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Supernova remnants and gamma-ray sources,
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Observations and Theory of Supernovae,
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Supernova mechanisms,
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New physics from Supernova SN1987A,
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The Physics of supernova explosions,
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The Weak Neutral Current and Its Effects in Stellar Collapse,
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Synthesis of the Elements in Stars,
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A Brief History of the Co-evolution of Supernova Theory with Neutrino Physics,
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Introduction to neutrino astronomy,
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4th Azarquiel School of Astronomy, June 2017, Porto Paolo di Capo Passero, Syracuse (Italy).
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Neutrino astrophysics and its connections to nuclear physics,
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Supernovae in SuperK-Gd and other experiments,
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Neutrino Astrophysics,
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52th Winter School of Theoretical Physics, Ladek Zdroj, 14-21 February 2016.
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Nuclear Physics and Astrophysics of Neutrino Oscillations,
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Detection of Supernova Neutrinos,
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Supernova Neutrinos: Theory,
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Neutrino astrophysics : recent advances and open issues,
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Recent advances in neutrino astrophysics,
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Current and Future Liquid Argon Neutrino Experiments,
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Review of Multi-messenger observations of neutron rich matter,
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Core-Collapse Supernovae, Neutrinos, and Gravitational Waves,
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Neutrino flavour conversion and supernovae,
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Neutrinos and the stars,
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ISAPP School 'Neutrino Physics and Astrophysics', 26 July-5 August 2011, Villa Monastero, Varenna, Italy.
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Neutrinos and core-collapse supernovae,
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Physics and Astrophysics Opportunities with Supernova Neutrinos,
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Significance of neutrino cross-sections for astrophysics,
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NUINT2009 (6th International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region), May 18-22, 2009, Sitges, Barcelona, Spain.
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Massive stars as thermonuclear reactors and their explosions following core collapse,
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Kodai School on Synthesis of Elements in Stars.
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Opportunities for Neutrino Physics at the Spallation Neutron Source (SNS),
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2008 Carolina International Symposium on Neutrino Physics.
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Physics of Supernovae: theory, observations, unresolved problems,
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Baikal Young Scientists' International School (BAYSIS), 17-22 September 2007, Irkutsk, Russia.
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NOW2006, Conca Specchiulla, Italy, September 9-16, 2006.
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Supernova neutrino observations: What can we learn?,
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arXiv:astro-ph/0701677.
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Supernova neutrino detection,
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arXiv:astro-ph/0701081.
Neutrino 2006, Santa Fe.
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Nuclear Astrophysics: CIPANP 2006,
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Nucleosynthesis in neutrino heated matter: The vp-process and the r-process,
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NIC-IX, International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, CERN, Geneva, Switzerland, 25-30 June, 2006.
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From progenitor to afterlife,
Roger A. Chevalier,
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2006 STScI May Symposium on Massive Stars.
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Supernova and GRB connection: Observations and Questions,
Massimo Della Valle,
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16th Annual October Astrophysics Conference in Maryland, 'Gamma Ray Bursts in the Swift Era'.
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The Cosmic Stellar Birth and Death Rates,
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Astronomy with Radioactivities V, Clemson Univ., Sept. 2005.
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Supernovae Shedding Light on Gamma-Ray Bursts,
M. Della Valle,
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4th Workshop Gamma-Ray Bursts in the Afterglow Era, Rome,18-22 October 2004.
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High Redshift Supernovae: Cosmological Implications,
Nino Panagia,
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Vulcano Workshop 2004, Frontier Objects in Astrophysics and Particle Physics.
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Supernova neutrino challenges,
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NOW2004, Conca Specchiulla (Otranto, Italy), September 11-17, 2004.
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Supernova Neutrino Oscillations,
Georg G. Raffelt,
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Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.
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Physics of Supernovae,
Dmitrij K. Nadyozhin, V. S. Imshennik,
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arXiv:astro-ph/0501002.
19th European Cosmic Ray Symposium (ECRS 2004), Florence, Italy, 30 Aug - 3 Sep 2004.
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Supernova neutrino detection,
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arXiv:hep-ph/0412029.
Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.
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Supernovae and Their Massive Star Progenitors,
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Science Symposium on the Fate of the Most Massive Stars, Grand Teton National Park, Wyoming, 23-28 May 2004.
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The Supernovae Associated with Gamma-Ray Bursts,
Thomas Matheson,
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Supernovae as Cosmological Lighthouses, Padua, 2004.
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Stellar explosions: from supernovae to gamma-ray bursts,
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ISCRA 14th School Neutrinos and Explosive Events in the Universe, Erice, Italy, July 2004.
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Kepler's Supernova Remnant: The view at 400 Years,
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Spectropolarimetry of Core-Collapse Supernovae,
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Supernovae as Cosmological Lighthouses, 16-19 June, Padua, Italy.
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Supernova neutrinos: production, propagation and oscillations,
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Neutrino 2004, Paris.
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Neutrinos: '...annus mirabilis',
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2nd Int. Workshop on Neutrino oscillations in Venice (NOVE) December 3-5, 2003, Venice, Italy.
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Spectropolarimetric Observations of Supernovae,
Alexei V. Filippenko, Douglas C. Leonard,
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3-D Signatures in Stellar Explosions, 10-13 June, 2003.
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A Review of X-ray Observations of Supernova Remnants,
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Neutrinos as astrophysical probes,
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arXiv:astro-ph/0311256.
ICTP Summer School on Astroparticle Physics and Cosmology, Trieste, Italy, 17 June - 5 Jul 2002.
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Supernova Spectra,
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IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.
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Observations of Type Ia Supernovae, and Challenges for Cosmology,
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IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.
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The Infrared Supernova Rate,
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IAU Colloquium 192: Supernovae (10 Years after SN1993J), Valencia, Spain, 22-26 Apr 2003.
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Neutrino Physics after KamLAND,
Alexei Yu. Smirnov,
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4th Workshop on 'Neutrino Oscillations and their Origin' (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan.
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Cosmology with Supernovae,
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JENAM 2002 (Porto, Portugal).
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Review on the Observed and Physical Properties of Core Collapse Supernovae,
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2003 Aspen Summer Workshop on the Nuclear Physics of Core Collapse Supernovae, Aspen, Colorado, 26 May - 8 June 2003.
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Supernova Neutrinos and Particle-Physics Applications,
G. Raffelt,
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Bolometric Light Curves of Supernovae,
N. B. Suntzeff,
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From Twilight to Highlight - The Physics of Supernovae ESO/MPA/MPE Workshop, Garching, July 29 - 31, 2002.
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Type Ia Supernova models: latest developments,
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JENAM-2002 meeting (Porto, Portugal, September, 3-8).
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Astrophysical and Cosmological Neutrinos,
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International School of Physics 'Enrico Fermi,' CLII Course 'Neutrino Physics,' 23 July-2 August 2002, Varenna, Lake Como, Italy.
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Neutrino masses in astroparticle physics,
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Dennis Sciama Memorial Volume of NAR.
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Second International Workshop on Matter, Anti-Matter and Dark Matter, Trento (Italy), 29-30 October 2001.
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TAUP 2001: Topics in Astroparticle and Underground Physics, Assergi, Italy, 8-12 Sep 2001.
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The Influence of Binaries on Stellar Population Studies, Brussels 21-25 Aug. 2000.
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Unveiling diverse nature of core collapse supernovae,
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Neutrino interactions in neutron matter,
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The Evolution of Low Mass Helium Stars towards Supernova Type I Explosion,
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Supernova neutrino spectra and applications to flavor oscillations,
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Search for low-energy neutrinos from astrophysical sources with Borexino,
M. Agostini et al.
(Borexino),
125
arXiv:1909.02422.
[Borexino:2019wln] - [5-12]
-
An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the First and Second Observing Runs of Advanced LIGO and Advanced Virgo,
B. P. Abbott et al.
(LIGO Scientific, Virgo),
D101
arXiv:1908.03584.
