Suppl. 221 (2011) 248-253, arXiv:astro-ph/0701081. Neutrino 2006, Santa Fe.
[Scholberg:2007nu]
[3-25]
Nuclear Astrophysics: CIPANP 2006, W. C. Haxton, AIP Conf. Proc. 870 (2006) 33-43, arXiv:nucl-th/0609006. CIPANP 2006.
[Haxton:2006ae]
[3-26]
Nucleosynthesis in neutrino heated matter: The vp-process and the r-process, G. Martinez-Pinedo et al., PoS NIC-IX (2006) 064, arXiv:astro-ph/0608490. NIC-IX, International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, CERN, Geneva, Switzerland, 25-30 June, 2006.
[MartinezPinedo:2006fk]
[3-27]
From progenitor to afterlife, Roger A. Chevalier, arXiv:astro-ph/0607422, 2006. 2006 STScI May Symposium on Massive Stars.
[Chevalier:2006af]
[3-28]
Supernova and GRB connection: Observations and Questions, Massimo Della Valle, AIP Conf. Proc. 836 (2006) 367-379, arXiv:astro-ph/0604110. 16th Annual October Astrophysics Conference in Maryland, 'Gamma Ray Bursts in the Swift Era'.
[DellaValle:2006yq]
[3-29]
The Cosmic Stellar Birth and Death Rates, John F. Beacom, New Astron. Rev. 50 (2006) 561-565, arXiv:astro-ph/0602101. Astronomy with Radioactivities V, Clemson Univ., Sept. 2005.
[Beacom:2006wz]
[3-30]
Supernovae Shedding Light on Gamma-Ray Bursts, M. Della Valle, Nuovo Cim. 28C (2005) 563, arXiv:astro-ph/0504517. 4th Workshop Gamma-Ray Bursts in the Afterglow Era, Rome,18-22 October 2004.
[DellaValle:2005cr]
[3-31]
High Redshift Supernovae: Cosmological Implications, Nino Panagia, Nuovo Cim. B120 (2005) 667, arXiv:astro-ph/0502247. Vulcano Workshop 2004, Frontier Objects in Astrophysics and Particle Physics.
[Panagia:2005hr]
[3-32]
Supernova neutrino challenges, Christian Y. Cardall, Nucl. Phys. Proc. Suppl. 145 (2005) 295, arXiv:astro-ph/0502232. NOW2004, Conca Specchiulla (Otranto, Italy), September 11-17, 2004.
[Cardall:2005zy]
[3-33]
Supernova Neutrino Oscillations, Georg G. Raffelt, Phys. Scripta T121 (2005) 102, arXiv:hep-ph/0501049. Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.
[Raffelt:2005fb]
[3-34]
Physics of Supernovae, Dmitrij K. Nadyozhin, V. S. Imshennik, Int. J. Mod. Phys. A20 (2005) 6597, arXiv:astro-ph/0501002. 19th European Cosmic Ray Symposium (ECRS 2004), Florence, Italy, 30 Aug - 3 Sep 2004.
[Nadyozhin:2005ji]
[3-35]
Supernova neutrino detection, M. Selvi, Nucl. Phys. Proc. Suppl. 145 (2005) 339-342.
[Selvi:2005ac]
[3-36]
Supernovae and Their Massive Star Progenitors, Alexei V. Filippenko, Publ.Astron.Soc.Pac. (2004), arXiv:astro-ph/0412029. Science Symposium on the Fate of the Most Massive Stars, Grand Teton National Park, Wyoming, 23-28 May 2004.
[Filippenko:2004mu]
[3-37]
Three-flavour effects and CP- and T-violation in neutrino oscillations, Evgeny Akhmedov, Phys. Scripta T121 (2005) 65, arXiv:hep-ph/0412029. Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.
[Akhmedov:2004ve]
[3-38]
The Supernovae Associated with Gamma-Ray Bursts, Thomas Matheson, ASP Conf.Ser. (2004), arXiv:astro-ph/0410668. Supernovae as Cosmological Lighthouses, Padua, 2004.
[Matheson:2004ge]
[3-39]
Stellar explosions: from supernovae to gamma-ray bursts, Konstantin Postnov, NATO Adv.Study Inst.Ser.C.Math.Phys.Sci. (2004) 95-117, arXiv:astro-ph/0410349. ISCRA 14th School Neutrinos and Explosive Events in the Universe, Erice, Italy, July 2004.
[Postnov:2004cn]
[3-40]
Kepler's Supernova Remnant: The view at 400 Years, W. P. Blair, ASP Conf.Ser. (2004), arXiv:astro-ph/0410081. 1604-2004: Supernovae as Cosmological Lighthouses.
[Blair:2004hy]
[3-41]
Spectropolarimetry of Core-Collapse Supernovae, Douglas C. Leonard, Alexei V. Filippenko, ASP Conf.Ser. (2004), arXiv:astro-ph/0409518. Supernovae as Cosmological Lighthouses, 16-19 June, Padua, Italy.
[Leonard:2004mi]
[3-42]
Supernova neutrinos: production, propagation and oscillations, Amol Dighe, Nucl. Phys. Proc. Suppl. 143 (2005) 449, arXiv:hep-ph/0409268. Neutrino 2004, Paris.
[Dighe:2004xy]
[3-43]
Neutrinos: '...annus mirabilis', A. Yu. Smirnov, arXiv:hep-ph/0402264, 2004. 2nd Int. Workshop on Neutrino oscillations in Venice (NOVE) December 3-5, 2003, Venice, Italy.
[Smirnov:2004ju]
[3-44]
Spectropolarimetric Observations of Supernovae, Alexei V. Filippenko, Douglas C. Leonard, arXiv:astro-ph/0312500, 2003. 3-D Signatures in Stellar Explosions, 10-13 June, 2003.
[Filippenko:2003cb]
[3-45]
A Review of X-ray Observations of Supernova Remnants, Jacco Vink, Nucl. Phys. Proc. Suppl. 132 (2004) 21, arXiv:astro-ph/0311406. The restless high energy universe, Amsterdam, May 2003.
[Vink:2003nf]
[3-46]
Neutrinos as astrophysical probes, F. Cavanna, M. L. Costantini, O. Palamara, F. Vissani, Surveys High Energ. Phys. 19 (2004) 35, arXiv:astro-ph/0311256. ICTP Summer School on Astroparticle Physics and Cosmology, Trieste, Italy, 17 June - 5 Jul 2002.
[Cavanna:2003fx]
[3-47]
Supernova Spectra, M. Turatto, Springer Proc.Phys. 99 (2005) 151-160, arXiv:astro-ph/0310837. IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.
[Turatto:2003bi]
[3-48]
Observations of Type Ia Supernovae, and Challenges for Cosmology, W. Li, A. V. Filippenko, Springer Proc.Phys. 99 (2005) 525-533, arXiv:astro-ph/0310529. IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.
[Li:2003mm]
[3-49]
The Infrared Supernova Rate, F. Mannucci, G. Cresci, R. Maiolino, M. Della Valle, Springer Proc.Phys. 99 (2005) 355-359, arXiv:astro-ph/0310210. IAU Colloquium 192: Supernovae (10 Years after SN1993J), Valencia, Spain, 22-26 Apr 2003.
[Mannucci:2003ty]
[3-50]
Evidence from Type Ia Supernovae for an Accelerating Universe and Dark Energy, A. V. Filippenko, arXiv:astro-ph/0307139, 2003.
[Filippenko:2003pr]
[3-51]
Neutrino Physics after KamLAND, Alexei Yu. Smirnov, arXiv:hep-ph/0306075, 2003. 4th Workshop on 'Neutrino Oscillations and their Origin' (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Smirnov.pdf.
[Smirnov:2003uu]
[3-52]
Cosmology with Supernovae, P. Ruiz-Lapuente, Astrophys. Space Sci. 290 (2004) 43, arXiv:astro-ph/0304108. JENAM 2002 (Porto, Portugal).
[RuizLapuente:2003cj]
[3-53]
Review on the Observed and Physical Properties of Core Collapse Supernovae, Mario Hamuy, arXiv:astro-ph/0301006, 2003. 2003 Aspen Summer Workshop on the Nuclear Physics of Core Collapse Supernovae, Aspen, Colorado, 26 May - 8 June 2003.
[Hamuy:2003xv]
[3-54]
Supernova Neutrinos and Particle-Physics Applications, G. Raffelt, 2003. Lectures given at ISAPP 2003 - International School on AstroParticle Physics, 14-19 July 2003, Madonna di Campiglio, Italy. http://wwwth.mppmu.mpg.de/members/raffelt/mytalks/ISAPP3.pdf.
[Raffelt:ISAPP2003]
[3-55]
Bolometric Light Curves of Supernovae, N. B. Suntzeff, arXiv:astro-ph/0212561, 2002. From Twilight to Highlight - The Physics of Supernovae ESO/MPA/MPE Workshop, Garching, July 29 - 31, 2002.
[Suntzeff:2002tc]
[3-56]
Type Ia Supernova models: latest developments, S. Blinnikov, E. Sorokina, Astrophys. Space Sci. 290 (2004) 13, arXiv:astro-ph/0212530. JENAM-2002 meeting (Porto, Portugal, September, 3-8).
[Blinnikov:2002gu]
[3-57]
Neutrinos from supernovae, Sandhya Choubey, Kamales Kar, Proc.Indian Natl.Sci.Acad. 70A (2004) 123, arXiv:hep-ph/0212326. INSA Proceedings.
[Choubey:2002hp]
[3-58]
Core Collapse and Then? The Route to Massive Star Explosions, H.-Th. Janka et al., arXiv:astro-ph/0212316, 2002. From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.
[Janka:2002ei]
[3-59]
Astrophysical and Cosmological Neutrinos, G. G. Raffelt, Proc.Int.Sch.Phys.Fermi 152 (2003) 161-181, arXiv:hep-ph/0208024. International School of Physics 'Enrico Fermi,' CLII Course 'Neutrino Physics,' 23 July-2 August 2002, Varenna, Lake Como, Italy.
[Raffelt:2002nz]
[3-60]
Neutrino masses in astroparticle physics, G. G. Raffelt, New Astron. Rev. 46 (2002) 699-708, arXiv:astro-ph/0207220. Dennis Sciama Memorial Volume of NAR.
[Raffelt:2002ed]
[3-61]
Neutrinos from supernovae: experimental status and perspectives, Fabrizio Cei, Int. J. Mod. Phys. A17 (2002) 1765-1776, arXiv:hep-ex/0202043. Second International Workshop on Matter, Anti-Matter and Dark Matter, Trento (Italy), 29-30 October 2001.
[Cei:2002mq]
[3-62]
Physics with supernovae, Georg. G. Raffelt, Nucl. Phys. Proc. Suppl. 110 (2012) 254-267, arXiv:hep-ph/0201099. TAUP 2001: Topics in Astroparticle and Underground Physics, Assergi, Italy, 8-12 Sep 2001.
[Das:2012zk]
[3-63]
Supernovae : Theory, expected Rates, Energy Spectrum, Flavor Composition, Time Structure, G. Raffelt, 2002. Workshop on Large Detectors for proton decay, supernovae, and atmospheric neutrinos, and low energy neutrinos from high intensity beams, NNN02, CERN, 16-18 January 2002. http://muonstoragerings.cern.ch/NuWorkshop02/presentations/raffelt.ppt.
[Raffelt-NNN02]
[3-64]
Supernova types and rates, E. Cappellaro, M. Turatto, Astrophys.Space Sci.Libr. 264 (2001) 199, arXiv:astro-ph/0012455. The Influence of Binaries on Stellar Population Studies, Brussels 21-25 Aug. 2000.
[Cappellaro:2000ez]
[3-65]
Supernova and Cosmology, M. Signore, D. Puy, New Astron. Rev. 45 (2001) 409, arXiv:astro-ph/0010634.
[Signore:2000mg]
[3-66]
Massive neutrinos in astrophysics, Georg G. Raffelt, Werner Rodejohann, arXiv:hep-ph/9912397, 1999. 4th National Summer School for German-speaking Graduate Students of Theoretical Physics, Saalburg, Germany, 31 Aug - 11 Sep 1998.
[Raffelt:1998qp]
[3-67]
Supernova 1987A - A review, Bhattacharya D., Bulletin of the Astronomical Society of India 16 (1988) 57-66. Astronomical Society of India, Meeting, 12th, Raipur, India, Dec. 1987.
[Bhattacharya-1988BASI-16-57B]
[3-68]
Supernova models, S. E. Woosley, T. A. Weaver, New York Academy Sciences Annals 375 (1981) 357-380.
[Woosley-Weaver-1981NYASA-375-357W]
[3-69]
Evolution and explosion of massive stars, S. E. Woosley, T. A. Weaver, Ninth Texas Symposium on Relativistic Astrophysics. 335-357 (1980).
[Weaver-Woosley-1980txra-symp-335W]

4 - PhD Theses

[4-1]
Detecting Fast Time Variations in the Supernova Neutrino Flux with Hyper-Kamiokande, Jost Migenda, arXiv:1609.04286, 2016.
[Migenda:2016xnc]
[4-2]
Neutrino interactions in neutron matter, Andrea Cipollone, arXiv:1212.5849, 2012.
[Cipollone:2012rb]
[4-3]
Supernovae as laboratories for neutrino properties, Andreu Esteban-Pretel, arXiv:0912.1616, 2009.
[EstebanPretel:2009ca]
[4-4]
Construction and Analysis of a Many-Body Neutrino model, Ivona Okuniewicz, arXiv:0903.2996, 2009.
[Okuniewicz:2006kz]
[4-5]
The Evolution of Low Mass Helium Stars towards Supernova Type I Explosion, Roni Waldman, Zalman Barkat, arXiv:astro-ph/0605692, 2006.
[Waldman:2006ge]
[4-6]
Supernova neutrino spectra and applications to flavor oscillations, Mathias Thorsten Keil, arXiv:astro-ph/0308228, 2003.
[Keil:2003sw]
[4-7]
A Search for Supernova Neutrinos with the Sudbury Neutrino Observatory, Jaret Heise, 2001. University of British Columbia, Vancouver BC, December 2001.
[Heise-PHD2001]

5 - Experiment - Type II

[5-1]
Detection of a Type IIn Supernova in Optical Follow-up Observations of IceCube Neutrino Events, M. G. Aartsen et al. (IceCube), Astrophys. J. 811 (2015) 52, arXiv:1506.03115.
[Aartsen:2015trq]
[5-2]
Implication on the core collapse supernova rate from 21 years of data of the Large Volume Detector, N.Y. Agafonova et al. (LVD), Astrophys.J. 802 (2015) 47, arXiv:1411.1709.
[Agafonova:2014leu]
[5-3]
Supernova Relic Neutrino Search with Neutron Tagging at Super-Kamiokande-IV, H. Zhang et al. (Super-Kamiokande), Astropart.Phys. 60 (2015) 41, arXiv:1311.3738.
[Zhang:2013tua]
[5-4]
Searching for soft relativistic jets in Core-collapse Supernovae with the IceCube Optical Follow-up Program, R. Abbasi et al. (IceCube), Astron. Astrophys. 539 (2012) A60, arXiv:1111.7030.
[Abbasi:2011ja]
[5-5]
Supernova Relic Neutrino Search at Super-Kamiokande, K. Bays et al. (Super-Kamiokande), Phys. Rev. D85 (2012) 052007, arXiv:1111.5031.
[Bays:2011si]
[5-6]
IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae, R. Abbasi et al. (IceCube), Astron. Astrophys. 535 (2011) A109, arXiv:1108.0171.
[Abbasi:2011ss]
[5-7]
Low Multiplicity Burst Search at the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Astrophys. J. 728 (2011) 83, arXiv:1011.5436.
[Collaboration:2010gx]
[5-8]
A Search for Core-Collapse Supernovae using the MiniBooNE Neutrino Detector, A. A. Aguilar-Arevalo et al. (MiniBooNE), Phys. Rev. D81 (2010) 032001, arXiv:0910.3182.
[AguilarArevalo:2009ju]
[5-9]
An Extremely Luminous X-ray Outburst Marking the Birth of a Normal Supernova, A. M. Soderberg et al., Nature. 453 (2008) 469-474, arXiv:0802.1712.
[Soderberg:2008uh]
[5-10]
Search for Supernova Neutrino Bursts at Super-Kamiokande, M. Ikeda, A. Takeda, Y. Fukuda, M. R. Vagins, M. Sakuda (Super-Kamiokande), Astrophys. J. 669 (2007) 519-524, arXiv:0706.2283.
[Ikeda:2007sa]
[5-11]
A Search for Neutrinos from the Solar hep Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory, B. Aharmim et al. (SNO), Astrophys. J. 653 (2006) 1545-1551, arXiv:hep-ex/0607010.
[Aharmim:2006wq]
[5-12]
Gamma-Ray Burst associated Supernovae: Outliers become Mainstream, E. Pian et al., Nature 442 (2006) 1011-1013, arXiv:astro-ph/0603530.
[Pian:2006pr]
[5-13]
Discovery of 35 New Supernova Remnants in the Inner Galaxy, C. L. Brogan et al., Astrophys. J. 639 (2006) L25, arXiv:astro-ph/0601451.
[Brogan:2006tv]
[5-14]
Echoes from Ancient Supernovae in the Large Magellanic Cloud, A. Rest et al., Nature (2005), arXiv:astro-ph/0510738.
[Rest:2005un]
[5-15]
Discovery of X-Ray Emission from Supernova 1970G with Chandra: Filling the Void between Supernovae and Supernova Remnants, Stefan Immler, K. D. Kuntz, Astrophys. J. 632 (2005) L99, arXiv:astro-ph/0506023.
[Immler:2005ym]
[5-16]
Late-time X-Ray, UV and Optical Monitoring of Supernova 1979C, Stefan Immler et al., Astrophys. J. 632 (2005) 283, arXiv:astro-ph/0503678.
[Immler:2005vx]
[5-17]
Hubble Space Telescope imaging of the progenitor sites of six nearby core-collapse supernovae, Justyn R. Maund, Stephen J. Smartt, Mon. Not. Roy. Astron. Soc. 360 (2005) 288, arXiv:astro-ph/0501323.
[Maund:2005nq]
[5-18]
SN Ib 1990I: Clumping and Dust in the Ejecta?, Abouazza Elmhamdi et al., Astron. Astrophys. 426 (2004) 963-977, arXiv:astro-ph/0407145.
[Elmhamdi:2004he]
[5-19]
SNEWS: The SuperNova Early Warning System, P. Antonioli et al., New J. Phys. 6 (2004) 114, arXiv:astro-ph/0406214.
[Antonioli:2004zb]
[5-20]
The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope, Nikolai N. Chugai et al., Mon. Not. Roy. Astron. Soc. 352 (2004) 1213, arXiv:astro-ph/0405369.
[Chugai:2004gq]
[5-21]
XMM-Newton observation of Kepler's supernova remnant, G. Cassam-Chenai et al., Astron.Astrophys. (2003), arXiv:astro-ph/0310687.
[CassamChenai:2003ft]
[5-22]
Twenty Years of Galactic Observations in Searching for Bursts of Collapse Neutrinos with the Baksan Underground Scintillation Telescope, E.N.Alexeyev, L.N.Alexeyeva, J. Exp. Theor. Phys. 95 (2002) 5, arXiv:astro-ph/0212499.
[Alekseev:2002ji]
[5-23]
Search for supernova relic neutrinos at Super-Kamiokande, M. Malek et al. (Super-Kamiokande), Phys. Rev. Lett. 90 (2003) 061101, arXiv:hep-ex/0209028.
[Malek:2002ns]
[5-24]
The Asiago Supernova Catalogue - 10 years after, R. Barbon, V. Buondi, E. Cappellaro, M. Turatto, Astron. Astrophys. 139 (1999) 531-536.
[Asiago-Supernova-Catalogue-AA139-1999]

6 - Experiment - Type II - Conference Proceedings

[6-1]
Improved Detection of Supernovae with the IceCube Observatory, Lutz Kopke (IceCube), arXiv:1704.03823, 2017. 8th international symposium on large TPCs for low-energy rare event detection, Paris, Dec. 5-7, 2016.
[Kopke:2017req]
[6-2]
The core collapse supernova rate from 24 years of data of the Large Volume Detector, G. Bruno, A. Molinario, W. Fulgione, C. Vigorito (LVD), arXiv:1701.06765, 2017. XXV ECRS 2016.
[Bruno:2017oxg]
[6-3]
The IceCube Neutrino Observatory Part V: Neutrino Oscillations and Supernova Searches, M. G. Aartsen et al. (IceCube), arXiv:1309.7008, 2013. 33nd International Cosmic Ray Conference, Rio de Janeiro 2013.
[Aartsen:2013nla]
[6-4]
Supernova Detection in IceCube: Status and Future, Ronald Bruijn (IceCube), Nucl. Phys.B, Proc.Suppl.237-238 2013 (2013) 94-97, arXiv:1302.2040. NOW 2012.
[Bruijn:2013ibl]
[6-5]
The IceCube Neutrino Observatory VI: Neutrino Oscillations, Supernova Searches, Ice Properties, R. Abbasi et al. (IceCube), arXiv:1111.2731, 2011. 32nd International Cosmic Ray Conference, Beijing 2011.
[Abbasi:2011eva]
[6-6]
Low Energy Neutrino Astronomy in Super-Kamiokande, Michael Smy, arXiv:1110.0012, 2011. DPF 2011.
[Smy:2011tm]
[6-7]
Search for neutrino bursts from core collapse supernovae at the Baksan Underground Scintillation Telescope, R.V. Novoseltseva et al., arXiv:0910.0738, 2009. 31 International Cosmic Ray Conference, Lodz, Poland, July 7-15, 2009.
[Novoseltseva:2009cr]
[6-8]
Supernova Search with the AMANDA / IceCube Detectors, Thomas Kowarik, Timo Griesel, Alexander Piegsa (Icecube), arXiv:0908.0441, 2009. 31st ICRC, Lodz, Poland, July 2009.
[Kowarik:2009qr]
[6-9]
Search for High Energetic Neutrinos from Supernova Explosions with AMANDA, Dirk Lennarz, Jan-Patrick Huls, Christopher Wiebusch (IceCube), arXiv:0907.4621, 2009. 31st ICRC, Lodz, Poland, July 2009.
[Lennarz:2009xr]
[6-10]
Recent Type II Radio Supernovae, Christopher J. Stockdale et al., AIP Conf. Proc. 937 (2007) 264-268, arXiv:0708.1182. Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.
[Stockdale:2007pe]
[6-11]
LVD highlights, Marco Selvi et al. (LVD), arXiv:hep-ex/0608061, 2006. Vulcano Workshop 2006 'Frontier Objects in Astrophysics and Particle Physics'.
[Selvi:2006bi]
[6-12]
SNLS - the Supernova Legacy Survey, C.J. Pritchet, SNLS (SNLS), ASP Conf.Ser. (2004), arXiv:astro-ph/0406242. Observing Dark Energy (NOAO/Tucson proceedings).
[Pritchet:2004af]
[6-13]
Evidence for Core Collapse in the Type Ib/c SN 1999ex, Mario Hamuy et al., arXiv:astro-ph/0212368, 2002. From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.
[Hamuy:2002rz]
[6-14]
The dusty type IIn Supernova 1998S, Peter Meikle et al., arXiv:astro-ph/0211144, 2002. ESO/MPA/MPE Workshop 'From Twilight to Highlight: The Physics of Supernovae', Garching, Germany, 29-31 July 2002.
[Meikle:2002dn]
[6-15]
A Search for Core-Collapse Supernova Progenitors In Hubble Space Telescope Images, Schuyler D. Van Dyk, Weidong Li, Alexei V. Filippenko, Publ.Astron.Soc.Pac. (2002), arXiv:astro-ph/0210347. PASP (2003 Jan).
[VanDyk:2002ry]
[6-16]
An Intermediate Redshift Supernova Search at ESO: Reduction Tools and Efficiency Tests, M. Riello et al., arXiv:astro-ph/0210265, 2002. ESO/MPA/MPE Workshop 'From Twilight to Highlight, The Physics of Supernovae', Garching, Jul 29-31, 2002.
[Riello:2002hm]
[6-17]
Search for double degenerate progenitors of supernovae type Ia with SPY, R. Napiwotzki, H. Drechsel, U. Heber, C. Karl, E.-M. Pauli et al., others, others, others, others, others, others, others, others, others, others, arXiv:astro-ph/0210155, 2002. 'White Dwarfs', Proc. XIII Workshop on White Dwarfs.
[Napiwotzki:2002sa]

7 - Experiment - Type Ia

[7-1]
Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey, A. Rest et al., Astrophys.J. 795 (2014) 44, arXiv:1310.3828.
[Rest:2013mwz]
[7-2]
Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample, D. Scolnic et al., Astrophys.J. 795 (2014) 45, arXiv:1310.3824.
[Scolnic:2013efb]
[7-3]
The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae, Gaston Folatelli et al., Astron. J. 139 (2010) 120-144, arXiv:0910.3317.
[Folatelli:2009nm]
[7-4]
Asymmetric Explosion of Type Ia Supernovae as Seen from Near Infrared Observations, K. Motohara et al., Astrophys. J. 652 (2006) L101-L104, arXiv:astro-ph/0610303.
[Motohara:2006tg]
[7-5]
The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey, A. Conley et al. (SNLS), Astron. J. 132 (2006) 1707-1713, arXiv:astro-ph/0607363.
[Conley:2006tw]
[7-6]
Nonlinear Decline-Rate Dependence and Intrinsic Variation of Type Ia Supernova Luminosities, Lifan Wang et al., Astrophys. J. 641 (2006) 50-69, arXiv:astro-ph/0512370.
[Wang:2005bw]
[7-7]
The Supernova Legacy Survey: Measurement of $\Omega_\text{M}$, $\Omega_{\Lambda}$ and $w$ from the First Year Data Set, P. Astier et al. (SNLS), Astron. Astrophys. 447 (2006) 31, arXiv:astro-ph/0510447.
From the abstract: With this data set, we have built a Hubble diagram extending to $z=1$, with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: $ \Omega_{\text{M}} = 0.263 \pm 0.042 \pm 0.032 $ for a flat $\Lambda\text{CDM}$; and $w = -1.023 \pm 0.090 \pm 0.054 $ for a flat cosmology with constant equation of state $w$ when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations.
[Astier:2005qq]
[7-8]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications, A. Clocchiatti et al. (High Z SN Search), Astrophys. J. 642 (2006) 1-21, arXiv:astro-ph/0510155.
[Clocchiatti:2005vy]
[7-9]
Spectroscopy of twelve Type Ia supernovae at intermediate redshift, C. Balland et al., Astron.Astrophys. (2005), arXiv:astro-ph/0507703.
[Balland:2005rw]
[7-10]
First results from the Canada-France High-z Quasar Survey: Constraints on the z=6 quasar luminosity function and the quasar contribution to reionization, Chris J. Willott et al., Astrophys. J. 633 (2005) 630, arXiv:astro-ph/0507183.
[Willott:2005zr]
[7-11]
Evidence for Spectropolarimetric Diversity in Type Ia Supernovae, Douglas C. Leonard et al., Astrophys. J. 632 (2005) 450, arXiv:astro-ph/0506470.
[Leonard:2005td]
[7-12]
A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex, R. J. Foley et al., Astrophys. J. 626 (2005) L11, arXiv:astro-ph/0504481.
[Foley:2005qu]
[7-13]
Restframe I-band Hubble diagram for type Ia supernovae up to redshift $z \sim 0.5$, Serena Nobili et al. (Supernova Cosmology Project), Astron.Astrophys. (2005), arXiv:astro-ph/0504139.
[Nobili:2005tr]
[7-14]
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant, Adam G. Riess et al., Astrophys. J. 627 (2005) 579, arXiv:astro-ph/0503159.
From the abstract: $H_0 = 73 +\pm 4 \pm 5 \, \text{km} \, \text{s}^{-1} \, \text{Mps}^{-1}$.
[Riess:2005zi]
[7-15]
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey, Louis-Gregory Strolger, Adam G. Riess, Astron. J. 131 (2006) 1629-1638, arXiv:astro-ph/0503093.
[Strolger:2005uk]
[7-16]
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT, C. Lidman et al. (Supernova Cosmology Project), Astron.Astrophys. (2004), arXiv:astro-ph/0410506.
[Lidman:2004en]
[7-17]
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models, L. G. Strolger et al., Astrophys. J. 613 (2004) 200-223, arXiv:astro-ph/0406546.
[Strolger:2004kk]
[7-18]
Type Ia supernova rate at a redshift of ~ 0.1, Guillaume Blanc et al. (EROS), Astron. Astrophys. 423 (2004) 881, arXiv:astro-ph/0405211.
[Blanc:2004ws]
[7-19]
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa, Gabriele Garavini et al. (The Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 356 (2004) 456, arXiv:astro-ph/0404393.
[Garavini:2004fa]
[7-20]
Type Ia Supernova Discoveries at z > 1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution, Adam G. Riess et al. (Supernova Search Team), Astrophys. J. 607 (2004) 665, arXiv:astro-ph/0402512.
From the abstract: We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration.
...
A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99\% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at $z=0.46 \pm 0.13$.
The data are consistent with the cosmic concordance model of $\Omega_M \approx 0.3, \Omega_\Lambda \approx 0.7$ ($\chi^2_{dof}=1.06$), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy.
For a flat Universe with a cosmological constant, we measure $\Omega_M = 0.29 {}^{+0.05}_{-0.03}$ (equivalently, $\Omega_\Lambda=0.71$). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find $w = -1.02 {}^{+0.13}_{-0.19}$ (and $w<-0.76$ at the 95\% confidence level) for an assumed static equation of state of dark energy, $P = w\rho c^2$.
...
Our constraints are consistent with the static nature of and value of $w$ expected for a cosmological constant (i.e., $w_0 = -1.0$, $dw/dz = 0$), and are inconsistent with very rapid evolution of dark energy.

[Ivanov:2004qa]
[7-21]
23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at $z > 0.7$, Brian J. Barris et al., Astrophys. J. 602 (2004) 571, arXiv:astro-ph/0310843.
From the abstract: This sample of 23 high-redshift supernovae includes 15 at $z\geq0.7$, doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry and others (2003), we calculate cosmological parameter density contours which are consistent with the flat universe indicated by the CMB [Go]. Adopting the constraint that $\Omega_{total} = 1.0$, we obtain best-fit values of ($\Omega_{m}$,$\Omega_{\Lambda}$)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation.
[Barris:2003dq]
[7-22]
New Constraints on $\Omega_M$, $\Omega_\Lambda$, and $w$ from an Independent Set of Eleven High-Redshift Supernovae Observed with HST, Robert A. Knop et al. (The Supernova Cosmology Project), Astrophys. J. 598 (2003) 102, arXiv:astro-ph/0309368.
From the abstract: We report measurements of $\Omega_{\mathrm{M}}$, $\Omega_{\Lambda}$, and $w$ from eleven supernovae at $z=0.36$-$0.86$ with high-quality lightcurves measured using WFPC2 on the HST. This is an independent set of high-redshift supernovae that confirms previous supernova evidence for an accelerating Universe. The high-quality lightcurves available from photometry on \wfpc\ make it possible for these eleven supernovae alone to provide measurements of the cosmological parameters comparable in statistical weight to the previous results. Combined with earlier Supernova Cosmology Project data, the new supernovae yield a measurement of the mass density $\Omega_{\mathrm{M}}=0.25^{+0.07}_{-0.06}$ (statistical) $\pm0.04$ (identified systematics), or equivalently, a cosmological constant of $\Omega_{\Lambda}=0.75^{+0.06}_{-0.07}$ (statistical) $\pm0.04$ (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value $w=-1$. When the supernova results are combined with independent flat-universe measurements of $\Omega_{\mathrm{M}}$ from CMB and galaxy redshift distortion data, they provide a measurement of $w=-1.05^{+0.15}_{-0.20}$ (statistical) $\pm0.09$ (identified systematic), if $w$ is assumed to be constant in time.... dark energy is required with $P(\Omega_{\Lambda}>0)>0.99$.
[Knop:2003iy]
[7-23]
Cosmological Results from High-z Supernovae, John L. Tonry et al. (Supernova Search Team), Astrophys. J. 594 (2003) 1, arXiv:astro-ph/0305008.
From the abstract: The High-$ z$ Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval $ z=0.3-1.2$. These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to $ z\approx 1$, where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is $ w=-1$, then $ H_0\,t_0 = 0.96\pm0.04$, and $ \Omega_\Lambda-1.4\Omega_M=0.35\pm0.14$. Including the constraint of a flat Universe, we find $ \Omega_M=0.28\pm0.05$, independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on $ \Omega_M$ and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range $ -1.48-1$, we obtain $ w<-0.73$ at 95% confidence.
[Tonry:2003zg]
[7-24]
SN 2002cx: The Most Peculiar Known Type Ia Supernova, Weidong Li et al., Publ. Astron. Soc. Pac. 115 (2003) 453-473, arXiv:astro-ph/0301428.
[Li:2003wja]
[7-25]
Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el, Kevin Krisciunas et al., Astron. J. 125 (2003) 166, arXiv:astro-ph/0210327.
[Krisciunas:2002rc]
[7-26]
The Type la Supernova 2001V in NGC 3987, J. Vinko et al., Astron. Astrophys. 397 (2003) 115, arXiv:astro-ph/0210186.
[Vinko:2002pa]
[7-27]
The distant Type Ia supernova rate, R. Pain et al. (Supernova Cosmology Project), Astrophys. J. 577 (2002) 120, arXiv:astro-ph/0205476.
[Pain:2002wj]
[7-28]
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration, Adam G. Riess et al. (Supernova Search Team), Astrophys. J. 560 (2001) 49-71, arXiv:astro-ph/0104455.
[Riess:2001gk]
[7-29]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae, S. Perlmutter et al. (Supernova Cosmology Project), Astrophys. J. 517 (1999) 565-586, arXiv:astro-ph/9812133.
From the abstract: The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation $0.8 \,\Omega_{\rm M}- 0.6\,\Omega_\Lambda \approx -0.2 \pm 0.1$ in the region of interest ($\Omega_{\rm M} \lesssim 1.5$). For a flat ($\Omega_{\rm M}+\Omega_\Lambda = 1$) cosmology we find $\Omega_{\rm M}^{\rm flat} = 0.28^{+0.09}_{-0.08}$ (1$\sigma$ statistical) $^{+0.05}_{-0.04}$ (identified systematics). The data are strongly inconsistent with a $\Lambda = 0$ flat cosmology, the simplest inflationary universe model. An open, $\Lambda = 0$ cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of $P(\Lambda > 0) = 99$\%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is $t_0^{\rm flat}=14.9^{+1.4}_{-1.1}\,(0.63/h)$ Gyr for a flat cosmology.
[Perlmutter:1998np]
[7-30]
Supernova Limits on the Cosmic Equation of State, Peter M. Garnavich et al. (Supernova Search Team), Astrophys. J. 509 (1998) 74-79, arXiv:astro-ph/9806396.
[Garnavich:1998th]
[7-31]
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Adam G. Riess et al. (Supernova Search Team), Astron. J. 116 (1998) 1009-1038, arXiv:astro-ph/9805201.
[Riess:1998cb]

8 - Experiment - Type Ia - Conference Proceedings

[8-1]
Exploring the Physics of Type Ia Supernovae Through the X-ray Spectra of their Remnants, C. Badenes et al., Mem.Soc.Ast.It. (2005), arXiv:astro-ph/0506576. "Stellar end products" workshop, 13-15 April 2005, Granada, Spain.
[Badenes:2005kx]
[8-2]
The Fall 2004 SDSS Supernova Survey, Masao Sako et al. (The SDSS), eConf C041213 (2004) 1424, arXiv:astro-ph/0504455. 22nd Texas Symposium on Relativistic Astrophysics.
[Sako:2005ps]

9 - Experiment - Type II - Supernova Remnant

[9-1]
A 'Missing' Supernova Remnant revealed by the 21-cm Line of Atomic Hydrogen, B-C Koo, J-h Kang, C.J. Salter, Astrophys. J. 643 (2006) L49-L52, arXiv:astro-ph/0604186.
[Koo:2006sr]