[LIGOScientific:2019ryq] - [5-13]
-
Detection of a Type IIn Supernova in Optical Follow-up Observations of IceCube Neutrino Events,
M. G. Aartsen et al.
(IceCube),
811
arXiv:1506.03115.
[IceCube:2015jsn] - [5-14]
-
Implication on the core collapse supernova rate from 21 years of data of the Large Volume Detector,
N.Y. Agafonova et al.
(LVD),
802
arXiv:1411.1709.
[LVD:2014uzr] - [5-15]
-
Supernova Relic Neutrino Search with Neutron Tagging at Super-Kamiokande-IV,
H. Zhang et al.
(Super-Kamiokande),
60
arXiv:1311.3738.
[Super-Kamiokande:2013ufi] - [5-16]
-
Searching for soft relativistic jets in Core-collapse Supernovae with the IceCube Optical Follow-up Program,
R. Abbasi et al.
(IceCube),
539
arXiv:1111.7030.
[IceCube:2011wip] - [5-17]
-
Supernova Relic Neutrino Search at Super-Kamiokande,
K. Bays et al.
(Super-Kamiokande),
D85
arXiv:1111.5031.
[Super-Kamiokande:2011lwo] - [5-18]
-
IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae,
R. Abbasi et al.
(IceCube),
535
arXiv:1108.0171.
[IceCube:2011cwc] - [5-19]
-
Low Multiplicity Burst Search at the Sudbury Neutrino Observatory,
B. Aharmim et al.
(SNO),
728
arXiv:1011.5436.
[SNO:2010noh] - [5-20]
-
A Search for Core-Collapse Supernovae using the MiniBooNE Neutrino Detector,
A. A. Aguilar-Arevalo et al.
(MiniBooNE),
D81
arXiv:0910.3182.
[MiniBooNE:2009sim] - [5-21]
-
An Extremely Luminous X-ray Outburst Marking the Birth of a Normal Supernova,
A. M. Soderberg et al.,
453
arXiv:0802.1712.
[Soderberg:2008uh] - [5-22]
-
Search for Supernova Neutrino Bursts at Super-Kamiokande,
M. Ikeda, A. Takeda, Y. Fukuda, M. R. Vagins, M. Sakuda
(Super-Kamiokande),
669
arXiv:0706.2283.
[Super-Kamiokande:2007zsl] - [5-23]
-
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),
653
arXiv:hep-ex/0607010.
[SNO:2006dke] - [5-24]
-
Gamma-Ray Burst associated Supernovae: Outliers become Mainstream,
E. Pian et al.,
442
arXiv:astro-ph/0603530.
[Pian:2006pr] - [5-25]
-
Discovery of 35 New Supernova Remnants in the Inner Galaxy,
C. L. Brogan et al.,
639
arXiv:astro-ph/0601451.
[Brogan:2006tv] - [5-26]
-
Echoes from Ancient Supernovae in the Large Magellanic Cloud,
A. Rest et al.,
arXiv:astro-ph/0510738.
[Rest:2005un] - [5-27]
-
Discovery of X-Ray Emission from Supernova 1970G with Chandra: Filling the Void between Supernovae and Supernova Remnants,
Stefan Immler, K. D. Kuntz,
632
arXiv:astro-ph/0506023.
[Immler:2005ym] - [5-28]
-
Late-time X-Ray, UV and Optical Monitoring of Supernova 1979C,
Stefan Immler et al.,
632
arXiv:astro-ph/0503678.
[Immler:2005vx] - [5-29]
-
Hubble Space Telescope imaging of the progenitor sites of six nearby core-collapse supernovae,
Justyn R. Maund, Stephen J. Smartt,
360
arXiv:astro-ph/0501323.
[Maund:2005nq] - [5-30]
-
SN Ib 1990I: Clumping and Dust in the Ejecta?,
Abouazza Elmhamdi et al.,
426
arXiv:astro-ph/0407145.
[Elmhamdi:2004he] - [5-31]
-
SNEWS: The SuperNova Early Warning System,
P. Antonioli et al.,
6
arXiv:astro-ph/0406214.
[Antonioli:2004zb] - [5-32]
-
The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope,
Nikolai N. Chugai et al.,
352
arXiv:astro-ph/0405369.
[Chugai:2004gq] - [5-33]
-
XMM-Newton observation of Kepler's supernova remnant,
G. Cassam-Chenai et al.,
arXiv:astro-ph/0310687.
[Cassam-Chenai:2003lgh] - [5-34]
-
Twenty Years of Galactic Observations in Searching for Bursts of Collapse Neutrinos with the Baksan Underground Scintillation Telescope,
E.N.Alexeyev, L.N.Alexeyeva,
95
arXiv:astro-ph/0212499.
[Alekseev:2002ji] - [5-35]
-
Search for supernova relic neutrinos at Super-Kamiokande,
M. Malek et al.
(Super-Kamiokande),
90
arXiv:hep-ex/0209028.
[Super-Kamiokande:2002hei] - [5-36]
-
The Asiago Supernova Catalogue - 10 years after,
R. Barbon, V. Buondi, E. Cappellaro, M. Turatto,
139
[Asiago-Supernova-Catalogue-AA139-1999]
- [6-1]
-
Eleven Year Search for Supernovae with the IceCube Neutrino Observatory,
Robert Cross, Alexander Fritz, Spencer Griswold
(IceCube),
ICRC2019
arXiv:1908.07249.
36th International Cosmic Ray Conference (ICRC 2019), Madison, WI, U.S.A.
[Cross:2019jpb] - [6-2]
-
Improved Detection of Supernovae with the IceCube Observatory,
Lutz Kopke
(IceCube),
1029
arXiv:1704.03823.
8th international symposium on large TPCs for low-energy rare event detection, Paris, Dec. 5-7, 2016.
[Kopke:2017req] - [6-3]
-
The core collapse supernova rate from 24 years of data of the Large Volume Detector,
G. Bruno, A. Molinario, W. Fulgione, C. Vigorito
(LVD),
888
arXiv:1701.06765.
XXV ECRS 2016.
[Bruno:2017oxg] - [6-4]
-
The IceCube Neutrino Observatory Part V: Neutrino Oscillations and Supernova Searches,
M. G. Aartsen et al.
(IceCube),
arXiv:1309.7008,
33nd International Cosmic Ray Conference, Rio de Janeiro 2013.
[IceCube:2013lje] - [6-5]
-
Supernova Detection in IceCube: Status and Future,
Ronald Bruijn
(IceCube),
2013
arXiv:1302.2040.
NOW 2012.
[Bruijn:2013ibl] - [6-6]
-
The IceCube Neutrino Observatory VI: Neutrino Oscillations, Supernova Searches, Ice Properties,
R. Abbasi et al.
(IceCube),
arXiv:1111.2731,
32nd International Cosmic Ray Conference, Beijing 2011.
[IceCube:2011vzz] - [6-7]
-
Low Energy Neutrino Astronomy in Super-Kamiokande,
Michael Smy,
arXiv:1110.0012,
DPF 2011.
[Smy:2011tm] - [6-8]
-
Search for neutrino bursts from core collapse supernovae at the Baksan Underground Scintillation Telescope,
R.V. Novoseltseva et al.,
arXiv:0910.0738,
31 International Cosmic Ray Conference, Lodz, Poland, July 7-15, 2009.
[Novoseltseva:2009cr] - [6-9]
-
Supernova Search with the AMANDA / IceCube Detectors,
Thomas Kowarik, Timo Griesel, Alexander Piegsa
(Icecube),
arXiv:0908.0441,
31st ICRC, Lodz, Poland, July 2009.
[Kowarik:2009qr] - [6-10]
-
Search for High Energetic Neutrinos from Supernova Explosions with AMANDA,
Dirk Lennarz, Jan-Patrick Huls, Christopher Wiebusch
(IceCube),
arXiv:0907.4621,
31st ICRC, Lodz, Poland, July 2009.