10 - Experiment - Type II - SN1987A

[10-1]
Time evolution of the line emission from the inner circumstellar ring of SN 1987A and its hot spots, Per Groeningsson et al., Astron.Astrophys. 492 (2008) 481, arXiv:0810.2661.
[Groeningsson:2008nc]
[10-2]
Chandra HETG Spectra of SN 1987A at 20 years, D. Dewey, S. A. Zhekov, R. McCray, C. R. Canizares, Astrophys.J. 676 (2008) L131, arXiv:0802.2340.
[Dewey:2008gy]
[10-3]
Infrared Integral Field Spectroscopy of SN 1987A, Karina Kjaer et al., AIP Conf. Proc. 937 (2007) 76-80, arXiv:astro-ph/0703720.
[Kjaer:2007wx]
[10-4]
Discovery of a nearby twin of SN1987A's nebula around the luminous blue variable HD168625: Was Sk-69 202 an LBV?, Nathan Smith, Astron. J. 133 (2007) 1034-1040, arXiv:astro-ph/0611544.
[Smith:2006es]
[10-5]
On the Progenitor of Supernova 1987A, M. Parthasarathy, David Branch, E. Baron, David J. Jeffery, Bull.Astron.Soc.India (2006), arXiv:astro-ph/0611033.
[Parthasarathy:2006jr]
[10-6]
Evolutionary Status of SNR 1987A at the Age of Eighteen, Sangwook Park et al., Astrophys. J. 646 (2006) 1001-1008, arXiv:astro-ph/0604201.
[Park:2006tg]
[10-7]
Coronal emission from the shocked circumstellar ring of SN 1987A, Per Groningsson et al., Astron.Astrophys. (2006), arXiv:astro-ph/0603815.
[Groningsson:2006cb]
[10-8]
SN 1987A After 18 Years: Mid-Infrared GEMINI and SPITZER Observations of the Remnant, Patrice Bouchet et al., Astrophys. J. 650 (2006) 212-227, arXiv:astro-ph/0601495.
[Bouchet:2006ff]
[10-9]
The reverse shock of SNR1987A at 18 years after outburst, Nathan Smith et al., Astrophys. J. 635 (2005) L41, arXiv:astro-ph/0510835.
[Smith:2005gu]
[10-10]
Supernova Remnant 1987A: Opening the Future by Reaching the Past, Sangwook Park, Svetozar A. Zhekov, David N. Burrows, Richard McCray, Astrophys. J. 634 (2005) L73, arXiv:astro-ph/0510442.
[Park:2005qj]
[10-11]
Imaging of the Radio Remnant of SN 1987A at 12 mm Wavelength, R. N. Manchester et al., Astrophys. J. 628 (2005) L131, arXiv:astro-ph/0506475.
[Manchester:2005ti]
[10-12]
Chandra Observations of Shock Kinematics in Supernova Remnant 1987A, S.A. Zhekov et al., Astrophys. J. 628 (2005) L127, arXiv:astro-ph/0506443.
[Zhekov:2005ni]
[10-13]
Limits from the Hubble Space Telescope on a Point Source in SN 1987A, G. J. M. Graves et al., Astrophys. J. 629 (2005) 944, arXiv:astro-ph/0505066.
[Graves:2005xy]
[10-14]
A New View of the Circumstellar Environment of SN 1987A, Ben E. K. Sugerman et al., Astrophys. J. 627 (2005) 888, arXiv:astro-ph/0502268.
[Sugerman:2005dk]
[10-15]
Supernova Remnant 1987A: The Latest Report from the Chandra X-Ray Observatory, Sangwook Park et al., Adv. Space Res. 35 (2005) 991-995, arXiv:astro-ph/0501561.
[Park:2005ic]
[10-16]
Constraints on the luminosity of the stellar remnant in SNR1987A, P. Shtykovskiy, A. Lutovinov, M. Gilfanov, R. Sunyaev, Astron. Lett. 31 (2005) 258, arXiv:astro-ph/0411731.
[Shtykovskiy:2004uj]
[10-17]
High Resolution Imaging of SN 1987A at 10 micron, P. Bouchet et al., Astrophys. J. 611 (2004) 394, arXiv:astro-ph/0312240.
[Bouchet:2003ng]
[10-18]
The X-ray Remnant of SN1987A, David N. Burrows et al., Astrophys. J. 543 (2000) L149-L152, arXiv:astro-ph/0009265.
[Burrows:2000yi]
[10-19]
Young Stellar Populations Around SN1987A, Nino Panagia, Martino Romaniello, Salvatore Scuderi, Robert P. Kirshner, Astrophys. J. 539 (2000) 197-208, arXiv:astro-ph/0001476.
[Panagia:2000ga]
[10-20]
A Second Bright Source Detected Near SN1987A, Peter Nisenson, Costas Papaliolios, Astrophys.J. 518 (1999) L29, arXiv:astro-ph/9904109.
[Nisenson:1999qd]
[10-21]
The X-ray lightcurve of SN 1987A, G. Hasinger, B. Aschenbach, J. Trumper, Astron. Astrophys. 312 (1996) L9-L12, arXiv:astro-ph/9606149.
[Hasinger:1996rj]
[10-22]
The progenitor of SN 1987A - Spatially resolved ultraviolet spectroscopy of the supernova field, George Sonneborn, Bruce Altner, Robert P. Kirshner, Astrophys. J. 323 (1987) L35-L39.
[Kirshner-ApJ323-1987]
[10-23]
Ultraviolet observations of SN 1987A, Robert P. Kirshner, George Sonneborn, D. Michael Crenshaw, George E. Nassiopoulos, Astrophys. J. 320 (1987) 602-608.
[Kirshner-ApJ320-1987]

11 - Experiment - Type II - SN1987A - Conference Proceedings

[11-1]
SN1987A: Revisiting the Data and the Correlation between Neutrino and Gravitational Detectors, P. Galeotti, G. V. Pallottino, G. Pizzella, arXiv:0810.3759, 2008. Vulcano Wokshop 2008, Frontier Objects in Astrophysics and Particle Physics, May 26-31.
[Galeotti:2008wc]
[11-2]
Chandra Observations of Supernova 1987A, Sangwook Park et al., AIP Conf. Proc. 937 (2007) 43-50, arXiv:0704.0209. Supernova 1987A: 20 Years after Supernovae and Gamma-Ray Bursters, Aspen, CO, USA, Feb 19-23, 2007.
[Park:2007nr]
[11-3]
Supernova Remnant 1987A: High Resolution Images and Spectrum from Chandra Observations, Sangwook Park et al., ESA Spec.Publ. 604 (2006) 335, arXiv:astro-ph/0511355. The X-Ray Universe 2005, Sept 26-30, 2005, El Escorial, Madrid, Spain.
[Park:2005vu]
[11-4]
A 2.14 ms Candidate Optical Pulsar in SN1987A, J. Middleditch et al., arXiv:astro-ph/0010044, 2000. 5th CTIO/ESO Workshop and 1st CTIO/ESO/LCO Workshop: SN 1987A: Ten Years After, La Serena, Chile, 22-28 Feb 1997.
[Middleditch:2000it]

12 - Experiment - Type II - SN1987A - Baksan

[12-1]
DETECTION OF THE NEUTRINO SIGNAL FROM SN1987A IN THE LMC USING THE INR BAKSAN UNDERGROUND SCINTILLATION TELESCOPE, E. N. Alekseev, L. N. Alekseeva, I. V. Krivosheina, V. I. Volchenko, Phys. Lett. B205 (1988) 209-214.
[Alekseev:1988gp]
[12-2]
CHARACTERISTICS OF THE NEUTRINO EMISSION FROM SUPERNOVA SN1987A, A. E. Chudakov, Ya. S. Elensky, S. P. Mikheev, JETP Lett. 46 (1987) 373-377. [Pisma Zh. Eksp. Teor. Fiz. 46, 297 (1987)].
[Chudakov:1987my]
[12-3]
POSSIBLE DETECTION OF A NEUTRINO SIGNAL ON 23 FEBRUARY 1987 AT THE BAKSAN UNDERGROUND SCINTILLATION TELESCOPE OF THE INSTITUTE OF NUCLEAR RESEARCH, E. N. Alekseev, L. N. Alekseeva, V. I. Volchenko, I. V. Krivosheina, JETP Lett. 45 (1987) 589-592. [Pisma Zh. Eksp. Teor. Fiz. 45, 461-464 (1987)].
[Alekseev:1987ej]

13 - Experiment - Type II - SN1987A - IMB

[13-1]
NEUTRINOS FROM SN1987A IN THE IMB DETECTOR, J. C. Van Der Velde et al. (IMB), Nucl. Instrum. Meth. A264 (1988) 28-31.
[VanDerVelde:1988hh]
[13-2]
ANGULAR DISTRIBUTION OF EVENTS FROM SN1987A, C. B. Bratton et al. (IMB), Phys. Rev. D37 (1988) 3361.
[Bratton:1988ww]
[13-3]
OBSERVATION OF A NEUTRINO BURST IN COINCIDENCE WITH SUPERNOVA SN1987A IN THE LARGE MAGELLANIC CLOUD, R. M. Bionta et al. (IMB), Phys. Rev. Lett. 58 (1987) 1494.
[Bionta:1987qt]

14 - Experiment - Type II - SN1987A - Kamiokande

[14-1]
Observation in the Kamiokande-II detector of the neutrino burst from supernova SN1987A, K. S. Hirata et al. (Kamiokande), Phys. Rev. D38 (1988) 448-458.
[Hirata:1988ad]
[14-2]
A search for high-energy neutrinos from SN1987a: first six months, Y. Oyama et al. (Kamiokande), Phys. Rev. Lett. 59 (1987) 2604.
[Oyama:1987aw]
[14-3]
Observation of a neutrino burst from the supernova SN1987a, K. Hirata et al. (Kamiokande), Phys. Rev. Lett. 58 (1987) 1490-1493.
[Hirata:1987hu]

15 - Experiment - Type II - SN1987A - LSD

[15-1]
Correlations between low-energy and high-energy pulses detected by the LSD installation under Mt. Blanc from 10 February 1987 to 1 July 1987, V. L. Dadykin et al., JETP Lett. 56 (1992) 426-429.
[Dadykin:1992yi]
[15-2]
Correlations of the low-energy pulses and muons recorded at the Mont Blanc LSD apparatus between 10 February and 1 July 1987, V. L. Dadykin et al., Bull. Russ. Acad. Sci. Phys. 55 (1991) 4129.
[Dadykin:1991sq]
[15-3]
Coincidences among the data recorded by the Baksan, Kamioka and Mont Blanc underground neutrino detectors, and by the Maryland and Rome gravitational wave detectors during supernova SN1987A, M. Aglietta et al., Nuovo Cim. C14 (1991) 171-193.
[Aglietta:1991im]
[15-4]
Correlation between the Maryland and Rome gravitational wave detectors and the Mont Blanc, Kamioka and IMB particle detectors during SN1987A, M. Aglietta et al., Nuovo Cim. B106 (1991) 1257-1269.
[Aglietta:1991xa]
[15-5]
Neutrino astrophysics and SN1987A, M. Aglietta et al., Nuovo Cim. C13 (1990) 365-374.
[Aglietta:1990sw]
[15-6]
ANALYSIS OF THE DATA RECORDED BY THE MONT BLANC NEUTRINO DETECTOR AND BY THE MARYLAND AND ROME GRAVITATIONAL WAVE DETECTORS DURING SN1987A, M. Aglietta et al., Nuovo Cim. C12 (1989) 75-103.
[Aglietta:1989tw]
[15-7]
NEUTRINO OBSERVATIONS FROM SUPERNOVA SN1987A, P. Galeotti et al., Helv. Phys. Acta 60 (1987) 619-628.
[Galeotti:1987kw]
[15-8]
DETECTION OF A RARE EVENT ON 23 FEBRUARY 1987 BY THE NEUTRINO RADIATION DETECTOR UNDER MONT BLANC, V. L. Dadykin et al., JETP Lett. 45 (1987) 593-595.
[Dadykin:1987ek]

16 - Phenomenology - Type II

[16-1]
Diffuse neutrino supernova background as a cosmological test, J. Barranco, Argelia Bernal, D. Delepine, arXiv:1706.03834, 2017.
[Barranco:2017lug]
[16-2]
Constraining high-energy neutrino emission from choked jets in stripped-envelope supernovae, Nicholas Senno, Kohta Murase, Peter Meszaros, arXiv:1706.02175, 2017.
[Senno:2017vtd]
[16-3]
Supernovae in compact star clusters as sources of high-energy cosmic rays and neutrinos, A. M. Bykov, D. C. Ellison, P. E. Gladilin, S. M. Osipov, arXiv:1706.01135, 2017.
[Bykov:2017fik]
[16-4]
Supernova Neutrino in a Strangeon Star Model, Mao Yuan, Jiguang Lu, Zhiliang Yang, Xiaoyu Lai, Renxin Xu, arXiv:1705.08188, 2017.
[Yuan:2017yql]
[16-5]
Point-source and diffuse high-energy neutrino emission from Type IIn supernovae, Maria Petropoulou, Stefan Coenders, Georgios Vasilopoulos, Atish Kamble, Lorenzo Sironi, arXiv:1705.06752, 2017.
[Petropoulou:2017ymv]
[16-6]
Detecting High-Energy Neutrinos from the Next Galactic Supernova, Kohta Murase, arXiv:1705.04750, 2017.
[Murase:2017pfe]
[16-7]
Diffuse neutrinos from luminous and dark supernovae: prospects for upcoming detectors at the O(10) kt scale, Alankrita Priya, Cecilia Lunardini, arXiv:1705.02122, 2017.
[Priya:2017bmm]
[16-8]
Neutrino emissions in all flavors up to the pre-bounce of massive stars and the possibility of their detections, Chinami Kato et al., arXiv:1704.05480, 2017.
[Kato:2017ehj]
[16-9]
Neutrino intensity interferometry: Measuring proto-neutron star radii during core-collapse supernovae, Warren P. Wright, James P. Kneller, arXiv:1704.00010, 2017.
[Wright:2017jwl]
[16-10]
The Nickel Mass Distribution of Normal Type II Supernovae, Tomas Muller, Jose L. Prieto, Ondrej Pejcha, Alejandro Clocchiatti, Astrophys.J. 841 (2017) 127, arXiv:1702.00416.
[Muller:2017bdf]
[16-11]
Neutrino fluxes from a core-collapse supernova in a model with three sterile neutrinos, A. V. Yudin, D. K. Nadyozhin, V. V. Khruschov, S. V. Fomichev, Astron. Lett. 42 (2016) 800-814, arXiv:1701.04713.
[Yudin:2016zqp]
[16-12]
Charged current neutrino interactions in hot and dense matter, Luke F. Roberts, Sanjay Reddy, Phys.Rev. C95 (2017) 045807, arXiv:1612.02764.
[Roberts:2016mwj]
[16-13]
Impact of $(\alpha,n)$ reactions on neutrino-driven wind nucleosynthesis, Julia Bliss, Almudena Arcones, Fernando Montes, Jorge Pereira, J.Phys. G44 (2017) 054003, arXiv:1612.02435.
[Bliss:2016spk]
[16-14]
Nuclear pasta and supernova neutrinos at late times, C. J. Horowitz et al., arXiv:1611.10226, 2016.
[1611.10226]
[16-15]
Evidence from stable isotopes and Be-10 for solar system formation triggered by a low-mass supernova, Projjwal Banerjee, Yong-Zhong Qian, Alexander Heger, W. C. Haxton, Nature Commun. 7 (2016) 3639, arXiv:1611.07162.
[Banerjee:2016tzd]
[16-16]
Neutrino-nucleon scattering in supernova matter from the virial expansion, C.J. Horowitz, O. L. Caballero, Zidu Lin, Evan O'Connor, A. Schwenk, Phys. Rev. C95 (2017) 025801, arXiv:1611.05140.
[Horowitz:2016gul]
[16-17]
Background Study on Supernova Relic Neutrinos Search in SuperK-Gd, Yang Zhang, arXiv:1610.09457, 2016.
[Zhang:2016mce]
[16-18]
Impact of new data for neutron-rich heavy nuclei on theoretical models for $r$-process nucleosynthesis, Toshitaka Kajino, Grant J. Mathews, Rept.Prog.Phys. 80 (2017) 084901, arXiv:1610.07929.
[Kajino:2016pia]
[16-19]
Inferring the core-collapse supernova explosion mechanism with gravitational waves, Jade Powell, Sarah Gossan, Joshua Logue, Ik Siong Heng, Phys. Rev. D94 (2016) 123012, arXiv:1610.05573.
[Powell:2016wke]
[16-20]
Supernova Constraints on Massive (Pseudo)Scalar Coupling to Neutrinos, Lucien Heurtier, Yongchao Zhang, JCAP 1702 (2017) 042, arXiv:1609.05882.
[Heurtier:2016otg]
[16-21]
Impact of Nucleon-Nucleon Bremsstrahlung Rates Beyond One-Pion Exchange, Alexander Bartl, Robert Bollig, Hans-Thomas Janka, Achim Schwenk, Phys. Rev. D94 (2016) 083009, arXiv:1608.05037.
[Bartl:2016iok]
[16-22]
Detecting supernova neutrinos with iron and lead detectors, Abhijit Bandyopadhyay, Pijushpani Bhattacharjee, Sovan Chakraborty, Kamales Kar, Satyajit Saha, Phys.Rev. D95 (2017) 065022, arXiv:1607.05591.
[Bandyopadhyay:2016gkv]
[16-23]
Detecting supernovae neutrino with Earth matter effect, Wei Liao, Phys. Rev. D94 (2016) 113016, arXiv:1607.03334.
[Liao:2016uis]
[16-24]
Supernova neutrino physics with xenon dark matter detectors: A timely perspective, Rafael F. Lang, Christopher McCabe, Shayne Reichard, Marco Selvi, Irene Tamborra, Phys. Rev. D94 (2016) 103009, arXiv:1606.09243.
[Lang:2016zhv]
[16-25]
Presupernova neutrino events relating to the final evolution of massive stars, Takashi Yoshida, Ko Takahashi, Hideyuki Umeda, Koji Ishidoshiro, Phys. Rev. D93 (2016) 123012, arXiv:1606.04915.
[Yoshida:2016imf]
[16-26]
Probing axions with the neutrino signal from the next galactic supernova, Tobias Fischer et al., Phys. Rev. D94 (2016) 085012, arXiv:1605.08780.
[Fischer:2016cyd]
[16-27]
Getting the Most from Detection of Galactic Supernova Neutrinos in Future Large Scintillator Detectors, Jia-Shu Lu, Yu-Feng Li, Shun Zhou, Phys. Rev. D94 (2016) 023006, arXiv:1605.07803.
[Lu:2016ipr]
[16-28]
Supernova energy measurement with longitudinal gravitational memory effect, Darsh Kodwani, Ue-Li Pen, I-Sheng Yang, arXiv:1605.05399, 2016.
[Kodwani:2016vis]
[16-29]
Non-Standard Neutrino Interactions in Supernovae, Charles J. Stapleford, Daavid J. Vaananen, James P. Kneller, Gail C. McLaughlin, Brandon T. Shapiro, Phys. Rev. D94 (2016) 093007, arXiv:1605.04903.
[Stapleford:2016jgz]
[16-30]
Neutrinos from Type Ia Supernovae I: The Deflagration-To-Detonation Transition Scenario, Warren P. Wright, Gautam Nagaraj, James P. Kneller, Kate Scholberg, Ivo R. Seitenzahl, Phys. Rev. D94 (2016) 025026, arXiv:1605.01408.
[Wright:2016xma]
[16-31]
Production of keV Sterile Neutrinos in Supernovae: New Constraints and Gamma Ray Observables, Carlos A. Arguelles, Vedran Brdar, Joachim Kopp, arXiv:1605.00654, 2016.
[Arguelles:2016uwb]
[16-32]
How well can new particles interacting with neutrinos be constrained after a galactic supernova?, Jonathan H. Davis, arXiv:1605.00011, 2016.
[Davis:2016dqh]
[16-33]
Determination of the Neutron-Capture Rate of 17C for the R-process Nucleosynthesis, M. Heine et al., Phys. Rev. C95 (2017) 014613, arXiv:1604.05832.
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[16-34]
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Resonant spin-flavor conversion of supernova neutrinos and deformation of the electron antineutrino spectrum, Tomonori Totani, Katsuhiko Sato, Phys. Rev. D54 (1996) 5975-5992, arXiv:astro-ph/9609035.
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Gravitational collapse of rotating stellar cores and supernovae, K. Sato, T. M. Shimizu, S. Yamada, Nucl. Phys. A606 (1996) 118-136.
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Spectrum of the Supernova Relic Neutrino Background and Evolution of Galaxies, Tomonori Totani, Katsuhiko Sato, Yuzuru Yoshii, Astrophys. J. 460 (1996) 303-312, arXiv:astro-ph/9509130.
[Totani:1995dw]
[16-364]
Effects of random density fluctuations on matter enhanced neutrino flavor transitions in supernovae and implications for supernova dynamics and nucleosynthesis, F. N. Loreti, Y. Z. Qian, G. M. Fuller, A. B. Balantekin, Phys. Rev. D52 (1995) 6664-6670, arXiv:astro-ph/9508106.
[Loreti:1995ae]
[16-365]
Cherenkov radiation by neutrinos in a supernova core, Subhendra Mohanty, Manoj K. Samal, Phys. Rev. Lett. 77 (1996) 806-809, arXiv:hep-ph/9506385.
[Mohanty:1995bx]
[16-366]
Spectrum of the relic neutrino background from past supernovae and cosmological models, Tomonori Totani, Katsuhiko Sato, Astropart. Phys. 3 (1995) 367-376, arXiv:astro-ph/9504015.
[Totani:1995rg]
[16-367]
Gravitational radiation from rotational collapse of a supernova core, S. Yamada, K. Sato, Astrophys. J. 450 (1995) 245-252.
[Yamada:1995pd]
[16-368]
Neutrino oscillations in the magnetic field of the sun, supernovae, and neutron stars, G.G. Likhachev, A.I. Studenikin, J.Exp.Theor.Phys. 81 (1995) 419-425.
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[16-369]
Neutrino-neutrino scattering and matter enhanced neutrino flavor transformation in Supernovae, Yong Zhong Qian, George M. Fuller, Phys. Rev. D51 (1995) 1479-1494, arXiv:astro-ph/9406073.
[Qian:1994wh]
[16-370]
Signature of supernova neutrino flavor mixing in water Cerenkov detectors, Yong-Zhong Qian, George M. Fuller, Phys. Rev. D49 (1994) 1762-1770.
[Qian:1994hh]
[16-371]
The Galactic supernova rate, G. A. Tammann, W. Loeffler, A. Schroder, Astrophys. J. Suppl. 92 (1994) 487-493.
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[16-372]
'Guest stars', sample completeness and the local supernova rate, R. G. Strom, Astron. Astrophys. 288 (1994) L1-L4.
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[16-373]
The Detection of a cosmologically significant neutrino mass from the neutrino burst of a galactic supernova, D. B. Cline et al., Phys. Rev. D50 (1994) 720-729.
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[16-374]
The Rate of Supernovae. II. the Selection Effects and the Frequencies Per Unit Blue Luminosity, E. Cappellaro et al., Astron. Astrophys. 273 (1993) 383, arXiv:astro-ph/9302017.
[Cappellaro:1993ns]
[16-375]
A Connection between flavor mixing of cosmologically significant neutrinos and heavy element nucleosynthesis in supernovae, Yong-Zhong Qian et al., Phys. Rev. Lett. 71 (1993) 1965-1968.
[Qian:1993dg]
[16-376]
The absolute magnitudes of Type IA supernovae, M. M. Phillips, Astrophys. J. 413 (1993) L105-L108.
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[16-377]
Convective instability in hot bubble in a delayed supernova explosion, Shoichi Yamada, Tetsuya Shimizu, Katsuhiko Sato, Prog. Theor. Phys. 89 (1993) 1175-1182.
[Yamada:1993sk]
[16-378]
How rare are supernovae?, S. van den Bergh, Comments on Astrophys. 17 (1993) 125-130.
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[16-379]
The Future of supernova neutrino detection, Adam Burrows, David Klein, Raj Gandhi, Phys. Rev. D45 (1992) 3361-3385.
From the abstract: In this paper, we construct a detailed fiducial model of supernova neutrino bursts that incorporates the numerous emission features derived and predicted by supernova and protoneutron star theorists during the last decade.
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[16-380]
High rate for Type IC supernovae, Richard A. Muller et al., Astrophys. J. 384 (1992) L9-L13.
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The rate of stellar collapses in the galaxy, Kavan U. Ratnatunga, Sidney van den Bergh, Astrophys. J. 343 (1989) 713-717.
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The modified correlation mass method for detecting neutrino mass from astrophysical neutrino bursts, K. L. Chan, H. Chiu, Y. Kondo, Astron. Astrophys. 215 (1989) 387-398.
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Neutronization neutrino pulses from supernovae and the triplet majoron model, Y. Aharonov, F. T. Avignone, S. Nussinov, Phys. Lett. B200 (1988) 122-124.
[Aharonov:1988ju]
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Resonant Helicity Flip of $\nu_e$ Due to Magnetic Moment and Dynamics of Supernova, M.B. Voloshin, Phys.Lett. B209 (1988) 360.
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Implications of the supernova SN1987a neutrino signals, I. Goldman, Y. Aharonov, G. Alexander, S. Nussinov, Phys. Rev. Lett. 60 (1988) 1789.
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[16-386]
Neutral current reactions of solar and supernova neutrinos on deuterium, J. N. Bahcall, K. Kubodera, S. Nozawa, Phys. Rev. D38 (1988) 1030.
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$\nu_e-\nu_e$ scattering and the possibility of a resonance change of neutrino helicity in the magnetic field of a supernova, L. B. Okun, Sov. J. Nucl. Phys. 48 (1988) 967-968.
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[16-388]
Magnetic moments of neutrinos: particle and astrophysical aspects, Shmuel Nussinov, Yoel Rephaeli, Phys. Rev. D36 (1987) 2278.
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Neutrino magnetic moment may solve the supernovae problem, Arnon Dar, 1987. Print-87-0178 (IAS, Princeton).
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Supernova explosions and constraints on mass and lifetime of heavy neutrinos, M. Takahara, K. Sato, Phys. Lett. B174 (1986) 373-377.
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Accreting white dwarf models of Type I supernovae. III - Carbon deflagration supernovae, K. Nomoto, F.K. Thielemann, K. Yokoi, Astrophys. J. 286 (1984) 644-658.
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17 - Phenomenology - Type II - Conference Proceedings