[Lennarz:2009xr] - [6-11]
-
Recent Type II Radio Supernovae,
Christopher J. Stockdale et al.,
937
arXiv:0708.1182.
Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.
[Stockdale:2007pe] - [6-12]
-
LVD highlights,
Marco Selvi et al.
(LVD),
arXiv:hep-ex/0608061,
Vulcano Workshop 2006 'Frontier Objects in Astrophysics and Particle Physics'.
[Selvi:2006bi] - [6-13]
-
SNLS - the Supernova Legacy Survey,
C.J. Pritchet, SNLS
(SNLS),
arXiv:astro-ph/0406242.
Observing Dark Energy (NOAO/Tucson proceedings).
[Pritchet:2004af] - [6-14]
-
Evidence for Core Collapse in the Type Ib/c SN 1999ex,
Mario Hamuy et al.,
arXiv:astro-ph/0212368,
From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.
[Hamuy:2002rz] - [6-15]
-
The dusty type IIn Supernova 1998S,
Peter Meikle et al.,
arXiv:astro-ph/0211144,
ESO/MPA/MPE Workshop 'From Twilight to Highlight: The Physics of Supernovae', Garching, Germany, 29-31 July 2002.
[Meikle:2002dn] - [6-16]
-
A Search for Core-Collapse Supernova Progenitors In Hubble Space Telescope Images,
Schuyler D. Van Dyk, Weidong Li, Alexei V. Filippenko,
arXiv:astro-ph/0210347.
PASP (2003 Jan).
[VanDyk:2002ry] - [6-17]
-
An Intermediate Redshift Supernova Search at ESO: Reduction Tools and Efficiency Tests,
M. Riello et al.,
arXiv:astro-ph/0210265,
ESO/MPA/MPE Workshop 'From Twilight to Highlight, The Physics of Supernovae', Garching, Jul 29-31, 2002.
[Riello:2002hm] - [6-18]
-
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,
'White Dwarfs', Proc. XIII Workshop on White Dwarfs.
[Napiwotzki:2002sa]
- [7-1]
-
Are classification metrics good proxies for SN Ia cosmological constraining power?,
Alex I. Malz et al.
(LSST Dark Energy Science),
arXiv:2305.14421,
[LSSTDarkEnergyScience:2023bbq] - [7-2]
-
Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey,
A. Rest et al.,
795
arXiv:1310.3828.
[Rest:2013mwz] - [7-3]
-
Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample,
D. Scolnic et al.,
795
arXiv:1310.3824.
[Scolnic:2013efb] - [7-4]
-
The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae,
Gaston Folatelli et al.,
139
arXiv:0910.3317.
[Folatelli:2009nm] - [7-5]
-
Asymmetric Explosion of Type Ia Supernovae as Seen from Near Infrared Observations,
K. Motohara et al.,
652
arXiv:astro-ph/0610303.
[Motohara:2006tg] - [7-6]
-
The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey,
A. Conley et al.
(SNLS),
132
arXiv:astro-ph/0607363.
[SNLS:2006vah] - [7-7]
-
Nonlinear Decline-Rate Dependence and Intrinsic Variation of Type Ia Supernova Luminosities,
Lifan Wang et al.,
641
arXiv:astro-ph/0512370.
[Wang:2005bw] - [7-8]
-
The Supernova Legacy Survey: Measurement of $\Omega_\text{M}$, $\Omega_{\Lambda}$ and $w$ from the First Year Data Set,
P. Astier et al.
(SNLS),
447
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.
[SNLS:2005qlf] - [7-9]
-
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),
642
arXiv:astro-ph/0510155.
[HighZSNSearch:2005xhg] - [7-10]
-
Spectroscopy of twelve Type Ia supernovae at intermediate redshift,
C. Balland et al.,
arXiv:astro-ph/0507703.
[Balland:2005rw] - [7-11]
-
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.,
633
arXiv:astro-ph/0507183.
[Willott:2005zr] - [7-12]
-
Evidence for Spectropolarimetric Diversity in Type Ia Supernovae,
Douglas C. Leonard et al.,
632
arXiv:astro-ph/0506470.
[Leonard:2005td] - [7-13]
-
A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex,
R. J. Foley et al.,
626
arXiv:astro-ph/0504481.
[Foley:2005qu] - [7-14]
-
Restframe I-band Hubble diagram for type Ia supernovae up to redshift $z \sim 0.5$,
Serena Nobili et al.
(Supernova Cosmology Project),
arXiv:astro-ph/0504139.
[SupernovaCosmologyProject:2005zcy] - [7-15]
-
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.,
627
arXiv:astro-ph/0503159.
From the abstract: $H_0 = 73 +\pm 4 \pm 5 \, \text{km} \, \text{s}^{-1} \, \text{Mps}^{-1}$.
[Riess:2005zi] - [7-16]
-
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey,
Louis-Gregory Strolger, Adam G. Riess,
131
arXiv:astro-ph/0503093.
[Strolger:2005uk] - [7-17]
-
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT,
C. Lidman et al.
(Supernova Cosmology Project),
arXiv:astro-ph/0410506.
[SupernovaCosmologyProject:2004akn] - [7-18]
-
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models,
L. G. Strolger et al.,
613
arXiv:astro-ph/0406546.
[Strolger:2004kk] - [7-19]
-
Type Ia supernova rate at a redshift of ~ 0.1,
Guillaume Blanc et al.
(EROS),
423
arXiv:astro-ph/0405211.
[EROS:2004reu] - [7-20]
-
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa,
Gabriele Garavini et al.
(The Supernova Cosmology Project),
356
arXiv:astro-ph/0404393.
[SupernovaCosmologyProject:2004yms] - [7-21]
-
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),
607
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] - [7-22]
-
23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at $z > 0.7$,
Brian J. Barris et al.,
602
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] - [7-23]
-
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),
598
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 $P(\Omega_{\Lambda}>0)>0.99$.
[SupernovaCosmologyProject:2003dcn] - [7-24]
-
Cosmological Results from High-z Supernovae,
John L. Tonry et al.
(Supernova Search Team),
594
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
[SupernovaSearchTeam:2003cyd] - [7-25]
-
SN 2002cx: The Most Peculiar Known Type Ia Supernova,
Weidong Li et al.,
115
arXiv:astro-ph/0301428.
[Li:2003wja] - [7-26]
-
Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el,
Kevin Krisciunas et al.,
125
arXiv:astro-ph/0210327.
[Krisciunas:2002rc] - [7-27]
-
The Type la Supernova 2001V in NGC 3987,
J. Vinko et al.,
397
arXiv:astro-ph/0210186.
[Vinko:2002pa] - [7-28]
-
The distant Type Ia supernova rate,
R. Pain et al.
(Supernova Cosmology Project),
577
arXiv:astro-ph/0205476.
[SupernovaCosmologyProject:2002nuh] - [7-29]
-
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),
560
arXiv:astro-ph/0104455.
[SupernovaSearchTeam:2001qse] - [7-30]
-
Measurements of Omega and Lambda from 42 High-Redshift Supernovae,
S. Perlmutter et al.
(Supernova Cosmology Project),
517
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.
[SupernovaCosmologyProject:1998vns] - [7-31]
-
Supernova Limits on the Cosmic Equation of State,
Peter M. Garnavich et al.
(Supernova Search Team),
509
arXiv:astro-ph/9806396.
[SupernovaSearchTeam:1998cav] - [7-32]
-
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,
Adam G. Riess et al.
(Supernova Search Team),
116
arXiv:astro-ph/9805201.
[SupernovaSearchTeam:1998fmf]
- [8-1]
-
Exploring the Physics of Type Ia Supernovae Through the X-ray Spectra of their Remnants,
C. Badenes et al.,
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),
C041213
arXiv:astro-ph/0504455.