[17-1]
Supernova Physics at DUNE, Artur Ankowski et al., arXiv:1608.07853, 2016. Summary of workshop 'Supernova Physics at DUNE', Virginia Tech.
[Ankowski:2016lab]
[17-2]
Neutrino-Induced Nucleosynthesis in Helium Shells of Early Core-Collapse Supernovae, Projjwal Banerjee, Yong-Zhong Qian, Alexander Heger, Wick Haxton, arXiv:1512.01523, 2015. OMEG 2015.
[1512.01523]
[17-3]
Probing Efficient Cosmic-Ray Acceleration in Young Supernovae, Vikram V. Dwarkadas, M. Renaud, A. Marcowith, V. Tatischeff, PoS ICRC2015 (2016) 493, arXiv:1509.00879. 34th International Cosmic Ray Conference (ICRC).
[Dwarkadas:2015ppa]
[17-4]
The Physics Of Supernova Neutrino Oscillations, James P. Kneller, arXiv:1507.01434, 2015. CIPANP2015.
[Kneller:2015lqa]
[17-5]
Type IIn supernovae as sources of high energy neutrinos, V.N. Zirakashvili, V.S. Ptuskin, PoS ICRC2015 (2016) 472, arXiv:1505.08144. 34th ICRC, Hague, Netherlands 30July-06Aug 2015.
[Zirakashvili:2015tda]
[17-6]
Principal Physical Effects in Collapsing Stellar Cores, D.K. Nadyozhin, A.V. Yudin, arXiv:1308.4448, 2013. ICRANet Workshop 'From Nuclei to White Dwarfs and Neutron Stars', Les Houches, 3-8 April 2011.
[Nadyozhin:2013kba]
[17-7]
A Critical Appraisal of Some Concepts Used in Neutrino Physics, Francesco Vissani, Manimala Mitra, Giulia Pagliaroli, Nuovo Cim. C36 (2013) 223-228, arXiv:1206.1466. IFAE 2012.
[Vissani:2012dm]
[17-8]
Estimations of the Distances of Stellar Collapses in the Galaxy by Analyzing the Energy Spectrum of Neutrino Bursts, Ernesto Kemp, Bruno Miguez, Walter Fulgione, Int.J.Mod.Phys. E20S2 (2011) 57-60, arXiv:1202.0181. SMFNS 2011.
[Kemp:2012in]
[17-9]
Astrophysical Models of r-Process Nucleosynthesis: An Update, Yong-Zhong Qian, AIP Conf.Proc. 1484 (2012) 201, arXiv:1201.5112. 11th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG11), Wako, Japan.
[Qian:2012pe]
[17-10]
Core-Collapse Supernovae: Explosion Dynamics, Neutrinos and Gravitational Waves, Bernhard Mueller et al., arXiv:1112.1913, 2011. HANSE 2011.
[Mueller:2011ab]
[17-11]
Neutral Current Coherent Cross Sections- Implications on Gaseous Spherical TPC's for detecting SN and Earth neutrinos, J. D. Vergados, J. Phys. Conf. Ser. 309 (2011) 012031, arXiv:1103.1107. Fifth symposium on large TPCs for low energy rare event detection and workshop on neutrinos from Supernovae, Paris Dec. 14-18, 2010.
[Vergados:2011ym]
[17-12]
Explosive nucleosynthesis in core-collapse supernovae, A. Arcones, J. Phys. Conf. Ser. 312 (2011) 042005, arXiv:1012.4917. INPC 2010 Vancouver.
[Arcones:2010fk]
[17-13]
Lepton flavor violating New Physics and supernova explosion, Oleg Lychkovskiy, Sergei Blinnikov, Mikhail Vysotsky, arXiv:1010.0883, 2010. 16th International Seminar on High Energy Physics 'QUARKS-2010', Kolomna, Russia, 6-12 June, 2010.
[Lychkovskiy:2010xh]
[17-14]
Dirac neutrino magnetic moment and a possible time evolution of the neutrino signal from a supernova, R.A. Anikin, A.V. Kuznetsov, N.V. Mikheev, Astron.Lett. 36 (2010) 680, arXiv:1010.0583. XVI International Seminar Quarks'2010, Kolomna, Moscow Region, June 6-12, 2010.
[Anikin:2010rh]
[17-15]
Can a supernova bang twice?, Jurgen Schaffner-Bielich et al., Prog. Theor. Phys. Suppl. 186 (2010) 93-98, arXiv:1009.6096. Yukawa International Program for Quark-Hadron Sciences: New Frontiers in QCD 2010, Kyoto, Japan.
[SchaffnerBielich:2010at]
[17-16]
The r-Process in Black Hole Winds, Shinya Wanajo, Hans-Thomas Janka, AIP Conf. Proc. 1269 (2010) 120-125, arXiv:1006.2277. OMEG10, March 2010.
[Wanajo:2010ab]
[17-17]
Using supernova neutrinos to monitor the collapse, to search for gravity waves and to probe neutrino masses, F. Vissani, G. Pagliaroli, F. Rossi-Torres, arXiv:1005.3682, 2010. Galileo-Xu Guangqi meeting: The Sun, the Stars, the Universe and General Relativity; October 26-30, 2009, Shanghai (China).
[Vissani:2011zz]
[17-18]
Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star, Men-Quan Liu, Ye-Fei Yuan, arXiv:1005.1845, 2010. Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, Beijing, P. R. China.
[Liu:2010pk]
[17-19]
Nucleosynthesis in neutrino-driven winds: influence of the nuclear physics input, Almudena Arcones, Gabriel Martinez-Pinedo, J. Phys. Conf. Ser. 202 (2010) 012007, arXiv:0909.1012. Nuclear Physics in Astrophysics IV.
[Arcones:2009gu]
[17-20]
Probing the Core-Collapse Supernova Mechanism with Gravitational Waves, C. D. Ott, Class. Quant. Grav. 26 (2009) 204015, arXiv:0905.2797. 13th Gravitational Wave Data Analysis Workshop.
[Ott:2009bw]
[17-21]
The Strange Prospects for Astrophysics, Irina Sagert et al., J. Phys. G36 (2009) 064009, arXiv:0902.2084. International conference on strangeness in quark matter (SQM2008), Beijing, October 6-10, Beijing, China.
[Sagert:2009bn]
[17-22]
Physics potential of future supernova neutrino observations, Amol Dighe, J. Phys. Conf. Ser. 136 (2008) 022041, arXiv:0809.2977. Neutrino 2008, Christchurch, NZ.
[Dighe:2008dq]
[17-23]
Supernova neutrinos: Strong coupling effects of weak interactions, G. L. Fogli, E. Lisi, A. Marrone, A. Mirizzi, arXiv:0809.2940, 2008. NO-VE 2008, IV International Workshop on.
[Fogli:2008cz]
[17-24]
Formation of quark phases in compact stars and SN explosion, Alessandro Drago, Giuseppe Pagliara, Giulia Pagliaroli, Francesco Lorenzo Villante, Francesco Vissani, AIP Conf. Proc. 1056 (2008) 256-263, arXiv:0809.0518. 6th International Conference on Perspectives in Hadronic Physics, May 2008, Trieste.
[Drago:2008tb]
[17-25]
Core-collapse supernova neutrinos and neutrino properties, J. Gava, C. Volpe, AIP Conf. Proc. 1038 (2008) 193-201, arXiv:0805.2717. Three days of Strong Interactions and Astrophysics HLPW08, 6-8 March 2008.
[Gava:2008st]
[17-26]
Nucleosynthesis in Early Neutrino Driven Winds, R.D. Hoffman et al., AIP Conf. Proc. 1005 (2008) 225-228, arXiv:0801.1828. CNR 2007 Compound-Nuclear Reactions and Related Topics Workshop.
[Hoffman:2008jm]
[17-27]
Plasma induced neutrino spin-flip in a supernova and new bounds on the neutrino magnetic moment, A.V. Kuznetsov, N.V. Mikheev, arXiv:0708.2802, 2007. XIV International School 'Particles and Cosmology', Baksan Valley, Kabardino Balkaria, Russia, April 16-21, 2007.
[Kuznetsov:2007np]
[17-28]
Spectral Modeling of Type II Supernovae, E. Baron, AIP Conf. Proc. 924 (2007) 350-357, arXiv:astro-ph/0611545. The Multicoloured Landscape of Compact Objects and their Explosive Progenitors: Theory vs Observations.
[Baron:2006et]
[17-29]
The diffuse supernova neutrino flux, Cecilia Lunardini, Nucl. Phys. Proc. Suppl. 221 (2011) 160-165, arXiv:astro-ph/0610534. Neutrino 2006, Santa Fe, June 2006.
[Lunardini:2006em]
[17-30]
Time-dependence Effects in Photospheric-Phase Type II Supernova Spectra, Luc Dessart, John Hillier, AIP Conf.Proc. 924 (2007) 441, arXiv:astro-ph/0610136. The Multicoloured Landscape of Compact Objects and their Explosive Progenitors: Theory vs Observations, Cefalu, Sicily, June 11-24, 2006.
[Dessart:2006ky]
[17-31]
Neutrinos from supernova remnants after the first HESS observations, Francesco Vissani, arXiv:astro-ph/0609575, 2006. Vulcano Workshop 2006: Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, 22-27 May 2006.
[Vissani:2006pi]
[17-32]
R-process Experimental Campaign at the National Superconducting Cyclotron Laboratory, J. Pereira et al., PoS NIC-IX (2006) 162, arXiv:astro-ph/0608582. PoS.
[Pereira:2006vr]
[17-33]
Thermal neutrinos from pre-supernova, A. Odrzywolek, M. Misiaszek, M. Kutschera, Nucl. Phys. Proc. Suppl. 221 (2011) 380, arXiv:astro-ph/0608492. Neutrino 2006.
[Odrzywolek:2006fn]
[17-34]
Aspects of Neutrino Production in Supernovae, Todd A. Thompson, arXiv:astro-ph/0608231, 2006. International Workshop on the Energy Budget in the High Energy Universe, Kashiwa campus, Univ. of Tokyo, Chiba, Japan, Feb. 2006.
[Thompson:2006ar]
[17-35]
Neutrinos, Fisson Cycling, and the r-process, J. Beun, G. C. McLaughlin, R. Surman, W. R. Hix, PoS NIC-IX (2006) 140, arXiv:astro-ph/0607180. NIC-IX, International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, CERN, Geneva, Switzerland, 25-30 June, 2006.
[Beun:2006vg]
[17-36]
Neutrino chirality flip in a supernova and the bound on the neutrino magnetic moment, A.V. Kuznetsov, N.V. Mikheev, arXiv:hep-ph/0606261, 2006. XIV International Seminar Quarks'2006, St.-Petersburg, Repino, Russia, May 19-25, 2006.
[Kuznetsov:2006ch]
[17-37]
The Supernova Gamma-Ray Burst Connection, Stan Woosley, Alexander Heger, AIP Conf. Proc. 836 (2006) 398-407, arXiv:astro-ph/0604131. AIP Conf. Proc. 'Gamma Ray Bursts in the Swift Era'.
[Woosley:2006gw]
[17-38]
Shell-type Supernova Remnants, Heinrich J. Volk, arXiv:astro-ph/0603502, 2006. Cherenkov 2005, Towards a Network of Atmospheric Cherenkov Detectors VII, Ecole Polytechnique, Palaiseau (France), April 27-29, 2005.
[Volk:2006nm]
[17-39]
The Relic Neutrino Backround from the First Stars, Keith A. Olive, Pearl Sandick, arXiv:astro-ph/0603236, 2006. IIIrd International Workshop on: NO-VE 'Neutrino Oscillations in Venice', Venice Italy, February 2006.
[Olive:2006ei]
[17-40]
Nucleosynthesis in Neutrino-Driven Supernovae, C. Froehlich et al., New Astron. Rev. 50 (2006) 496-499, arXiv:astro-ph/0511584. Astronomy with Radioactivities V, Clemson University, September 5-9, 2005.
[Frohlich:2005em]
[17-41]
Neutrinos from Supernovas and Supernova Remnants, Francesco Vissani, Maria Laura Costantini, Aip Conf. Proc. 794 (2005) 219, arXiv:astro-ph/0508152. IFAE, Catania 2005.
[Costantini:2005vh]
[17-42]
Nucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of Extremely Metal Poor Stars, Marco Limongi, Alessandro Chieffi, IAU Symp. (2005), arXiv:astro-ph/0507340. 6IAU Symp. No. 228 'From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution'.
[Limongi:2005yu]
[17-43]
Neutrino Processes in Strong Magnetic Fields, Huaiyu Duan, Yong-Zhong Qian, arXiv:astro-ph/0506129, 2005. INT workshop.
[Duan:2005wv]
[17-44]
SN/GRB connection: a statistical approach with BATSE and Asiago Catalogues, S. Valenti et al., Nuovo Cim. 28C (2005) 633, arXiv:astro-ph/0505052. 4th workshop on Gamma Ray Bursts in the Afterglow Era, Rome, 2004.
[Valenti:2005vh]
[17-45]
Supernova search at intermediate z. II. Host galaxy morphology, J. Mendez et al., ASP Conf.Ser. 342 (2005) 488, arXiv:astro-ph/0502397. 1604-2004: Supernovae as Cosmological Lighthouses.
[Mendez:2005iu]
[17-46]
Supernova search at intermediate z. I. Spectroscopic analysis, G. Altavilla et al., ASP Conf.Ser. 342 (2005) 486, arXiv:astro-ph/0502395. 1604-2004: Supernovae as Cosmological Lighthouses.
[Altavilla:2005is]
[17-47]
Supernova Rates in Galaxy Clusters, Dan Maoz, ASP Conf.Ser. (2005), arXiv:astro-ph/0501492. 1604-2004: Supernovae as Cosmological Lighthouses.
[Maoz:2005xu]
[17-48]
Searching for Progenitors of Core-Collapse Supernovae, Schuyler D. Van Dyk, ASP Conf.Ser. (2005), arXiv:astro-ph/0501363. 1604-2004: Supernovae as Cosmological Lighthouses.
[VanDyk:2005yn]
[17-49]
Nuclear physics and astrophysics of the r-process, Y. -Z. Qian, Nucl. Phys. A752 (2005) 550, arXiv:astro-ph/0501237. International Nuclear Physics Conference (INPC2004).
[Qian:2005am]
[17-50]
IMF variations and their implications for Supernovae numbers, C. Weidner, P. Kroupa, Proc. Sci. BDMH2004 (2004) 063, arXiv:astro-ph/0412114. 'Baryons in Dark Matter Halos', Novigrad, Croatia, October 5-9, 2004.
[Weidner:2004ni]
[17-51]
Supernova Neutrinos and the absolute scale of neutrino masses - a Bayesian approach, Enrico Nardi, arXiv:hep-ph/0412024, 2004. Fifth Latin American Simposium on High Energy Physics (V-SILAFAE) Lima, Peru, July 12-17, 2004.
[Nardi:2004uz]
[17-52]
Supernova Neutrino Process and its Impact on the Galactic Chemical Evolution of the Light Elements, Takashi Yoshida, Toshitaka Kajino, Nucl. Phys. A758 (2005) 35, arXiv:astro-ph/0410651. Nuclei in the Cosmos VIII.
[Yoshida:2004fm]
[17-53]
The r-process nucleosynthesis: a continued challenge for nuclear physics and astrophysics, S. Goriely et al., Nucl. Phys.A (2004), arXiv:astro-ph/0410429. Nuclei in the Cosmos.
[Goriely:2004qb]
[17-54]
Sterile Neutrinos in astrophysical and cosmological sauce, Marco Cirelli, arXiv:astro-ph/0410122, 2004. 10th International Symposium on Particles, Strings and Cosmology (PASCOS '04), August 2004, Boston, USA, and XVI Incontri sulla Fisica delle Alte Energie (IFAE), April 2004, Torino, Italy.
[Cirelli:2004qs]
[17-55]
Parity Violation in Astrophysics, C. J. Horowitz, Eur. Phys. J. A24S2 (2005) 167, arXiv:nucl-th/0410074. PAVI04 conference in Grenoble, France.
[Horowitz:2004pc]
[17-56]
Powerful gravitational-wave bursts from supernova neutrino oscillations, Herman J. Mosquera Cuesta, Karen Fiuza, Aip Conf. Proc. 739 (2005) 702, arXiv:astro-ph/0407526. 'Hadron Physics - RANP 2004', Angra dos Reis - Rio de Janeiro - Brazil, March 28 to April 03.
[MosqueraCuesta:2004xd]
[17-57]
Neutrino Oscillations at Supernova Core Bounce Generate the Strongest Gravitational-Wave Bursts, Herman J. Mosquera Cuesta, Karen Fiuza, Int. J. Mod. Phys. D13 (2004) 1297, arXiv:astro-ph/0407184. International Workshop on Astronomy and Relativistic Astrophysics, Olinda (Brazil), October 12-16 (2003).
[MosqueraCuesta:2004qh]
[17-58]
Core-Collapse Supernovae Induced by Anisotropic Neutrino Radiation, Yuko Motizuki, Hideki Madokoro, Tetsuya Shimizu, EAS Publ.Ser. 11 (2004) 163, arXiv:astro-ph/0406303. Int. conf. in hohour of the 60th birthday of Marcel Arnould, The Future Astronuclear Physics, From microscopic puzzles to macroscopic nightmares.
[Motizuki:2004jg]
[17-59]
Supernova Neutrino-Nucleus Physics and the r-process, W. C. Haxton, arXiv:nucl-th/0406012, 2004. 'The r-process: The Astrophysical Origin of the Heavy Elements...'.
[Haxton:2004qn]
[17-60]
Global Anisotropies in Supernova Explosions and Pulsar Recoil, L. Scheck et al., arXiv:astro-ph/0405311, 2004. 12th Workshop on Nuclear Astrophysics, Ringberg Castle, March 22-27, 2004.
[Scheck:2004wq]
[17-61]
Decays of supernova relic neutrinos, G.L. Fogli, E. Lisi, A. Mirizzi, D. Montanino, arXiv:hep-ph/0405136, 2004. 39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Italy, 21-28 Mar 2004.
[Fogli:2004uy]
[17-62]
Sterile neutrinos: from cosmology to experiments, Guido Marandella, arXiv:hep-ph/0405090, 2004. 39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 21-28 March 2004.
[Marandella:2004xv]
[17-63]
Neutrinos from pre-supernova star, A. Odrzywolek, M. Misiaszek, M. Kutschera, Acta Phys. Polon. B35 (2004) 1981, arXiv:astro-ph/0405006. Epiphany Conference on Astroparticle Physics, 8-11 January 2004, Cracow, Poland.
[Odrzywolek:2004em]
[17-64]
An Approach to Neutrino Radiative Transfer in Supernova Simulations, Christian Y. Cardall, arXiv:astro-ph/0404401, 2004. Numerical Methods for Multidimensional Radiative Transfer Problems (RadConf2003), Heidelberg, Germany, 24-26 September 2003.
[Cardall:2004nd]
[17-65]
The Evolution of Supernovae in the Winds of Massive Stars, Vikram Dwarkadas, arXiv:astro-ph/0403195, 2004. Cosmic Explosions in Three Dimensions: Asymmetries in Supernovae and Gamma-Ray Bursts.
[Dwarkadas:2004zu]
[17-66]
Detection of Supernova Neutrinos, B. Bekman, J. Holeczek, J. Kisiel, Acta Phys. Polon. B35 (2004) 1215, arXiv:hep-ph/0403117. XXVIII Mazurian Lakes School of Physics, Krzyze, Poland, August 31 - September 7, 2003.
[Bekman:2004qj]
[17-67]
Neutrino Processes in Supernovae and Neutrons Stars in Their Infancy and Old Age, M. Prakash, S. Ratkovic, S. I. Dutta, arXiv:astro-ph/0403038, 2004. KIAS-APCTP International Symposium in Astro-Hadron Physics, November 10-14, 2003.
[Prakash:2004wv]
[17-68]
Measuring neutrino masses with supernova neutrinos, Enrico Nardi, arXiv:astro-ph/0401624, 2004. X Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July 2003.
[Nardi:2004ms]
[17-69]
Neutron Star Kicks and Supernova Asymmetry, Dong Lai, arXiv:astro-ph/0312542, 2003. 3D Signatures of Stellar Explosion, a workshop honoring J.C. Wheeler's 60th Birthday.
[Lai:2003hm]
[17-70]
Low frequency radio and X-ray properties of core-collapse supernovae, A. Ray, P. Chandra, F. Sutaria, S. Bhatnagar, Springer Proc.Phys. 99 (2005) 145-150, arXiv:astro-ph/0311419. IAU Colloquium 192 'Supernovae (10 years of SN 1993J)', April 2003, Valencia, Spain.
[Ray:2003nu]
[17-71]
Pulsar velocities and dark matter hint at a singlet neutrino, Alexander Kusenko, arXiv:astro-ph/0311240, 2003. Sixth RESCEU International Symposium 'Frontier in Astroparticle Physics and Cosmology', Tokyo, Japan, November 4 - 7, 2003.
[Kusenko:2003ff]
[17-72]
Expected Changes of Supernovae with Redshift due to Evolution of their Progenitors, I. Dominguez et al., Springer Proc.Phys. 99 (2005) 567-572, arXiv:astro-ph/0311140. IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003.
[Dominguez:2003rx]
[17-73]
44Ti radioactivity in young supernova remnants: Cas A and SN 1987A, Y. Motizuki, S. Kumagai, New Astron. Rev. 48 (2004) 69, arXiv:astro-ph/0311080. 'Astronomy with Radioactivities IV', Seeon, Germany, June 2003.
[Motizuki:2003dx]
[17-74]
Supernova Statistics, E. Cappellaro, R. Barbon, M. Turatto, Springer Proc.Phys. 99 (2005) 347-354, arXiv:astro-ph/0310859. IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.
[Cappellaro:2003eg]
[17-75]
Type Ia Supernovae: Spectroscopic Surprises, D. Branch, arXiv:astro-ph/0310685, 2003. 3-D Signatures of Stellar Explosions: A Workshop Honoring J. Craig Wheeler's 60th Birthday.
[Branch:2003fr]
[17-76]
Effects of Small-Scale Fluctuations of Neutrino Flux in Supernova Explosions, H. Madokoro, T. Shimizu, Y. Motizuki, Springer Proc.Phys. 99 (2005) 309-314, arXiv:astro-ph/0310481. IAU Colloquium 192, SUPERNOVAE (10 years of SN1993J), Valencia, Spain.
[Madokoro:2003hh]
[17-77]
Understanding Type II Supernovae, L. Zampieri, M. Ramina, A. Pastorello, Springer Proc.Phys. 99 (2005) 275-280, arXiv:astro-ph/0310057. IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003.
[Zampieri:2003qn]
[17-78]
Observational Properties of Type II Plateau Supernovae, A. Pastorello et al., Springer Proc.Phys. 99 (2005) 195-199, arXiv:astro-ph/0310056. IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003.
[Pastorello:2003qm]
[17-79]
Cosmic rays, stellar evolution, and supernova physics, P. L. Biermann, New Astron. Rev. 48 (2004) 41, arXiv:astro-ph/0309810. 'Astronomy With Radioactivities IV - Filling the Sensitivty Gap in MEV Astronomy', Seeon Conference, Bavaria, Germany, May 2003.
[Biermann:2003et]
[17-80]
A Geometric Determination of the Distance to SN 1987A and the LMC, N. Panagia, Springer Proc.Phys. 99 (2005) 585-592, arXiv:astro-ph/0309416. IAU Colloquium 192 'Supernovae (10 years of SN1993J)', Valencia, Spain.
[Panagia:2003rt]
[17-81]
$^{56}\mathrm{Ni}$ mass in type IIP SNe: Light curves and H-alpha luminosities diagnostics, Abouazza Elmhamdi, N. N. Chugai, I. J. Danziger, Springer Proc.Phys. 99 (2005) 303-308, arXiv:astro-ph/0309286. IAU Colloquium 192: Supernovae (10 Years after SN1993J), Valencia, Spain, 22-26 Apr 2003.
[Elmhamdi:2003wu]
[17-82]
Neutrinos and (anti)neutrinos from supernovae and from the earth in the Borexino detector, L. Miramonti, arXiv:hep-ex/0307029, 2003. 1st Yamada Symposium on Neutrinos and Dark Matter in Nuclear Physics June 9-14, 2003, Nara, Japan.
[Miramonti:2003hw]
[17-83]
Neutrinos in Extra Dimensions and Supernovae, M. Cirelli, arXiv:hep-ph/0305141, 2003. 38th Rencontres de Moriond - Electroweak Interactions and Unified Theories, March 15-22, 2003, Les Arcs, France.
[Cirelli:2003vh]
[17-84]
Supernova neutrinos: Flavor-dependent fluxes and spectra, G.G.Raffelt et al., arXiv:astro-ph/0303226, 2003. NOON 03, Kanazawa, 10-14 Feb 2003.
[Raffelt:2003en]
[17-85]
Neutrinos and Nucleosynthesis in Supernova, U. Solis, J. C. D'Olivo, L. G. Cabral-Rosetti, J. Phys. Conf. Ser. 37 (2006) 127-130, arXiv:hep-ph/0302015. Mexican School of Astrophysics (EMA), Guanajuato, Mexico, July 31 - August 7, 2002.
[Solis:2003ak]
[17-86]
Supernova Explosions from Accretion Disk Winds, Andrew I. MacFadyen, arXiv:astro-ph/0301425, 2003. 'From Twilight to Highlight - The Physics of Supernovae' ESO/MPA/MPE Workshop, Garching July 2002.
[MacFadyen:2003wg]
[17-87]
Presupernova Evolution of Rotating Massive Stars and the Rotation Rate of Pulsars, A. Heger, S. E. Woosley, N. Langer, H. C. Spruit, IAU Symp. 215 (2004) 591, arXiv:astro-ph/0301374. IAU 215 'Stellar Rotation'.
[Heger:2003nh]
[17-88]
Supernovae, Gamma-Ray Bursts, and Stellar Rotation, S. E. Woosley, A. Heger, IAU Symp. (2003), arXiv:astro-ph/0301373. IAU 215 'Stellar Rotation'.
[Woosley:2003ng]
[17-89]
Circumstellar Interaction Around Supernovae, Roger A. Chevalier, arXiv:astro-ph/0301368, 2003. 'From Twilight to Highlight - The Physics of Supernovae' ESO/MPA/MPE Workshop, Garching July 2002.
[Chevalier:2003nb]
[17-90]
Supernova Neutrinos : oscillations and new interactions, D. Montanino, 2003. Seminar at Padua University, November 18, 2003, Padua, Italy. http://www.pd.infn.it/~laveder/unbound/seminari/sn/SuperNovae.ppt.
[Montanino:PD2003]
[17-91]
Observable Effects of Shocks in Compact and Extended Presupernovae, S. Blinnikov et al., arXiv:astro-ph/0212569, 2002. ESO/MPA/MPE Workshop 'From Twilight to Highlight: The Physics of Supernovae', Garching, July 2002.
[Blinnikov:2002tk]
[17-92]
Light Curves of Type Ia Supernovae as a Probe for an Explosion Model, Elena Sorokina, Sergey Blinnikov, arXiv:astro-ph/0212527, 2002. From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.
[Sorokina:2002gr]
[17-93]
The Mechanism of Core-Collapse Supernovae and the Ejection of Heavy Elements, H.-Th. Janka, R. Buras, M. Rampp, Nucl. Phys. A718 (2003) 269, arXiv:astro-ph/0212317. NIC7, Fuji-Yoshida, Japan, July 8-12, 2002.
[Janka:2002ej]
[17-94]
X-ray emission of young SN Ia remnants as a probe for an explosion model, D.I.Kosenko, E.I.Sorokina, S.I.Blinnikov, P. Lundqvist, arXiv:astro-ph/0212188, 2002. 34th COSPAR Sci. Assembly, Houston, 10-19 october 2002.
[Kosenko:2002yc]
[17-95]
Energy exchange inside SN ejecta and light curves of SNe Ia, E.I.Sorokina, S.I.Blinnikov, arXiv:astro-ph/0212187, 2002. 11th Workshop on 'Nuclear Astrophysics', Ringberg Castle, Tegernsee, Germany, February 11-16, 2002.
[Sorokina:2002yb]
[17-96]
Magnetic Field in Supernovae, Shizuka Akiyama, J. Craig Wheeler, arXiv:astro-ph/0211458, 2002. conference 'Core Collapse of Massive Stars'.
[Akiyama:2002ur]
[17-97]
The Neutrino Signal in Stellar Core Collapse and Postbounce Evolution, M. Liebendoerfer et al., Nucl. Phys. A719 (2003) 144, arXiv:astro-ph/0211329. Nuclear Physics in Astrophysics Conference, Debrecen, Hungary, 2002.
[Liebendoerfer:2002ny]
[17-98]
Variety in Supernovae, Massimo Turatto, Stefano Benetti, Enrico Cappellaro, arXiv:astro-ph/0211219, 2002. ESO / MPA / MPE Workshop: From Twilight to Highlight: The Physics of Supernovae, Garching, Germany, 29-31 June 2002.
[Turatto:2002nx]
[17-99]
Synchronised neutrino oscillations from self interaction and associated applications, Yvonne Y. Y. W., Aip Conf. Proc. 655 (2003) 240, arXiv:hep-ph/0211045. 3rd Topical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology, San Juan, Puerto Rico, 19-24 Aug 2002.
[Wong:2002sc]
[17-100]
Nucleosynthesis as a result of multiple delayed detonations in Type Ia Supernovae, Domingo Garcia-Senz, Eduardo Bravo, Nucl. Phys. A718 (2003) 563, arXiv:astro-ph/0210339. 'Nuclei in the Cosmos VII' 2002.
[GarciaSenz:2002rq]
[17-101]
Neutrino-nucleon scattering rate in the relativistic random phase approximation, L. Mornas, Nucl. Phys. A721 (2003) 1040, arXiv:nucl-th/0210035. PANIC02 conference, 30 sept - 4 oct 2002, Osaka, Japan.
[Mornas:2002ji]
[17-102]
Supernovae and Neutrinos, John F. Beacom, Nucl. Phys. Proc. Suppl. 118 (2003) 307, arXiv:astro-ph/0209136. XXth International Conference on Neutrino Physics and Astrophysics (Neutrino 2002), Munich, Germany, May 25-30, 2002.
[Beacom:2002th]
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Neutron Stars, Pulsars and Supernova Remnants: concluding remarks, F. Pacini, arXiv:astro-ph/0208563, 2002. Proceedings of the 270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Jan. 21-25, 2002, Physikzentrum Bad Honnef.
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[17-104]
Supernova neutrinos, LSND and MiniBooNE, Michel Sorel, arXiv:hep-ph/0205207, 2002. 37th Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, France, 9-16 Mar 2002.
[Sorel:2002hd]
[17-105]
Core-collapse supernova simulations: Variations of the input physics, M. Rampp, R. Buras, H.-Th. Janka, G. Raffelt, arXiv:astro-ph/0203493, 2002. Proceedings of the 11th Workshop on 'Nuclear Astrophysics' held at Ringberg Castle, February 11-16, 2002.
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Neutrinos from SNR, T. Stanev, 2002. International Workshop on Neutrinos and Subterranean Science - NeSS 02, Washington, DC, September 19-21, 2002. http://mocha.phys.washington.edu/~int_talk/WorkShops/Neutrino02/Working_Groups/People/Stanev_T/stanev_thurs_astrocosmo.pdf.
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Supernova constraints on neutrino mass and mixing, Srubabati Goswami, Pramana 54 (2000) 173-184, arXiv:hep-ph/0104094. Meeting on Recent Developments in Neutrino Physics, Ahmedabad, India, 2-4 Feb 1999.
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Supernova neutrinos and the neutrino masses, J. F. Beacom, Rev.Mex.Fis. 45 (1999) 36, arXiv:hep-ph/9901300. 22nd Symposium on Nuclear Physics, Oaxtepec, Morelos, Mexico, 5-8 Jan 1999.
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18 - Phenomenology - Type II - SN1987A