22nd Texas Symposium on Relativistic Astrophysics.
[SDSS:2004bao]
- [9-1]
-
Additional evidence for a pulsar wind nebula in the heart of SN 1987A from multi-epoch X-ray data and MHD modeling,
Emanuele Greco et al.,
931
arXiv:2204.06804.
[Greco:2022cto] - [9-2]
-
A 'Missing' Supernova Remnant revealed by the 21-cm Line of Atomic Hydrogen,
B-C Koo, J-h Kang, C.J. Salter,
643
arXiv:astro-ph/0604186.
[Koo:2006sr]
- [10-1]
-
JWST NIRSpec observations of Supernova 1987A - from the inner ejecta to the reverse shock,
J. Larsson et al.,
949
arXiv:2302.03576.
[Larsson:2023lml] - [10-2]
-
Polarized radio emission unveils the structure of the pre-supernova circumstellar magnetic field and the radio emission in SN1987A,
O. Petruk, V. Beshley, S. Orlando, F. Bocchino, M. Miceli, S. Nagataki, M. Ono, S. Loru, A. Pellizzoni, E. Egron,
518
arXiv:2212.00656.
[Petruk:2022urq] - [10-3]
-
A 3D view of molecular hydrogen in Supernova 1987A,
J.Larsson, J. Spyromilio, C. Fransson, R. Indebetouw, M. Matsuura, F. J. Abellan, P. Cigan, H. Gomez, B. Leibundgut,
873
arXiv:1901.11235.
[Larsson:2019uwm] - [10-4]
-
Time evolution of the line emission from the inner circumstellar ring of SN 1987A and its hot spots,
Per Groeningsson et al.,
492
arXiv:0810.2661.
[Groeningsson:2008nc] - [10-5]
-
Chandra HETG Spectra of SN 1987A at 20 years,
D. Dewey, S. A. Zhekov, R. McCray, C. R. Canizares,
676
arXiv:0802.2340.
[Dewey:2008gy] - [10-6]
-
Infrared Integral Field Spectroscopy of SN 1987A,
Karina Kjaer et al.,
937
arXiv:astro-ph/0703720.
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Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background,
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Effects of the Metallicity on Li and B Production in Supernova Neutrino Process,
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Diagnosing the Structure of Massive Stars with Galactic Supernova Neutrinos,
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Supernova Physics at DUNE,
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34th International Cosmic Ray Conference (ICRC).
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Type IIn supernovae as sources of high energy neutrinos,
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Principal Physical Effects in Collapsing Stellar Cores,
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A Critical Appraisal of Some Concepts Used in Neutrino Physics,
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Can a supernova bang twice?,
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arXiv:1009.6096.
Yukawa International Program for Quark-Hadron Sciences: New Frontiers in QCD 2010, Kyoto, Japan.
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The r-Process in Black Hole Winds,
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1269
arXiv:1006.2277.
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Using supernova neutrinos to monitor the collapse, to search for gravity waves and to probe neutrino masses,
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Galileo-Xu Guangqi meeting: The Sun, the Stars, the Universe and General Relativity; October 26-30, 2009, Shanghai (China).
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Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star,
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The Strange Prospects for Astrophysics,
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Neutrino 2008, Christchurch, NZ.
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Supernova neutrinos: Strong coupling effects of weak interactions,
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Formation of quark phases in compact stars and SN explosion,
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Nucleosynthesis in Early Neutrino Driven Winds,
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Spectral Modeling of Type II Supernovae,
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The Supernova Gamma-Ray Burst Connection,
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The Relic Neutrino Backround from the First Stars,
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Astronomy with Radioactivities V, Clemson University, September 5-9, 2005.
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IFAE, Catania 2005.
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Nucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of Extremely Metal Poor Stars,
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6IAU Symp. No. 228 'From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution'.
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SN/GRB connection: a statistical approach with BATSE and Asiago Catalogues,
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Supernova Rates in Galaxy Clusters,
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Searching for Progenitors of Core-Collapse Supernovae,
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Nuclear physics and astrophysics of the r-process,
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International Nuclear Physics Conference (INPC2004).
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IMF variations and their implications for Supernovae numbers,
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BDMH2004
arXiv:astro-ph/0412114.
'Baryons in Dark Matter Halos', Novigrad, Croatia, October 5-9, 2004.
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Supernova Neutrinos and the absolute scale of neutrino masses - a Bayesian approach,
Enrico Nardi,
arXiv:hep-ph/0412024,
Fifth Latin American Simposium on High Energy Physics (V-SILAFAE) Lima, Peru, July 12-17, 2004.
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Supernova Neutrino Process and its Impact on the Galactic Chemical Evolution of the Light Elements,
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Nuclei in the Cosmos VIII.
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The r-process nucleosynthesis: a continued challenge for nuclear physics and astrophysics,
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Sterile Neutrinos in astrophysical and cosmological sauce,
Marco Cirelli,
arXiv:astro-ph/0410122,
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.
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Parity Violation in Astrophysics,
C. J. Horowitz,
A24S2
arXiv:nucl-th/0410074.
PAVI04 conference in Grenoble, France.
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Powerful gravitational-wave bursts from supernova neutrino oscillations,
Herman J. Mosquera Cuesta, Karen Fiuza,
739
arXiv:astro-ph/0407526.
'Hadron Physics - RANP 2004', Angra dos Reis - Rio de Janeiro - Brazil, March 28 to April 03.
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Neutrino Oscillations at Supernova Core Bounce Generate the Strongest Gravitational-Wave Bursts,
Herman J. Mosquera Cuesta, Karen Fiuza,
D13
arXiv:astro-ph/0407184.
International Workshop on Astronomy and Relativistic Astrophysics, Olinda (Brazil), October 12-16 (2003).
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Core-Collapse Supernovae Induced by Anisotropic Neutrino Radiation,
Yuko Motizuki, Hideki Madokoro, Tetsuya Shimizu,
11
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.
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Supernova Neutrino-Nucleus Physics and the r-process,
W. C. Haxton,
arXiv:nucl-th/0406012,
'The r-process: The Astrophysical Origin of the Heavy Elements...'.
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Global Anisotropies in Supernova Explosions and Pulsar Recoil,
L. Scheck et al.,
arXiv:astro-ph/0405311,
12th Workshop on Nuclear Astrophysics, Ringberg Castle, March 22-27, 2004.
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-
Decays of supernova relic neutrinos,
G.L. Fogli, E. Lisi, A. Mirizzi, D. Montanino,
arXiv:hep-ph/0405136,
39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Italy, 21-28 Mar 2004.
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-
Sterile neutrinos: from cosmology to experiments,
Guido Marandella,
arXiv:hep-ph/0405090,
39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 21-28 March 2004.
[Marandella:2004xv] - [17-72]
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Neutrinos from pre-supernova star,
A. Odrzywolek, M. Misiaszek, M. Kutschera,
B35
arXiv:astro-ph/0405006.
Epiphany Conference on Astroparticle Physics, 8-11 January 2004, Cracow, Poland.
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An Approach to Neutrino Radiative Transfer in Supernova Simulations,
Christian Y. Cardall,
arXiv:astro-ph/0404401,
Numerical Methods for Multidimensional Radiative Transfer Problems (RadConf2003), Heidelberg, Germany, 24-26 September 2003.
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The Evolution of Supernovae in the Winds of Massive Stars,
Vikram Dwarkadas,
arXiv:astro-ph/0403195,
Cosmic Explosions in Three Dimensions: Asymmetries in Supernovae and Gamma-Ray Bursts.
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Detection of Supernova Neutrinos,
B. Bekman, J. Holeczek, J. Kisiel,
B35
arXiv:hep-ph/0403117.
XXVIII Mazurian Lakes School of Physics, Krzyze, Poland, August 31 - September 7, 2003.
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Neutrino Processes in Supernovae and Neutrons Stars in Their Infancy and Old Age,
M. Prakash, S. Ratkovic, S. I. Dutta,
arXiv:astro-ph/0403038,
KIAS-APCTP International Symposium in Astro-Hadron Physics, November 10-14, 2003.
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Measuring neutrino masses with supernova neutrinos,
Enrico Nardi,
arXiv:astro-ph/0401624,
X Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July 2003.
[Nardi:2004ms] - [17-78]
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Neutron Star Kicks and Supernova Asymmetry,
Dong Lai,
arXiv:astro-ph/0312542,
3D Signatures of Stellar Explosion, a workshop honoring J.C. Wheeler's 60th Birthday.
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Low frequency radio and X-ray properties of core-collapse supernovae,
A. Ray, P. Chandra, F. Sutaria, S. Bhatnagar,
99
arXiv:astro-ph/0311419.
IAU Colloquium 192 'Supernovae (10 years of SN 1993J)', April 2003, Valencia, Spain.
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Pulsar velocities and dark matter hint at a singlet neutrino,
Alexander Kusenko,
arXiv:astro-ph/0311240,
Sixth RESCEU International Symposium 'Frontier in Astroparticle Physics and Cosmology', Tokyo, Japan, November 4 - 7, 2003.
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Expected Changes of Supernovae with Redshift due to Evolution of their Progenitors,
I. Dominguez et al.,
99
arXiv:astro-ph/0311140.
IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003.
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44Ti radioactivity in young supernova remnants: Cas A and SN 1987A,
Y. Motizuki, S. Kumagai,
48
arXiv:astro-ph/0311080.
'Astronomy with Radioactivities IV', Seeon, Germany, June 2003.
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Supernova Statistics,
E. Cappellaro, R. Barbon, M. Turatto,
99
arXiv:astro-ph/0310859.
IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003.
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Type Ia Supernovae: Spectroscopic Surprises,
D. Branch,
arXiv:astro-ph/0310685,
3-D Signatures of Stellar Explosions: A Workshop Honoring J. Craig Wheeler's 60th Birthday.
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Effects of Small-Scale Fluctuations of Neutrino Flux in Supernova Explosions,
H. Madokoro, T. Shimizu, Y. Motizuki,
99
arXiv:astro-ph/0310481.
IAU Colloquium 192, SUPERNOVAE (10 years of SN1993J), Valencia, Spain.
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Understanding Type II Supernovae,
L. Zampieri, M. Ramina, A. Pastorello,
99
arXiv:astro-ph/0310057.
IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003.
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Observational Properties of Type II Plateau Supernovae,
A. Pastorello et al.,
99
arXiv:astro-ph/0310056.
IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003.
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Cosmic rays, stellar evolution, and supernova physics,
P. L. Biermann,
48
arXiv:astro-ph/0309810.
'Astronomy With Radioactivities IV - Filling the Sensitivty Gap in MEV Astronomy', Seeon Conference, Bavaria, Germany, May 2003.
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A Geometric Determination of the Distance to SN 1987A and the LMC,
N. Panagia,
99
arXiv:astro-ph/0309416.
IAU Colloquium 192 'Supernovae (10 years of SN1993J)', Valencia, Spain.
[Panagia:2003rt] - [17-90]
-
$^{56}\mathrm{Ni}$ mass in type IIP SNe: Light curves and H-alpha luminosities diagnostics,
Abouazza Elmhamdi, N. N. Chugai, I. J. Danziger,
99
arXiv:astro-ph/0309286.
IAU Colloquium 192: Supernovae (10 Years after SN1993J), Valencia, Spain, 22-26 Apr 2003.
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-
Neutrinos and (anti)neutrinos from supernovae and from the earth in the Borexino detector,
L. Miramonti,
arXiv:hep-ex/0307029,
1st Yamada Symposium on Neutrinos and Dark Matter in Nuclear Physics June 9-14, 2003, Nara, Japan.
[Miramonti:2003hw] - [17-92]
-
Neutrinos in Extra Dimensions and Supernovae,
M. Cirelli,
arXiv:hep-ph/0305141,
38th Rencontres de Moriond - Electroweak Interactions and Unified Theories, March 15-22, 2003, Les Arcs, France.
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-
Supernova neutrinos: Flavor-dependent fluxes and spectra,
G.G.Raffelt et al.,
arXiv:astro-ph/0303226,
NOON 03, Kanazawa, 10-14 Feb 2003.
[Raffelt:2003en] - [17-94]
-
Neutrinos and Nucleosynthesis in Supernova,
U. Solis, J. C. D'Olivo, L. G. Cabral-Rosetti,
37
arXiv:hep-ph/0302015.
Mexican School of Astrophysics (EMA), Guanajuato, Mexico, July 31 - August 7, 2002.
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Supernova Explosions from Accretion Disk Winds,
Andrew I. MacFadyen,
arXiv:astro-ph/0301425,
'From Twilight to Highlight - The Physics of Supernovae' ESO/MPA/MPE Workshop, Garching July 2002.
[MacFadyen:2003wg] - [17-96]
-
Presupernova Evolution of Rotating Massive Stars and the Rotation Rate of Pulsars,
A. Heger, S. E. Woosley, N. Langer, H. C. Spruit,
215
arXiv:astro-ph/0301374.
IAU 215 'Stellar Rotation'.
[Heger:2003nh] - [17-97]
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Supernovae, Gamma-Ray Bursts, and Stellar Rotation,
S. E. Woosley, A. Heger,
arXiv:astro-ph/0301373.
IAU 215 'Stellar Rotation'.
[Woosley:2003ng] - [17-98]
-
Circumstellar Interaction Around Supernovae,
Roger A. Chevalier,
arXiv:astro-ph/0301368,
'From Twilight to Highlight - The Physics of Supernovae' ESO/MPA/MPE Workshop, Garching July 2002.
[Chevalier:2003nb] - [17-99]
-
Supernova Neutrinos : oscillations and new interactions,
D. Montanino,
Seminar at Padua University, November 18, 2003, Padua, Italy.
http://www.pd.infn.it/~laveder/unbound/seminari/sn/SuperNovae.ppt.
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Observable Effects of Shocks in Compact and Extended Presupernovae,
S. Blinnikov et al.,
arXiv:astro-ph/0212569,
ESO/MPA/MPE Workshop 'From Twilight to Highlight: The Physics of Supernovae', Garching, July 2002.
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Light Curves of Type Ia Supernovae as a Probe for an Explosion Model,
Elena Sorokina, Sergey Blinnikov,
arXiv:astro-ph/0212527,
From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia.
[Sorokina:2002gr] - [17-102]
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The Mechanism of Core-Collapse Supernovae and the Ejection of Heavy Elements,
H.-Th. Janka, R. Buras, M. Rampp,
A718
arXiv:astro-ph/0212317.
NIC7, Fuji-Yoshida, Japan, July 8-12, 2002.
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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,
33
arXiv:astro-ph/0212188.
34th COSPAR Sci. Assembly, Houston, 10-19 october 2002.
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-
Energy exchange inside SN ejecta and light curves of SNe Ia,
E.I.Sorokina, S.I.Blinnikov,
arXiv:astro-ph/0212187,
11th Workshop on 'Nuclear Astrophysics', Ringberg Castle, Tegernsee, Germany, February 11-16, 2002.
[Sorokina:2002yb] - [17-105]
-
Magnetic Field in Supernovae,
Shizuka Akiyama, J. Craig Wheeler,
arXiv:astro-ph/0211458,
conference 'Core Collapse of Massive Stars'.
[Akiyama:2002ur] - [17-106]
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The Neutrino Signal in Stellar Core Collapse and Postbounce Evolution,
M. Liebendoerfer et al.,
A719
arXiv:astro-ph/0211329.
Nuclear Physics in Astrophysics Conference, Debrecen, Hungary, 2002.