[18-1]
Revisiting Supernova 1987A Constraints on Dark Photons, Jae Hyeok Chang, Rouven Essig, Samuel D. McDermott, JHEP 1701 (2017) 107, arXiv:1611.03864.
[Chang:2016ntp]
[18-2]
New analysis for the correlation between gravitational waves and neutrino detectors during SN1987A, P. Galeotti, G. Pizzella, Eur.Phys.J. C76 (2016) 426, arXiv:1603.05076.
[Galeotti:2016uum]
[18-3]
The Mont Blanc mystery solved? A $m^2=-0.28 keV^2$ neutrino, Robert Ehrlich, Astropart.Phys. 85 (2016) 43-49, arXiv:1602.09043.
[Ehrlich:2016ljp]
[18-4]
Neutrino Signal of Collapse-Induced Thermonuclear Supernovae: The Case for Prompt Black Hole Formation in SN1987A, Kfir Blum, Doron Kushnir, Astrophys.J. 828 (2016) 31, arXiv:1601.03422.
[Blum:2016afe]
[18-5]
Nucleon-nucleon bremsstrahlung of dark gauge bosons and revised supernova constraints, Ermal Rrapaj, Sanjay Reddy, Phys. Rev. C94 (2016) 045805, arXiv:1511.09136.
[Rrapaj:2015wgs]
[18-6]
Supernova 1987A: neutrino-driven explosions in three dimensions and light curves, Victor Utrobin, Annop Wongwathanarat, H.-Thomas Janka, Ewald Mueller, arXiv:1412.4122, 2014.
[1412.4122]
[18-7]
Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles, Alexandre Payez et al., JCAP 1502 (2015) 006, arXiv:1410.3747.
[Payez:2014xsa]
[18-8]
Comparative analysis of SN1987A antineutrino fluence, Francesco Vissani, J. Phys. G42 (2015) 013001, arXiv:1409.4710.
[Vissani:2014doa]
[18-9]
Signatures of Neutrino Cooling in the SN1987A Scenario, Cristian G. Bernal, Nissim Fraija, Hidalgo-Gamez A. M, Mon.Not.Roy.Astron.Soc. 442 (2014) 239, arXiv:1402.6292.
[Bernal:2014cca]
[18-10]
Evidence for two neutrino mass eigenstates from SN 1987A and the possibility of superluminal neutrinos, Robert Ehrlich, Astropart.Phys. 35 (2012) 625-628, arXiv:1111.0502.
[Ehrlich:2011kb]
[18-11]
Neutrino mass bound in the standard scenario for supernova electronic antineutrino emission, Giulia Pagliaroli, Fernando Rossi-Torres, Francesco Vissani, Astropart. Phys. 33 (2010) 287-291, arXiv:1002.3349.
[Pagliaroli:2010ik]
[18-12]
The likelihood for supernova neutrino analyses, A. Ianni et al., Phys. Rev. D80 (2009) 043007, arXiv:0907.1891.
[Ianni:2009bd]
[18-13]
Active and Sterile Neutrino Emission and SN1987A Pulsar Velocity, Leonard S Kisslinger, Sandip Pakvasa, arXiv:0906.4117, 2009.
[Kisslinger:2009xb]
[18-14]
Could the compact remnant of SN 1987A be a quark star?, T. C. Chan et al., Astrophys. J. 695 (2009) 732-746, arXiv:0902.0653.
[Chan:2009mw]
[18-15]
Bounds on the Parameter of Noncommutativity from Supernova SN1987A, Mansour Haghighat, Phys. Rev. D79 (2009) 025011, arXiv:0901.1069.
[Haghighat:2009pv]
[18-16]
Improved analysis of SN1987A antineutrino events, G. Pagliaroli, F. Vissani, M.L. Costantini, A. Ianni, Astropart.Phys. 31 (2009) 163-176, arXiv:0810.0466.
[Pagliaroli:2008ur]
[18-17]
How much can we learn from SN1987A events? Or: An analysis with a two-Component model for the antineutrino signal, F. Vissani, G. Pagliaroli, arXiv:0807.1301, 2008.
[Vissani:2008ac]
[18-18]
Bounds on large extra dimensions from photon fusion process in SN1987A, V. H. Satheeshkumar, P. K. Suresh, JCAP 0806 (2008) 011, arXiv:0805.3429.
[Satheeshkumar:2008fb]
[18-19]
Analysis of Neutrino Signals from SN1987A, G. Pagliaroli, M.L. Costantini, F. Vissani, IFAE 2007 (2008) Proceedings. Edited by G. Carlino, arXiv:0804.4598.
[Pagliaroli:2008qi]
[18-20]
SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels, Leonard S. Kisslinger, Sandip Pakvasa, arXiv:0802.1689, 2008.
[Kisslinger:2008rx]
[18-21]
Constraints on Astro-unparticle Physics from SN 1987A, Sukanta Dutta, Ashok Goyal, JCAP 0803 (2008) 027, arXiv:0712.0145.
[Dutta:2007tz]
[18-22]
Statistical analysis of neutrino events from SN1987A neutrino burst: estimation of the electron antineutrino mass, B. I. Goryachev, arXiv:0709.4627, 2007.
[Goryachev:2007xg]
[18-23]
Unparticle constraints from SN1987A, Steen Hannestad, Georg Raffelt, Yvonne Y. Y. Wong, Phys. Rev. D76 (2007) 121701, arXiv:0708.1404.
[Hannestad:2007ys]
[18-24]
Supernovae as Probes of Extra Dimensions, V. H. Satheesh Kumar, P. K. Suresh, P. K. Das, AIP Conf. Proc. 939 (2007) 258-262, arXiv:0706.3551.
[SatheeshKumar:2007gb]
[18-25]
The first second of SN1987A neutrino emission, G. Pagliaroli, M.L. Costantini, A. Ianni, F. Vissani, arXiv:0705.4032, 2007.
[Pagliaroli:2007sd]
[18-26]
High resolution spectroscopy of the line emission from the inner circumstellar ring of SN 1987A and its hot spots, Per Groeningsson et al., Astron.Astrophys. (2007), arXiv:astro-ph/0703788.
[Groeningsson:2007nh]
[18-27]
Neutrino Spectrum from SN 1987A and from Cosmic Supernovae, Hasan Yuksel, John F. Beacom, Phys. Rev. D76 (2007) 083007, arXiv:astro-ph/0702613.
[Yuksel:2007mn]
[18-28]
Magnetic field in supernova remnant SN 1987A, E.G. Berezhko, L.T. Ksenofontov, Astrophys. J. 650 (2006) L59-L62, arXiv:astro-ph/0608586.
[Berezhko:2006vv]
[18-29]
Is there a problem with low energy SN1987A neutrinos?, Maria Laura Costantini, Aldo Ianni, Giulia Pagliaroli, Francesco Vissani, JCAP 0705 (2007) 014, arXiv:astro-ph/0608399.
[Costantini:2006xd]
[18-30]
Constraints on neutrino mixing angle $\theta_{13}$ and Supernova neutrino fluxes from the LSD neutrino signal from SN1987A, Oleg Lychkovskiy, arXiv:hep-ph/0604113, 2006.
[Lychkovskiy:2006yw]
[18-31]
Evolution of the Reverse Shock Emission from SNR 1987A, Kevin Heng et al., Astrophys. J. 644 (2006) 959-970, arXiv:astro-ph/0603151.
[Heng:2006nt]
[18-32]
Lower neutrino mass bound from SN1987A data and quantum geometry, G. Lambiase, G. Papini, R. Punzi, G. Scarpetta, Class. Quant. Grav. 23 (2006) 1347-1358, arXiv:gr-qc/0512154.
[Lambiase:2005ui]
[18-33]
New analysis of the SN 1987A neutrinos with a flexible spectral shape, Alessandro Mirizzi, Georg G. Raffelt, Phys. Rev. D72 (2005) 063001, arXiv:astro-ph/0508612.
[Mirizzi:2005tg]
[18-34]
The Three-Dimensional Circumstellar Environment of SN 1987A, Ben E. K. Sugerman et al., Astrophys. J. Suppl. 159 (2005) 60-99, arXiv:astro-ph/0502378.
[Sugerman:2005dr]
[18-35]
The Light Curve of Supernova 1987A: The Structure of the Presupernova and Radioactive Nickel Mixing, V. P. Utrobin, Astron. Lett. 30 (2004) 293, arXiv:astro-ph/0406410.
[Utrobin:2004rt]
[18-36]
SN1987A and the properties of neutrino burst, Maria Laura Costantini, Aldo Ianni, Francesco Vissani, Phys. Rev. D70 (2004) 043006, arXiv:astro-ph/0403436.
[Costantini:2004ry]
[18-37]
Constraints on a Putative Pulsar in SN 1987A, H. Ogelman, M.A. Alpar, Astrophys. J. 603 (2004) L33, arXiv:astro-ph/0402147.
[Ogelman:2004iu]
[18-38]
Neutrinos from SN1987A: flavor conversion and interpretation of results, C. Lunardini, A. Yu. Smirnov, Astropart. Phys. 21 (2004) 703, arXiv:hep-ph/0402128.
[Lunardini:2004bj]
[18-39]
A Rotating Collapsar and Possible Interpretation of the LSD Neutrino Signal from SN 1987A, V.S. Imshennik, O.G. Ryazhskaya, Astron. Lett. 30 (2004) 14, arXiv:astro-ph/0401613.
[Imshennik:2004iya]
[18-40]
Evidence of non-zero mass features for the neutrinos emitted at Supernova LMC-'87A, Humiaki Huzita, arXiv:hep-ph/0212337, 2002.
[Huzita:2002ia]
[18-41]
Supernova 1987A did not test the neutrino mass hierarchy, V. Barger, D. Marfatia, B. P. Wood, Phys. Lett. B532 (2002) 19-28, arXiv:hep-ph/0202158.
[Barger:2002px]
[18-42]
SN1987A and the status of oscillation solutions to the solar neutrino problem, M. Kachelriess, A. Strumia, R. Tomas, J. W. F. Valle, Phys. Rev. D65 (2002) 073016, arXiv:hep-ph/0108100.
[Kachelriess:2001sg]
[18-43]
Bayesian analysis of neutrinos observed from supernova SN 1987A, Thomas J. Loredo, Don Q. Lamb, Phys. Rev. D65 (2002) 063002, arXiv:astro-ph/0107260.
From the abstract: We present a Bayesian analysis of the energies and arrival times of the neutrinos from supernova SN 1987A detected by the Kamiokande II, IMB, and Baksan detectors, and find strong evidence for two components in the neutrino signal: a long time scale component from thermal Kelvin-Helmholtz cooling of the nascent neutron star, and a brief ($\sim 1$ s), softer component similar to that expected from emission by accreting material in the delayed supernova scenario. In the context of this model, we show that the data constrain the electron antineutrino rest mass to be less than 5.7~eV with 95% probability.
[Loredo:2001rx]
[18-44]
Large lepton mixing and supernova 1987A, M. Kachelriess, R. Tomas, J. W. F. Valle, JHEP 01 (2001) 030, arXiv:hep-ph/0012134.
[Kachelriess:2000fe]
[18-45]
Inverted hierarchy of neutrino masses disfavored by supernova 1987A, Hisakazu Minakata, Hiroshi Nunokawa, Phys. Lett. B504 (2001) 301-308, arXiv:hep-ph/0010240.
[Minakata:2000rx]
[18-46]
Neutrinos from SN1987A, Earth matter effects and the LMA solution of the solar neutrino problem, C. Lunardini, A. Yu. Smirnov, Phys. Rev. D63 (2001) 073009, arXiv:hep-ph/0009356.
[Lunardini:2000sw]
[18-47]
SN1987A: A testing ground for the KARMEN anomaly, I. Goldman, R. Mohapatra, S. Nussinov, Phys. Lett. B481 (2000) 151-159, arXiv:hep-ph/9912465.
[Goldman:1999hg]
[18-48]
Contact interactions involving right-handed neutrinos and SN 1987A, J. A. Grifols, E. Masso, R. Toldra, Phys. Rev. D57 (1998) 2005-2008, arXiv:hep-ph/9707531.
[Grifols:1997iy]
[18-49]
Gamma rays from SN1987A due to pseudoscalar conversion, J. A. Grifols, E. Masso, R. Toldra, Phys. Rev. Lett. 77 (1996) 2372-2375, arXiv:astro-ph/9606028.
[Grifols:1996id]
[18-50]
Gamma-rays and the decay of neutrinos from SN1987A, Andrew H. Jaffe, Michael S. Turner, Phys. Rev. D55 (1997) 7951-7959, arXiv:astro-ph/9601104.
[Jaffe:1995sw]
[18-51]
Bounds on the neutrino magnetic moment from SN1987A, A. Goyal, S. Dutta, S. R. Choudhury, Phys. Lett. B346 (1995) 312-316.
[Goyal:1995yd]
[18-52]
Testing special relativity with SN1987A neutrino pulses, E. Atzmon, S. Nussinov, Phys. Lett. B328 (1994) 103-108.
[Atzmon:1994ch]
[18-53]
Constraints from nucleosynthesis and SN1987A on majoron emitting double beta decay, Sanghyeon Chang, Kiwoon Choi, Phys. Rev. D49 (1994) 12-15, arXiv:hep-ph/9303243.
[Chang:1993yp]
[18-54]
Dirac neutrinos and SN1987A, Michael S. Turner, Phys. Rev. D45 (1992) 1066-1075.
[Turner:1992ax]
[18-55]
Constraints to the decays of Dirac neutrinos from SN1987A, Scott Dodelson, Joshua A. Frieman, Michael S. Turner, Phys. Rev. Lett. 68 (1992) 2572-2575.
[Dodelson:1992tv]
[18-56]
Massive Dirac neutrinos and SN1987A, Adam Burrows, Raj Gandhi, MIchael S. Turner, Phys. Rev. Lett. 68 (1992) 3834-3837.
[Burrows:1992ec]
[18-57]
E(6) models confront SN1987A, J. A. Grifols, E. Masso, T. G. Rizzo, Phys. Rev. D42 (1990) 3293-3296.
[Grifols:1990tk]
[18-58]
limits on the muon-neutrino and tau-neutrino masses from SN1987A, J. A. Grifols, E. Masso, Phys. Lett. B242 (1990) 77.
[Grifols:1990jn]
[18-59]
Massive Dirac neutrinos and the SN1987A signal, Raj Gandhi, Adam Burrows, Phys. Lett. B246 (1990) 149-155.
[Gandhi:1990bq]
[18-60]
Neutrino helicity flips via electroweak interactions and SN1987A, K. J. F. Gaemers, R. Gandhi, J. m. Lattimer, Phys. Rev. D40 (1989) 309.
[Gaemers:1989fp]
[18-61]
Constraints on decaying right-handed majorana neutrinos from SN1987A observations, R. N. Mohapatra, S. Nussinov, Phys. Rev. D39 (1989) 1378-1385.
[Mohapatra:1989su]
[18-62]
axions and SN1987A, Adam Burrows, Michael S. Turner, R. P. Brinkmann, Phys. Rev. D39 (1989) 1020.
[Burrows:1989ah]
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comment on 'constraints on the majoron interactions from the supernova SN1987A.', Y. Aharonov, F. T. Avignone, S. Nussinov, Phys. Rev. D39 (1989) 985.
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Comment: The author assumed that electron antineutrinos are emitted from the supernova in a very short time, of the order of 0.1 sec. This assumption is contrary to the standard understanding of the core-collapse supernova mechanism, according to which electron antineutrinos are emitted during the cooling phase of the proto-neutron star on a time scale of about 10 sec (see Supernovae). Moreover, the existence of neutrinos with masses of about 4 eV and 22 eV which have large mixing with the electron antineutrino is excluded by the Tritium upper bound on the effective electron neutrino mass (see Neutrino Mass: Direct Measurements). (C.G.).
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limits on the neutrino magnetic moment from SN1987A, J. M. Lattimer, J. Cooperstein, Phys. Rev. Lett. 61 (1988) 23-26.
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19 - Phenomenology - Type II - SN1987A - Conference Proceedings