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Variety in Supernovae,
Massimo Turatto, Stefano Benetti, Enrico Cappellaro,
arXiv:astro-ph/0211219,
ESO / MPA / MPE Workshop: From Twilight to Highlight: The Physics of Supernovae, Garching, Germany, 29-31 June 2002.
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Synchronised neutrino oscillations from self interaction and associated applications,
Yvonne Y. Y. W.,
655
arXiv:hep-ph/0211045.
3rd Topical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology, San Juan, Puerto Rico, 19-24 Aug 2002.
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Nucleosynthesis as a result of multiple delayed detonations in Type Ia Supernovae,
Domingo Garcia-Senz, Eduardo Bravo,
A718
arXiv:astro-ph/0210339.
'Nuclei in the Cosmos VII' 2002.
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-
Neutrino-nucleon scattering rate in the relativistic random phase approximation,
L. Mornas,
A721
arXiv:nucl-th/0210035.
PANIC02 conference, 30 sept - 4 oct 2002, Osaka, Japan.
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-
Supernovae and Neutrinos,
John F. Beacom,
118
arXiv:astro-ph/0209136.
XXth International Conference on Neutrino Physics and Astrophysics (Neutrino 2002), Munich, Germany, May 25-30, 2002.
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-
Neutron Stars, Pulsars and Supernova Remnants: concluding remarks,
F. Pacini,
arXiv:astro-ph/0208563,
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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-
Supernova neutrinos, LSND and MiniBooNE,
Michel Sorel,
arXiv:hep-ph/0205207,
37th Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, France, 9-16 Mar 2002.
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Core-collapse supernova simulations: Variations of the input physics,
M. Rampp, R. Buras, H.-Th. Janka, G. Raffelt,
arXiv:astro-ph/0203493,
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,
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,
54
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,
45
arXiv:hep-ph/9901300.
22nd Symposium on Nuclear Physics, Oaxtepec, Morelos, Mexico, 5-8 Jan 1999.
[Beacom:1999bn] - [17-118]
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Supernova Remnants - Part One - Historical Events,
R. G. Strom,
NATO Advanced Study Institute on Neutron Stars: Their Birth, Evolution, Radiation and Winds, Erice, Sicily, Italy, September 5-17, 1988, p. 253.
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Supernova statistics and related problems,
G. A. Tammann,
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Probing the Sterile Neutrino Dipole Portal with SN1987A and Low-Energy Supernovae,
Garv Chauhan, Shunsaku Horiuchi, Patrick Huber, Ian M. Shoemaker,
arXiv:2402.01624,
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SN1987A constraints to BSM models with extra neutral bosons near the trapping regime: $U(1)_{L_\mu-L_\tau}$ model as an illustrative example,
Kwang-Chang Lai, Chun Sing Jason Leung, Guey-Lin Lin,
arXiv:2401.16023,
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Axion emission from strange matter in core-collapse SNe,
Mael Cavan-Piton, Diego Guadagnoli, Micaela Oertel, Hyeonseok Seong, Ludovico Vittorio,
arXiv:2401.10979,
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Limits on heavy neutral leptons, $Z'$ bosons and majorons from high-energy supernova neutrinos,
Kensuke Akita, Sang Hui Im, Mehedi Masud, Seokhoon Yun,
arXiv:2312.13627,
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Comprehensive constraints on heavy sterile neutrinos from core-collapse supernovae,
Pierluca Carenza, Giuseppe Lucente, Leonardo Mastrototaro, Alessandro Mirizzi, Pasquale Dario Serpico,
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arXiv:2311.00033.
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Supernova Simulations Confront SN 1987A Neutrinos,
Damiano F. G. Fiorillo, Malte Heinlein, Hans-Thomas Janka, Georg Raffelt, Edoardo Vitagliano,
108
arXiv:2308.01403.
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Old Data, New Forensics: The First Second of SN 1987A Neutrino Emission,
Shirley Weishi Li, John F. Beacom, Luke F. Roberts, Francesco Capozzi,
arXiv:2306.08024,
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SN1987A cooling due to Plasmon-Plasmon scattering in the Randall-Sundrum Model,
Manish Kumar Sharma, Saumyen Kundu, Prasanta Kumar Das,
40
arXiv:2304.00380.
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The Neutrino Magnetic Moment Portal and Supernovae: New Constraints and Multimessenger Opportunities,
Vedran Brdar, Andre de Gouvea, Ying-Ying Li, Pedro A. N. Machado,
107
arXiv:2302.10965.
[Brdar:2023tmi] - [18-10]
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SN1987A neutrino burst: limits on flavor conversion,
Pedro Dedin Neto, Marcos V. dos Santos, Pedro Cunha de Holanda, Ernesto Kemp,
83
arXiv:2301.11407.
[DedinNeto:2023hhp] - [18-11]
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Strong Supernova 1987A Constraints on Bosons Decaying to Neutrinos,
Damiano F. G. Fiorillo, Georg G. Raffelt, Edoardo Vitagliano,
131
arXiv:2209.11773.
[Fiorillo:2022cdq] - [18-12]
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Gravitational Lensing of Supernova Neutrino Bursts,
John M. LoSecco,
7
arXiv:2109.01957.
[LoSecco:2021sdt] - [18-13]
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Understanding and visualizing the statistical analysis of SN1987A neutrino data,
Marcos V. dos Santos, Pedro Cunha de Holanda,
82
arXiv:2108.06448.
[dosSantos:2021egl] - [18-14]
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Relationships among detector signals recorded during events SN1987A and GW170817,
N. Agafonova, A. Malgin, E. Fischbach,
arXiv:2107.00265,
[Agafonova:2021tgr] - [18-15]
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SN1987A still shining: A Quest for Pseudo-Dirac Neutrinos,
Ivan Martinez-Soler, Yuber F. Perez-Gonzalez, Manibrata Sen,
105
arXiv:2105.12736.
[Martinez-Soler:2021unz] - [18-16]
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Supernova 1987A: 3D Mixing and light curves for explosion models based on binary-merger progenitors,
V. P. Utrobin, A. Wongwathanarat, H.-Th. Janka, E. Mueller, T. Ertl, A. Menon, A. Heger,
914
arXiv:2102.09686.
[Utrobin:2021nhm] - [18-17]
-
Indication of a Pulsar Wind Nebula in the hard X-ray emission from SN 1987A,
Emanuele Greco, Marco Miceli, Salvatore Orlando, Barbara Olmi, Fabrizio Bocchino, Shigehiro Nagataki, Masaomi Ono, Akira Dohi, Giovanni Peres,
908
arXiv:2101.09029.
[Greco:2021sfi] - [18-18]
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Discovery of an 8 MeV line in the SN 1987A neutrino spectrum,
R. Ehrlich,
2021
arXiv:2101.08128.
[Ehrlich:2021era] - [18-19]
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Supernova Constraints on Dark Flavored Sectors,
Jorge Martin Camalich, Jorge Terol-Calvo, Laura Tolos, Robert Ziegler,
D103
arXiv:2012.11632.
[Camalich:2020wac] - [18-20]
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Supernova Muons: New Constraints on Z' Bosons, Axions, and ALPs,
Djuna Croon, Gilly Elor, Rebecca K. Leane, Samuel D. McDermott,
2101
arXiv:2006.13942.
[Croon:2020lrf] - [18-21]
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NS 1987A in SN 1987A,
Dany Page, Mikhail V. Beznogov, Ivan Garibay, James M. Lattimer, Madappa Prakash, Hans-Thomas Janka,
898
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[Page:2020gsx] - [18-22]
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Properties of gamma-ray decay lines in 3D core-collapse supernova models, with application to SN 1987A and Cas A,
A. Jerkstrand et al.,
494
arXiv:2003.05156.
[Jerkstrand:2020hlf] - [18-23]
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Is there a supernova bound on axions?,
Nitsan Bar, Kfir Blum, Guido D'Amico,
D101
arXiv:1907.05020.
[Bar:2019ifz] - [18-24]
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Possible Explanation of the Geograv Detector Signal during the Explosion of SN 1987A in Modified Gravity Models,
Yu. N. Eroshenko, E. O. Babichev, V. I. Dokuchaev, A. S. Malgin,
128
arXiv:1906.06088.
[Eroshenko:2019qiv] - [18-25]
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Three-dimensional mixing and light curves: constraints on the progenitor of supernova 1987A,
Victor Utrobin, Annop Wongwathanarat, H.-Thomas Janka, Ewald Mueller, T. Ertl, Stan Woosley,
624
arXiv:1812.11083.
[Utrobin:2018mjr] - [18-26]
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Revisiting Supernova 1987A Limits on Axion-Like-Particles,
Jun Seok Lee,
arXiv:1808.10136,
[Lee:2018lcj] - [18-27]
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The 30-Year Search for the Compact Object in SN 1987A,
Dennis Alp et al.,
864
arXiv:1805.04526.
[Alp:2018oek] - [18-28]
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Can a bright and energetic X-ray pulsar be hiding amid the debris of SN 1987A?,
P. Esposito et al.,
857
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[Esposito:2018nib] - [18-29]
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Explaining the morphology of supernova remnant (SNR) 1987A with the jittering jets explosion mechanism,
Ealeal Bear, Noam Soker,
478
arXiv:1803.03946.
[Bear:2018ssf] - [18-30]
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Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle,
Jae Hyeok Chang, Rouven Essig, Samuel D. McDermott,
1809
arXiv:1803.00993.
[Chang:2018rso] - [18-31]
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Interaction of the SN1987A Neutrino with the Galaxy,
Kenzo Ishikawa, Terry Sloan, Yutaka Tobita,
arXiv:1710.03441,
[Ishikawa:2017yrb] - [18-32]
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Updated Constraints on Self-Interacting Dark Matter from Supernova 1987A,
Cameron Mahoney, Adam K. Leibovich, Andrew R. Zentner,
D96
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[Mahoney:2017jqk] - [18-33]
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Evidence for two neutrinos bursts from SN1987A,
R. Valentim, J. E. Horvath, E. M. Rangel,
45
arXiv:1706.07824.
[Valentim:2017ihe] - [18-34]
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Revisiting Supernova 1987A Constraints on Dark Photons,
Jae Hyeok Chang, Rouven Essig, Samuel D. McDermott,
1701
arXiv:1611.03864.
[Chang:2016ntp] - [18-35]
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New analysis for the correlation between gravitational waves and neutrino detectors during SN1987A,
P. Galeotti, G. Pizzella,
C76
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[Galeotti:2016uum] - [18-36]
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The Mont Blanc mystery solved? A $m^2=-0.28 keV^2$ neutrino,
Robert Ehrlich,
85
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[Ehrlich:2016ljp] - [18-37]
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Neutrino Signal of Collapse-Induced Thermonuclear Supernovae: The Case for Prompt Black Hole Formation in SN1987A,
Kfir Blum, Doron Kushnir,
828
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[Blum:2016afe] - [18-38]
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Nucleon-nucleon bremsstrahlung of dark gauge bosons and revised supernova constraints,
Ermal Rrapaj, Sanjay Reddy,
C94
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[Rrapaj:2015wgs] - [18-39]
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Supernova 1987A: neutrino-driven explosions in three dimensions and light curves,
Victor Utrobin, Annop Wongwathanarat, H.-Thomas Janka, Ewald Mueller,
arXiv:1412.4122,
[1412.4122] - [18-40]
-
Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles,
Alexandre Payez et al.,
1502
arXiv:1410.3747.
[Payez:2014xsa] - [18-41]
-
Comparative analysis of SN1987A antineutrino fluence,
Francesco Vissani,
G42
arXiv:1409.4710.
[Vissani:2014doa] - [18-42]
-
Signatures of Neutrino Cooling in the SN1987A Scenario,
Cristian G. Bernal, Nissim Fraija, Hidalgo-Gamez A. M,
442
arXiv:1402.6292.
[Fraija:2014qup] - [18-43]
-
Evidence for two neutrino mass eigenstates from SN 1987A and the possibility of superluminal neutrinos,
Robert Ehrlich,
35
arXiv:1111.0502.
[Ehrlich:2011kb] - [18-44]
-
Neutrino mass bound in the standard scenario for supernova electronic antineutrino emission,
Giulia Pagliaroli, Fernando Rossi-Torres, Francesco Vissani,
33
arXiv:1002.3349.
[Pagliaroli:2010ik] - [18-45]
-
The likelihood for supernova neutrino analyses,
A. Ianni et al.,
D80
arXiv:0907.1891.
[Ianni:2009bd] - [18-46]
-
Active and Sterile Neutrino Emission and SN1987A Pulsar Velocity,
Leonard S Kisslinger, Sandip Pakvasa,
arXiv:0906.4117,
[Kisslinger:2009xb] - [18-47]
-
Could the compact remnant of SN 1987A be a quark star?,
T. C. Chan et al.,
695
arXiv:0902.0653.
[Chan:2009mw] - [18-48]
-
Bounds on the Parameter of Noncommutativity from Supernova SN1987A,
Mansour Haghighat,
D79
arXiv:0901.1069.
[Haghighat:2009pv] - [18-49]
-
Improved analysis of SN1987A antineutrino events,
G. Pagliaroli, F. Vissani, M.L. Costantini, A. Ianni,
31
arXiv:0810.0466.
[Pagliaroli:2008ur] - [18-50]
-
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,
[Vissani:2008ac] - [18-51]
-
Bounds on large extra dimensions from photon fusion process in SN1987A,
V. H. Satheeshkumar, P. K. Suresh,
0806
arXiv:0805.3429.
[Satheeshkumar:2008fb] - [18-52]
-
SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels,
Leonard S. Kisslinger, Sandip Pakvasa,
arXiv:0802.1689,
[Kisslinger:2008rx] - [18-53]
-
Constraints on Astro-unparticle Physics from SN 1987A,
Sukanta Dutta, Ashok Goyal,
0803
arXiv:0712.0145.
[Dutta:2007tz] - [18-54]
-
Statistical analysis of neutrino events from SN1987A neutrino burst: estimation of the electron antineutrino mass,
B. I. Goryachev,
arXiv:0709.4627,
[Goryachev:2007xg] - [18-55]
-
Unparticle constraints from SN1987A,
Steen Hannestad, Georg Raffelt, Yvonne Y. Y. Wong,
D76
arXiv:0708.1404.
[Hannestad:2007ys] - [18-56]
-
Supernovae as Probes of Extra Dimensions,
V. H. Satheesh Kumar, P. K. Suresh, P. K. Das,
939
arXiv:0706.3551.
[SatheeshKumar:2007gb] - [18-57]
-
The first second of SN1987A neutrino emission,
G. Pagliaroli, M.L. Costantini, A. Ianni, F. Vissani,
arXiv:0705.4032,
[Pagliaroli:2007sd] - [18-58]
-
High resolution spectroscopy of the line emission from the inner circumstellar ring of SN 1987A and its hot spots,
Per Groeningsson et al.,
arXiv:astro-ph/0703788.
[Groeningsson:2007nh] - [18-59]
-
Neutrino Spectrum from SN 1987A and from Cosmic Supernovae,
Hasan Yuksel, John F. Beacom,
D76
arXiv:astro-ph/0702613.
[Yuksel:2007mn] - [18-60]
-
Magnetic field in supernova remnant SN 1987A,
E.G. Berezhko, L.T. Ksenofontov,
650
arXiv:astro-ph/0608586.
[Berezhko:2006vv] - [18-61]
-
Is there a problem with low energy SN1987A neutrinos?,
Maria Laura Costantini, Aldo Ianni, Giulia Pagliaroli, Francesco Vissani,
0705
arXiv:astro-ph/0608399.