[19-1]
Neutrinos from SN 1987a. A Puzzle Revisited, Gerd Schatz, J. Phys. Conf. Ser. 632 (2015) 012024, arXiv:1507.07107. 24th European Cosmic Ray Symposium Kiel 2014.
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Reexamination of a Bound on the Dirac Neutrino Magnetic Moment from the Supernova Neutrino Luminosity, A.V. Kuznetsov, N.V. Mikheev, A.A. Okrugin, arXiv:1011.2100, 2010. XVI International Seminar Quarks'2010, Kolomna, Moscow Region, June 6-12, 2010.
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[19-3]
What is the issue with SN1987A neutrinos?, F. Vissani, M.L. Costantini, W. Fulgione, A. Ianni, G. Pagliaroli, arXiv:1008.4726, 2010. Vulcano Workshop 2010: Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, May 24-29, 2010.
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Analysis of the SN1987A two-stage explosion hypothesis with account for the MSW neutrino flavour conversion, Oleg Lychkovskiy, arXiv:0707.2508, 2007. Rencontres de Moriond EW 2007, 10-17 March 2007.
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Neutrino events from SN1987A revisited, B. Bekman, J. Holeczek, J. Kisiel, Acta Phys. Polon. B37 (2006) 269, arXiv:hep-ph/0511271. XXIX Mazurian Lakes Conference on Physics, August 30 - September 6, 2005, Piaski, Poland.
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SN 1987A: The Unusual Explosion of a Normal Type II Supernova, Nino Panagia, ASP Conf.Ser. (2004), arXiv:astro-ph/0410275. International Conference '1604-2004 Supernovae as Cosmological Lighthouses' (Padova, Italy, June 16-19, 2004).
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Comment: {Same as in [18-76].
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Mass determination of neutrinos, H. Y. Chiu, 1987. IN 'FAIRFAX 1987, PROCEEDINGS, SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD' 185-193.
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20 - Phenomenology - Type II - Simulations

[20-1]
Supernova Simulations from a 3D Progenitor Model - Impact of Perturbations and Evolution of Explosion Properties, B. Muller, T. Melson, A. Heger, H.-Th. Janka, arXiv:1705.00620, 2017.
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Light curve analysis of ordinary type IIP supernovae based on neutrino-driven explosion simulations in three dimensions, V. P. Utrobin, A. Wongwathanarat, H.-Th. Janka, E. Mueller, arXiv:1704.03800, 2017.
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A Parametric Study of the Acoustic Mechanism for Core-Collapse Supernovae, A. Harada, H. Nagakura, W. Iwakami, S. Yamada, Astrophys.J. 839 (2017) 28, arXiv:1704.02984.
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The effect upon neutrinos of core-collapse supernova accretion phase turbulence, James P. Kneller, Mithi de los Reyes, arXiv:1702.06951, 2017.
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Electron-Capture and Low-Mass Iron-Core-Collapse Supernovae: New Neutrino-Radiation-Hydrodynamics Simulations, David Radice, Adam Burrows, David Vartanyan, M. Aaron Skinner, Joshua C. Dolence, arXiv:1702.03927, 2017.
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Six-Dimensional Simulations of Core-Collapse Supernovae with Full Boltzmann Neutrino Transport, Hiroki Nagakura et al., arXiv:1702.01752, 2017.
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Flavor-dependent neutrino angular distribution in core-collapse supernovae, Irene Tamborra, Lorenz Huedepohl, Georg Raffelt, Hans-Thomas Janka, Astrophys.J. 839 (2017) 2, arXiv:1702.00060.
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The Gravitational Wave Signal of a Core Collapse Supernova Explosion of a 15M$_\odot$ Star, Konstantin N. Yakunin et al., arXiv:1701.07325, 2017.
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Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions, Shinya Wanajo, Bernhard Muller, Hans-Thomas Janka, Alexander Heger, arXiv:1701.06786, 2017.
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[20-10]
Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism, Adam Burrows, David Vartanyan, Joshua C. Dolence, M. Aaron Skinner, David Radice, arXiv:1611.05859, 2016.
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Production and Distribution of 44Ti and 56Ni in a Three-dimensional Supernova Model Resembling Cassiopeia A, A. Wongwathanarat, H.-Th. Janka, E. Mueller, E. Pllumbi, S. Wanajo, Astrophys.J. 842 (2017) 13, arXiv:1610.05643.
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Gravitational Wave Signals from 3D Neutrino Hydrodynamics Simulations of Core-Collapse Supernovae, Haakon Andresen, Bernhard Mueller, Ewald Mueller, Hans-Thomas Janka, Mon.Not.Roy.Astron.Soc. 468 (2017) 2032-2051, arXiv:1607.05199.
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A new gravitational-wave signature of SASI activities in non-rotating supernova cores, Takami Kuroda, Kei Kotake, Tomoya Takiwaki, Astrophys.J. 829 (2016) L14, arXiv:1605.09215.
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Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars II. The Implementation of moving-mesh for neutron star kicks, Hiroki Nagakura et al., Astrophys.J.Suppl. 229 (2017) 42, arXiv:1605.00666.
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General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae, Luke F. Roberts et al., arXiv:1604.07848, 2016.
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Parametric initial conditions for core-collapse supernova simulations, Yudai Suwa, Ewald Muller, Mon.Not.Roy.Astron.Soc. 460 (2016) 2664-2674, arXiv:1603.05578.
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Three-dimensional hydrodynamics simulations of rapidly rotating core-collapse supernovae: finding a new class of rotation-aided explosions, Tomoya Takiwaki, Kei Kotake, Yudai Suwa, Mon.Not.Roy.Astron.Soc. 461 (2016) L112, arXiv:1602.06759.
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[20-18]
Erratum: Progenitor-explosion connection and remnant birth masses for neutrino-driven supernovae of iron-core progenitors (2012, ApJ, 757, 69), Thomas Ertl, Marcella Ugliano, H.-Thomas Janka, Andreas Marek, Almudena Arcones, Astrophys.J. 821 (2016) 69, arXiv:1602.06327.
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Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae, Alexander Summa et al., Astrophys.J. 825 (2016) 6, arXiv:1511.07871.
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Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport, Evan O'Connor, Sean Couch, arXiv:1511.07443, 2015.
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[20-21]
Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations, David Radice et al., Astrophys.J. 820 (2016) 76, arXiv:1510.05022.
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[20-22]
Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions, Tuguldur Sukhbold, T. Ertl, S. E. Woosley, Justin M. Brown, H.-T. Janka, Astrophys.J. 821 (2016) 38, arXiv:1510.04643.
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[20-23]
Quantum Simulations of Nuclei and Nuclear Pasta with the Multi-resolution Adaptive Numerical Environment for Scientific Simulations, I. Sagert, G. I. Fann, F. J. Fattoyev, S. Postnikov, C. J. Horowitz, Phys. Rev. C93 (2016) 055801, arXiv:1509.06671.
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[20-24]
Stochasticity and efficiency of convection-dominated vs. SASI-dominated supernova explosions, Christian Y. Cardall, Reuben D. Budiardja, Astrophys. J. 813 (2015) L6, arXiv:1509.02494.
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[20-25]
A Comparative study of hyperon equations of state in supernova simulations, Prasanta Char, Sarmistha Banik, Debades Bandyopadhyay, Astrophys. J. 809 (2015) 116, arXiv:1508.01854.
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[20-26]
Jittering-jets explosion triggered by the standing accretion shock instability, Oded Papish, Avishai Gilkis, Noam Soker, arXiv:1508.00218, 2015.
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Neutrino-driven explosions of ultra-stripped type Ic supernovae generating binary neutron stars, Yudai Suwa, Takashi Yoshida, Masaru Shibata, Hideyuki Umeda, Koh Takahashi, Mon. Not. Roy. Astron. Soc. 454 (2015) 3073-3081, arXiv:1506.08827.
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[20-28]
The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D, Bernhard Muller, Mon. Not. Roy. Astron. Soc. 453 (2015) 287, arXiv:1506.05139.
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Gravitational Wave Signatures of Ab Initio Two-Dimensional Core Collapse Supernova Explosion Models for 12-25 Solar Masses Stars, Konstantin N. Yakunin et al., Phys. Rev. D92 (2015) 084040, arXiv:1505.05824.
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Three-dimensional core-collapse supernova simulated using a 15 $M_\odot$ projenitor, Eric J. Lentz et al., arXiv:1505.05110, 2015.
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Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport, Kuo-Chuan Pan, Matthias Liebendorfer, Matthias Hempel, Friedrich-Karl Thieleman, Astrophys. J. 817 (2016) 72, arXiv:1505.02513.
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Three-Dimensional Simulations of SASI- and Convection-Dominated Core-Collapse Supernovae, Rodrigo Fernandez, Mon. Not. Roy. Astron. Soc. 452 (2015) 2071-2086, arXiv:1504.07996.
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Neutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering, Tobias Melson et al., Astrophys. J. 808 (2015) L42, arXiv:1504.07631.
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The Three Dimensional Evolution to Core Collapse of a Massive Star, Sean M. Couch, Emmanouil Chatzopoulos, W. David Arnett, F.X. Timmes, Astrophys. J. 808 (2015) L21, arXiv:1503.02199.
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A New Multi-Energy Neutrino Radiation-Hydrodynamics Code in Full General Relativity and Its Application to Gravitational Collapse of Massive Stars, Takami Kuroda, Tomoya Takiwaki, Kei Kotake, Astrophys. J. Suppl. 222 (2016) 20, arXiv:1501.06330.
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A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics, Oliver Just, Martin Obergaulinger, H.-Thomas Janka, Mon. Not. Roy. Astron. Soc. 453 (2015) 3386-3413, arXiv:1501.02999.
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Pushing 1D CCSNe to explosions: model and SN 1987A, A. Perego et al., Astrophys. J. 806 (2015) 275, arXiv:1501.02845.
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Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection, Tobias Melson, Hans-Thomas Janka, Andreas Marek, Astrophys.J. 801 (2015) L24, arXiv:1501.01961.
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[20-39]
Recent Progress on Ascertaining the Core Collapse Supernova Explosion Mechanism, Anthony Mezzacappa et al., arXiv:1501.01688, 2015.
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Failure of a neutrino-driven explosion after core-collapse may lead to a thermonuclear supernova, Doron Kushnir, Boaz Katz, Astrophys. J. 811 (2015) 97, arXiv:1412.1096.
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An Open-Source Neutrino Radiation Hydrodynamics Code for Core-Collapse Supernovae, Evan O'Connor, Astrophys. J. Suppl. 219 (2015) 24, arXiv:1411.7058.
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Magnetohydrodynamic Turbulence Powered by Magnetorotational Instability in Nascent Proto-Neutron Stars, Youhei Masada, Tomoya Takiwaki, Kei Kotake, Astrophys.J. 798 (2015) L22, arXiv:1411.6705.
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Neutrino-driven Turbulent Convection and Standing Accretion Shock Instability in Three-Dimensional Core-Collapse Supernovae, E. Abdikamalov et al., Astrophys. J. 808 (2015) 70, arXiv:1409.7078.
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The Development of Explosions in Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 $M_\odot$ Stars, Stephen W. Bruenn et al., Astrophys. J. 818 (2016) 123, arXiv:1409.5779.
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Three-Dimensional Simulations of Core-Collapse Supernovae: From Shock Revival to Shock Breakout, Annop Wongwathanarat, Ewald Mueller, H.-Thomas Janka, Astron.Astrophys. 577 (2015) A48, arXiv:1409.5431.
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Non-Radial Instabilities and Progenitor Asphericities in Core-Collapse Supernovae, B. Mueller, H.-Th. Janka, Mon.Not.Roy.Astron.Soc. 448 (2015) 2141, arXiv:1409.4783.
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The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions, Sean M. Couch, Christian D. Ott, Astrophys.J. 799 (2015) 5, arXiv:1408.1399.
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Three-dimensional Boltzmann-Hydro code for core-collapse in massive stars I. special relativistic treatments, Hiroki Nagakura, Kohsuke Sumiyoshi, Shoichi Yamada, Astrophys.J.Suppl. 214 (2014) 16, arXiv:1407.5632.
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The criterion of supernova explosion revisited: the mass accretion history, Yudai Suwa, Shoichi Yamada, Tomoya Takiwaki, Kei Kotake, Astrophys. J. 816 (2016) 43, arXiv:1406.6414.
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Systematic Features of Axisymmetric Neutrino-Driven Core-Collapse Supernova Models in Multiple Progenitors, Ko Nakamura, Tomoya Takiwaki, Takami Kuroda, Kei Kotake, Publ.Astron.Soc.Jap. 67 (2015) 107, arXiv:1406.2415.
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Impacts of Rotation on Three-dimensional Hydrodynamics of Core-collapse Supernovae, Ko Nakamura, Takami Kuroda, Tomoya Takiwaki, Kei Kotake, Astrophys.J. 793 (2014) 45, arXiv:1403.7290.
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Two-Dimensional Core-Collapse Supernova Models with Multi-Dimensional Transport, Joshua C. Dolence, Adam Burrows, Weiqun Zhang, Astrophys.J. 800 (2015) 10, arXiv:1403.6115.
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Multi-dimensional Features of Neutrino Transfer in Core-Collapse Supernovae, K. Sumiyoshi, T. Takiwaki, H. Matsufuru, S. Yamada, Astrophys.J.Suppl. 216 (2015) 5, arXiv:1403.4476.
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MODA: a new algorithm to compute optical depths in multi-dimensional hydrodynamic simulations, A. Perego, E. Gafton, R. Cabezon, S. Rosswog, M. Liebendoerfer, Astron.Astrophys. 568 (2014) A11, arXiv:1403.1297.
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A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal, B. Mueller, H.-Th. Janka, Astrophys.J. 788 (2014) 82, arXiv:1402.3415.
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Application of the nuclear equation of state obtained by the variational method to core-collapse supernovae, H. Togashi, M. Takano, K. Sumiyoshi, K. Nakazato, PTEP 2014 (2014) 023D05, arXiv:1401.5579.
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Chaos and Turbulent Nucleosynthesis Prior to a Supernova Explosion, W. David Arnett, Casey Meakin, Maxime Viallet, arXiv:1312.3279, 2013.
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From supernovae to neutron stars, Yudai Suwa, Publ.Astron.Soc.Jap. 66 (2014) L1, arXiv:1311.7249.
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Gravitational wave signatures in black-hole forming core collapse, Pablo Cerda-Duran, Nicolas DeBrye, Miguel A Aloy, Jose A Font, Martin Obergaulinger, Astrophys.J. 779 (2013) L18, arXiv:1310.8290.
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High-Resolution Three-Dimensional Simulations of Core-Collapse Supernovae in Multiple Progenitors, Sean M. Couch, Evan P. O'Connor, Astrophys.J. 785 (2014) 123, arXiv:1310.5728.
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Porting Large HPC Applications to GPU Clusters: The Codes GENE and VERTEX, Tilman Dannert, Andreas Marek, Markus Rampp, arXiv:1310.1485, 2013.
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Characterizing SASI- and Convection-Dominated Core-Collapse Supernova Explosions in Two Dimensions, Rodrigo Fernandez, Bernhard Mueller, Thierry Foglizzo, Hans-Thomas Janka, Mon.Not.Roy.Astron.Soc. 440 (2014) 2763, arXiv:1310.0469.
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New equations of state in core-collapse supernova simulations, Matthias Hempel, Tobias Fischer, Jurgen Schaffner-Bielich, Matthias Liebendorfer, Astrophys. J. 748 (2012) 70, arXiv:1108.0848.
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From the abstract: Accurate neutrino transport has been built into spherically symmetric simulations of stellar core collapse and postbounce evolution. The results of such simulations agree that spherically symmetric models with standard microphysical input fail to explode by the delayed, neutrino-driven mechanism.
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Core-Collapse Supernova Mechanism - Importance of Rotation, A. Odrzywolek, M. Kutschera, M. Misiaszek, K. Grotowski, Acta Phys.Polon.34:2791 (2003), arXiv:astro-ph/0310047.
[Odrzywolek:2003qc]
[20-165]
3-Dimensional Core-Collapse, Chris L. Fryer, Michael S. Warren, Astrophys. J. 601 (2004) 391-404, arXiv:astro-ph/0309539.
[Fryer:2003jj]
[20-166]
Pulsar Recoil by Large-Scale Anisotropies in Supernova Explosions, L. Scheck, T. Plewa, Hans-Thomas Janka, K. Kifonidis, E. Mueller, Phys. Rev. Lett. 92 (2004) 011103, arXiv:astro-ph/0307352.
[Scheck:2003rw]
[20-167]
Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae, M. Limongi, A. Chieffi, Astrophys. J. 592 (2003) 404, arXiv:astro-ph/0304185.
[Limongi:2003ui]
[20-168]
Improved Models of Stellar Core Collapse and Still no Explosions: What is Missing?, R. Buras, M. Rampp, H.-Th. Janka, K. Kifonidis, Phys. Rev. Lett. 90 (2003) 241101, arXiv:astro-ph/0303171.
[Buras:2003sn]
[20-169]
Electron capture rates on nuclei and implications for stellar core collapse, K. Langanke et al., Phys. Rev. Lett. 90 (2003) 241102, arXiv:astro-ph/0302459.
[Langanke:2003ii]
[20-170]
Non-spherical Core Collapse Supernovae I. Neutrino-Driven Convection, Rayleigh-Taylor Instabilities, and the Formation and Propagation of Metal Clumps, K. Kifonidis, T. Plewa, H.-Th. Janka, E. Mueller, Astron. Astrophys. 408 (2003) 621, arXiv:astro-ph/0302239.
[Kifonidis:2003fv]
[20-171]
Shock breakout in core-collapse supernovae and its neutrino signature, Todd A. Thompson, Adam Burrows, Philip A. Pinto, Astrophys. J. 592 (2003) 434, arXiv:astro-ph/0211194.
[Thompson:2002mw]
[20-172]
Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae, J. M. Blondin, A. Mezzacappa, C. DeMarino, Astrophys. J. 584 (2003) 971, arXiv:astro-ph/0210634.
[Blondin:2002sm]
[20-173]
A finite difference representation of neutrino radiation hydrodynamics for spherically symmetric general relativistic supernova simulations, M. Liebendoerfer et al., Astrophys. J. Suppl. 150 (2004) 263, arXiv:astro-ph/0207036.
[Liebendoerfer:2002xn]
[20-174]
Modeling Core-Collapse Supernovae in Three Dimensions, C.L. Fryer, M.S. Warren, Astrophys. J. 574 (2002) L65-L68, arXiv:astro-ph/0206017.
[Fryer:2002zw]
[20-175]
Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations, H.-T. Janka M. Rampp, Astron. Astrophys. 396 (2002) 361, arXiv:astro-ph/0203101.
[Rampp:2002bq]
[20-176]
NewtonPlus: Approximate Relativity for Supernova Simulations, Christian Y. Cardall, Anthony Mezzacappa, Matthias Liebendorfer, Phys. Rev.D (2001), arXiv:astro-ph/0106105.
[Cardall:2001fu]
[20-177]
Spherical collapse of supermassive stars: neutrino emission and gamma-ray bursts, Felix Linke, Jose A. Font, Hans-Thomas Janka, E. Mueller, Philippos Papadopoulos, Astron.Astrophys. (2001), arXiv:astro-ph/0103144.
[Linke:2001mq]
[20-178]
General Relativistic Effects in the Core Collapse Supernova Mechanism, S. W. Bruenn, K. R. De Nisco, A. Mezzacappa, Astrophys. J. 560 (2001) 326, arXiv:astro-ph/0101400.
[Bruenn:2001vu]
[20-179]
Conservative General Relativistic Radiation Hydrodynamics in Spherical Symmetry and Comoving Coordinates, Matthias Liebendorfer, Anthony Mezzacappa, Friedrich-Karl Thielemann, Phys. Rev. D63 (2001) 104003, arXiv:astro-ph/0012201.
[Liebendoerfer:2000fw]
[20-180]
Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae, H.-Th. Janka, Astron. Astrophys. 368 (2000) 527-560, arXiv:astro-ph/0008432.
[Janka:2000bt]
[20-181]
Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport, Matthias Liebendorfer et al., Phys. Rev. D63 (2001) 103004, arXiv:astro-ph/0006418.
From the article: We investigate the confluence of (i) matter and radiation in a deeper effective gravitational potential, (ii) a GR core hydrodynamic structure that acts as a more intense neutrino source, and (iii) an increased heating efficiency obtained from accurate three-flavor Boltzmann neutrino transport. However, we find that the combination of these ingredients does not result in a supernova explosion. Our model shares this outcome with recent simulations that investigated a subset of these issues (Rampp and Janka [20-182], Mezzacappa and others [20-183], Bruenn and others [20-178]).
[Liebendoerfer:2000cq]
[20-182]
Spherically symmetric simulation with Boltzmann neutrino transport of core collapse and post-bounce evolution of a 15 solar mass star, Markus Rampp, H. Thomas Janka, Astrophys. J. 539 (2000) L33-L36, arXiv:astro-ph/0005438.
[Rampp:2000ws]
[20-183]
The Simulation of a Spherically Symmetric Supernova of a 13 Solar Mass Star with Boltzmann Neutrino Transport, and Its Implications for the Supernova Mechanism, Anthony Mezzacappa et al., Phys. Rev. Lett. 86 (2001) 1935-1938, arXiv:astro-ph/0005366.
From the abstract: In this model, a supernova explosion is not obtained.
[Mezzacappa:2000jb]
[20-184]
A new algorithm for supernova neutrino transport and some applications, A. Burrows, T. Young, P. Pinto, R. Eastman, T. A. Thompson, Astrophys. J. 539 (2000) 865-887.
[Burrows:1999es]
[20-185]
Future detection of supernova neutrino burst and explosion mechanism, T. Totani, K. Sato, H. E. Dalhed, J. R. Wilson, Astrophys. J. 496 (1998) 216-225, arXiv:astro-ph/9710203.
From the abstract: We mainly discuss the detectability of the signatures of the delayed explosion mechanism in the time evolution of the $\bar\nu_e$ luminosity and spectrum.
[Totani:1997vj]
[20-186]
An investigation of neutrino-driven convection and the core collapse supernova mechanism using multigroup neutrino transport, A. Mezzacappa et al., Astrophys.J.Lett. (1996), arXiv:astro-ph/9612107.
[Mezzacappa:1996ae]
[20-187]
On the nature of core collapse supernova explosions, Adam Burrows, John Hayes, Bruce A. Fryxell, Astrophys. J. 450 (1995) 830, arXiv:astro-ph/9506061.
[Burrows:1995ww]
[20-188]
Neutrino Emission from Type II Supernovae: The First 100 Milliseconds, E. Myra, A. Burrows, Astrophys. J. 364 (1989) 222.
[Myra-Burrows-ApJ364-222-1989]
[20-189]
The Hydrodynamic Behavior of Supernovae Explosions, S. A. Colgate, R. H. White, Astrophys. J. 143 (1966) 626-681.
[Colgate-White-ApJ143-1966]

21 - Phenomenology - Type II - Simulations - Conference Proceedings

[21-1]
Spatial distribution of radionuclides in 3D models of SN 1987A and Cas A, H.-Thomas Janka, Michael Gabler, Annop Wongwathanarat, arXiv:1705.01159, 2017. SN 1987A, 30 years later, IAU Symposium No. 331, 2017.
[Janka:2017nhh]
[21-2]
Multi-dimensional Core-Collapse Supernova Simulations with Neutrino Transport, Kuo-Chuan Pan, Matthias Liebendorfer, Matthias Hempel, Friedrich-Karl Thielemann, JPS Conf.Proc. 14 (2017) 020703, arXiv:1701.06701. Nuclei in the Cosmos XIV, Niigata, Japan (2016).
[Pan:2017nzj]
[21-3]
PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry: Nucleosynthesis Yields, Sanjana Sinha, Carla Frohlich, Kevin Ebinger, Albino Perego, Matthias Hempel, Marius Eichler, Matthias Liebendorfer, Friedrich-Karl Thielemann, JPS Conf.Proc. 14 (2017) 020608, arXiv:1701.05203. 14th International Symposium on Nuclei in the Cosmos (NIC-XIV).
[Sinha:2017hnn]
[21-4]
Constraining the supersaturation density equation of state from core-collapse supernova simulations - Excluded volume extension of the baryons, Tobias Fischer, Eur.Phys.J. A52 (2016) 54, arXiv:1604.01629. EPJA topical issue 'Exotic Matter in Neutron Stars'.
[Fischer:2016jkc]
[21-5]
Expected impact from weak reactions with light nuclei in core-collapse supernova simulations, T. Fischer et al., EPJ Web Conf. 109 (2016) 06002, arXiv:1512.00193. OMEG 2015.
[Fischer:2015sll]
[21-6]
Multimessengers from 3D Core-Collapse Supernovae, Konstantin N. Yakunin et al., arXiv:1507.05901, 2015. 50th Rencontres de Moriond on Gravitation: La Thuile, Italy, March 21-28, 2014.
[Yakunin:2015nma]
[21-7]
A Neutrino-Driven Core Collapse Supernova Explosion of a 15 M Star, Anthony Mezzacappa et al., arXiv:1507.05680, 2015. ASTRONUM 2014.
[Mezzacappa:2015bma]
[21-8]
Two- and Three-Dimensional Multi-Physics Simulations of Core Collapse Supernovae: A Brief Status Report and Summary of Results from the 'Oak Ridge' Group, Anthony Mezzacappa et al., ASP Conf.Ser. 488 (2014) 102, arXiv:1405.7075. ASTRONUM 2013.
[Mezzacappa:2014era]
[21-9]
Towards Petaflops Capability of the VERTEX Supernova Code, Andreas Marek, Markus Rampp, Florian Hanke, Hans-Thomas Janka, arXiv:1404.1719, 2014.
[1404.1719]
[21-10]
Two- and three-dimensional simulations of core-collapse supernovae with CHIMERA, Eric J. Lentz et al., PoS NICXII NICXII (2012) 208, arXiv:1301.1326. 12th Symposium on Nuclei in the Cosmos. 5-12 August 2012.
[Lentz:2013da]
[21-11]
Numerical modeling of core-collapse supernovae and compact objects, K. Sumiyoshi, IAU Symp. 291 (2013) 67, arXiv:1212.6131. IAUS 291 'Neutron Stars and Pulsars: Challenges and Opportunities after 80 years'.
[Sumiyoshi:2012un]
[21-12]
Exploding SNe with jets: time-scales, Oded Papish, Noam Soker, IAU Symp. 279 (2012) 377, arXiv:1204.2560. IAU Symposium No. 279, 2012.
[Papish:2012qx]
[21-13]
General Relativistic Explosion Models of Core-Collapse Supernovae, Bernhard Mueller, Andreas Marek, Hans-Thomas Janka, Harald Dimmelmeier, ASP Conf.Ser. 459 (2012) 137, arXiv:1112.1920.
[Mueller:2011aa]
[21-14]
Studies of Stellar Collapse and Black Hole Formation with the Open-Source Code GR1D, Christian D. Ott, Evan O'Connor, AIP Conf. Proc. 1269 (2010) 166-173, arXiv:1011.0005. OMEG10 Symposium, Osaka, Japan, March 8-10, 2010.
[Ott:2010mk]
[21-15]
Mechanisms of Core-Collapse Supernovae & Simulation Results from the CHIMERA Code, S. W. Bruenn et al., AIP Conference Proceedings 1111 (2010) 593-601, arXiv:1002.4909. Probing Stellar Populations Out To The Distant Universe: Cefalu 2008.
[Bruenn:2010ae]
[21-16]
PoS NICXI (2010) 082.
[Arcones:2010nj]
[21-17]
Computational Models of Stellar Collapse and Core-Collapse Supernovae, C. D. Ott et al., J. Phys. Conf. Ser. 180 (2009) 012022, arXiv:0907.4043. DOE/SciDAC 2009.
[Ott:2009ii]
[21-18]
Nucleosynthesis Calculations from Core-Collapse Supernovae, Christopher L. Fryer et al. (The NuGrid), arXiv:0811.4648, 2008. 10th Symposium on Nuclei in the Cosmos (NIC X), July 27 - August 1 2008, Mackinack Island, Michigan, USA.
[Fryer:2008ti]
[21-19]
Supernova explosions and the birth of neutron stars, H.-Th. Janka, A. Marek, B. Mueller, L. Scheck, AIP Conf. Proc. 983 (2008) 369-378, arXiv:0712.3070. 40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More, August 12-17, 2007, McGill Univ., Montreal, Canada.
[Janka:2007hi]
[21-20]
Nuclear physics with spherically symmetric supernova models, M. Liebendoerfer, T. Fischer, C. Frohlich, F.-K. Thielemann, S. Whitehouse, J. Phys. G35 (2008) 014056, arXiv:0708.4296. NPA III, Dresden 2007.
[Liebendoerfer:2007hq]
[21-21]
Multi-Dimensional Explorations in Supernova Theory, Adam Burrows, Luc Dessart, Christian D. Ott, Eli Livne, Phys. Rept. 442 (2007) 23-37, arXiv:astro-ph/0612460. Centennial Festschrift for Hans Bethe, 2006.
[Burrows:2006ci]
[21-22]
Collapse and black hole formation in magnetized, differentially rotating neutron stars, Branson C. Stephens et al., Class. Quant. Grav. 24 (2007) S207-S220, arXiv:gr-qc/0610103. New Frontiers in Numerical Relativity, the Albert Einstein Institute, Potsdam, July 17-21, 2006.
[Stephens:2006cn]
[21-23]
Efficient approximations of neutrino physics for three-dimensional simulations of stellar core collapse, M. Liebendoerfer, U.-L. Pen, C. Thompson, PoS NIC-IX (2006) 132, arXiv:astro-ph/0609651. Nuclei in the Cosmos IX, Geneva, June 25-30.
[Liebendorfer:2006et]
[21-24]
Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae, Kei Kotake, Naofumi Ohnishi, Shoichi Yamada, Katsuhiko Sato, J. Phys. Conf. Ser. 31 (2006) 95, arXiv:astro-ph/0511826. Third 21COE Symposium : Astrophysics as Interdisciplinary Science, Waseda University, Japan, September 1-3, 2005.
[Kotake:2005ng]
[21-25]
Toward Five-dimensional Core-collapse Supernova Simulations, Christian Y. Cardall et al., J. Phys. Conf. Ser. 16 (2005) 390, arXiv:astro-ph/0510706. SciDAC 2005, Scientific Discovery through Advanced Computing, San Francisco, CA, 26-30 June 2005.
[Cardall:2005id]
[21-26]
The Long Term: Six-dimensional Core-collapse Supernova Models, Christian Y. Cardall, Alexei O. Razoumov, Eirik Endeve, Anthony Mezzacappa, arXiv:astro-ph/0510704, 2005. Open Issues in Understanding Core Collapse Supernovae, National Institute for Nuclear Theory, University of Washington, 22-24 June 2004.
[Cardall:2005ib]
[21-27]
Multigroup Models of the Convective Epoch in Core Collapse Supernovae, F. Douglas Swesty, Eric S. Myra, J. Phys. Conf. Ser. 16 (2005) 380, arXiv:astro-ph/0507294. SciDAC 2005, San Francisco, CA, USA, 26-30 June 2005.
[Swesty:2005jv]
[21-28]
An approach toward the successful supernova explosion by physics of unstable nuclei, K. Sumiyoshi et al., Nucl. Phys. A758 (2005) 63, arXiv:astro-ph/0506619. Nuclei in the Cosmos 8.
[Sumiyoshi:2005rh]
[21-29]
Issues with Core-Collapse Supernova Progenitor Models, Stephen W. Bruenn, arXiv:astro-ph/0506313, 2005. Workshop on Open Issues in Understanding Core Collapse Supernovae, Seattle, Washington, 22-24 June 2004.
[Bruenn:2005hv]
[21-30]
Magnetic Fields in Core Collapse Supernovae: Possibilities and Gaps, J. Craig Wheeler, Shizuka Akiyama, arXiv:astro-ph/0412382, 2004. INT workshop 'Open Issues in Understanding Core Collapse Supernovae,' Seattle, 2004.
[Wheeler:2004ff]
[21-31]
Neutrino-Driven Supernovae: an Accretion Instability in a Nuclear Physics Controlled Environment, Hans-Thomas Janka et al., Nucl. Phys. A758 (2005) 19, arXiv:astro-ph/0411347. 8th Symposium on Nuclei in the Cosmos, Vancouver, BC, Canada, 19-23 Jul 2004.
[Janka:2004an]
[21-32]
Magnetorotational supernova simulations, S.G. Moiseenko, G.S. Bisnovatyi-Kogan, N.V. Ardeljan, ASP Conf.Ser. (2004), arXiv:astro-ph/0410330. International Conference '1604-2004 Supernovae as Cosmological Lighthouses' (Padova, Italy, June 16-19, 2004).
[Moiseenko:2004vg]
[21-33]
The Core Collapse Supernova Mechanism: Current Models, Gaps, and the Road Ahead, Anthony Mezzacappa, ASP Conf.Ser. 342 (2005) 175, arXiv:astro-ph/0410085. Supernovae as Cosmological Lighthouses, Padua, Italy, June 16-19, 2004.
[Mezzacappa:2004ic]
[21-34]
Early Spectra of Supernovae, E. Baron, Peter Nugent, David Branch, Peter H. Hauschildt, ASP Conf.Ser. (2004), arXiv:astro-ph/0409659. 1604-2004 Supernovae As Cosmological Lighthouses, San Francisco.
[Baron:2004nw]
[21-35]
Rotating Core Collapse and Bipolar Supernova Explosions, Adam Burrows, Rolf Walder, Christian D. Ott, Eli Livne, ASP Conf.Ser. (2004), arXiv:astro-ph/0409035. Fate of the Most Massive Stars, Grand Teton National Park, Wyoming, 23-28 May 2004.
[Burrows:2004va]
[21-36]
Understanding Core-Collapse Supernovae, Adam Burrows, arXiv:astro-ph/0405427, 2004. Twelfth Workshop on 'Nuclear Astrophysics,' a Tribute to an Explosive Astrophysicist, Wolfgang Hillebrandt, on the occasion of his 60th Birthday, Ringberg Castle, Lake Tegernsee, Germany, March 22 - 27, 2004.
[Burrows:2004pu]
[21-37]
Core-Collapse Supernovae: Modeling between Pragmatism and Perfectionism, H.-Th. Janka et al., arXiv:astro-ph/0405289, 2004. 12th Workshop on Nuclear Astrophysics, Ringberg Castle, March 22-27, 2004.
[Janka:2004tt]
[21-38]
Fifty-Nine Reasons for a Supernova to not Explode, M. Liebendoerfer, arXiv:astro-ph/0405029, 2004. 12th Workshop on 'Nuclear Astrophysics', Ringberg Castle, March 22-27, 2004.
[Liebendoerfer:2004fk]
[21-39]
An Approach to Neutrino Radiative Transfer in Supernova Simulations, Christian Y. Cardall, arXiv:astro-ph/0404401, 2004. Numerical Methods for Multidimensional Radiative Transfer Problems (RadConf2003), Heidelberg, Germany, 24-26 September 2003.
[Cardall:2004nd]
[21-40]
Synthetic Spectrum Methods for Three-Dimensional Supernova Models, R. C. Thomas, arXiv:astro-ph/0310619, 2003. '3-D Signatures in Stellar Explosions', Austin, Texas.
[Thomas:2003ue]
[21-41]
Effects of Small-Scale Fluctuations of Neutrino Flux in Supernova Explosions, H. Madokoro, T. Shimiz