[Costantini:2006xd] - [18-62]
-
Constraints on neutrino mixing angle $\theta_{13}$ and Supernova neutrino fluxes from the LSD neutrino signal from SN1987A,
Oleg Lychkovskiy,
arXiv:hep-ph/0604113,
[Lychkovskiy:2006yw] - [18-63]
-
Evolution of the Reverse Shock Emission from SNR 1987A,
Kevin Heng et al.,
644
arXiv:astro-ph/0603151.
[Heng:2006nt] - [18-64]
-
Lower neutrino mass bound from SN1987A data and quantum geometry,
G. Lambiase, G. Papini, R. Punzi, G. Scarpetta,
23
arXiv:gr-qc/0512154.
[Lambiase:2005ui] - [18-65]
-
New analysis of the SN 1987A neutrinos with a flexible spectral shape,
Alessandro Mirizzi, Georg G. Raffelt,
D72
arXiv:astro-ph/0508612.
[Mirizzi:2005tg] - [18-66]
-
The Three-Dimensional Circumstellar Environment of SN 1987A,
Ben E. K. Sugerman et al.,
159
arXiv:astro-ph/0502378.
[Sugerman:2005dr] - [18-67]
-
The Light Curve of Supernova 1987A: The Structure of the Presupernova and Radioactive Nickel Mixing,
V. P. Utrobin,
30
arXiv:astro-ph/0406410.
[Utrobin:2004rt] - [18-68]
-
SN1987A and the properties of neutrino burst,
Maria Laura Costantini, Aldo Ianni, Francesco Vissani,
D70
arXiv:astro-ph/0403436.
[Costantini:2004ry] - [18-69]
-
Constraints on a Putative Pulsar in SN 1987A,
H. Ogelman, M.A. Alpar,
603
arXiv:astro-ph/0402147.
[Ogelman:2004iu] - [18-70]
-
Neutrinos from SN1987A: flavor conversion and interpretation of results,
C. Lunardini, A. Yu. Smirnov,
21
arXiv:hep-ph/0402128.
[Lunardini:2004bj] - [18-71]
-
A Rotating Collapsar and Possible Interpretation of the LSD Neutrino Signal from SN 1987A,
V.S. Imshennik, O.G. Ryazhskaya,
30
arXiv:astro-ph/0401613.
[Imshennik:2004iya] - [18-72]
-
Evidence of non-zero mass features for the neutrinos emitted at Supernova LMC-'87A,
Humiaki Huzita,
arXiv:hep-ph/0212337,
[Huzita:2002ia] - [18-73]
-
Supernova 1987A did not test the neutrino mass hierarchy,
V. Barger, D. Marfatia, B. P. Wood,
B532
arXiv:hep-ph/0202158.
[Barger:2002px] - [18-74]
-
SN1987A and the status of oscillation solutions to the solar neutrino problem,
M. Kachelriess, A. Strumia, R. Tomas, J. W. F. Valle,
D65
arXiv:hep-ph/0108100.
[Kachelriess:2001sg] - [18-75]
-
Bayesian analysis of neutrinos observed from supernova SN 1987A,
Thomas J. Loredo, Don Q. Lamb,
D65
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] - [18-76]
-
Large lepton mixing and supernova 1987A,
M. Kachelriess, R. Tomas, J. W. F. Valle,
01
arXiv:hep-ph/0012134.
[Kachelriess:2000fe] - [18-77]
-
Inverted hierarchy of neutrino masses disfavored by supernova 1987A,
Hisakazu Minakata, Hiroshi Nunokawa,
B504
arXiv:hep-ph/0010240.
[Minakata:2000rx] - [18-78]
-
Neutrinos from SN1987A, Earth matter effects and the LMA solution of the solar neutrino problem,
C. Lunardini, A. Yu. Smirnov,
D63
arXiv:hep-ph/0009356.
[Lunardini:2000sw] - [18-79]
-
SN1987A: A testing ground for the KARMEN anomaly,
I. Goldman, R. Mohapatra, S. Nussinov,
B481
arXiv:hep-ph/9912465.
[Goldman:1999hg] - [18-80]
-
Contact interactions involving right-handed neutrinos and SN 1987A,
J. A. Grifols, E. Masso, R. Toldra,
D57
arXiv:hep-ph/9707531.
[Grifols:1997iy] - [18-81]
-
Gamma rays from SN1987A due to pseudoscalar conversion,
J. A. Grifols, E. Masso, R. Toldra,
77
arXiv:astro-ph/9606028.
[Grifols:1996id] - [18-82]
-
Gamma-rays and the decay of neutrinos from SN1987A,
Andrew H. Jaffe, Michael S. Turner,
D55
arXiv:astro-ph/9601104.
[Jaffe:1995sw] - [18-83]
-
Bounds on the neutrino magnetic moment from SN1987A,
A. Goyal, S. Dutta, S. R. Choudhury,
B346
[Goyal:1995yd] - [18-84]
-
Testing special relativity with SN1987A neutrino pulses,
E. Atzmon, S. Nussinov,
B328
[Atzmon:1994ch] - [18-85]
-
Constraints from nucleosynthesis and SN1987A on majoron emitting double beta decay,
Sanghyeon Chang, Kiwoon Choi,
D49
arXiv:hep-ph/9303243.
[Chang:1993yp] - [18-86]
-
Massive Dirac neutrinos and SN1987A,
Adam Burrows, Raj Gandhi, MIchael S. Turner,
68
[Burrows:1992ec] - [18-87]
-
Constraints to the decays of Dirac neutrinos from SN1987A,
Scott Dodelson, Joshua A. Frieman, Michael S. Turner,
68
[Dodelson:1992tv] - [18-88]
-
Dirac neutrinos and SN1987A,
Michael S. Turner,
D45
[Turner:1992ax] - [18-89]
-
Massive Dirac neutrinos and the SN1987A signal,
Raj Gandhi, Adam Burrows,
B246
[Gandhi:1990bq] - [18-90]
-
limits on the muon-neutrino and tau-neutrino masses from SN1987A,
J. A. Grifols, E. Masso,
B242
[Grifols:1990jn] - [18-91]
-
E(6) models confront SN1987A,
J. A. Grifols, E. Masso, T. G. Rizzo,
D42
[Grifols:1990tk] - [18-92]
-
comment on 'constraints on the majoron interactions from the supernova SN1987A.',
Y. Aharonov, F. T. Avignone, S. Nussinov,
D39
[Aharonov:1989ik] - [18-93]
-
axions and SN1987A,
Adam Burrows, Michael S. Turner, R. P. Brinkmann,
D39
[Burrows:1989ah] - [18-94]
-
Neutrino helicity flips via electroweak interactions and SN1987A,
K. J. F. Gaemers, R. Gandhi, J. m. Lattimer,
D40
[Gaemers:1989fp] - [18-95]
-
Charge radius of the neutrino: a limit from SN1987A,
J. A. Grifols, E. Masso,
D40
[Grifols:1989vi] - [18-96]
-
Limits to the Radiative Decays of Neutrinos and Axions from Gamma-Ray Observations of SN 1987a,
Edward W. Kolb, Michael S. Turner,
62
[Kolb:1988pe] - [18-97]
-
Constraints on decaying right-handed majorana neutrinos from SN1987A observations,
R. N. Mohapatra, S. Nussinov,
D39
[Mohapatra:1989su] - [18-98]
-
constraints on the neutrino mass from the supernova data: a systematic analysis,
L. F. Abbott, A. De Rujula, T. P. Walker,
B299
[Abbott:1988bm] - [18-99]
-
implications of the triplet - majoron model for the supernova SN1987A,
Y. Aharonov, F. T. Avignone, S. Nussinov,
D37
[Aharonov:1988ee] - [18-100]
-
Limit on the magnetic moment of the neutrino from supernova SN1987A observations,
Riccardo Barbieri, Rabindra N. Mohapatra,
61
[Barbieri:1988nh] - [18-101]
-
The magnetic moment of the neutrino and its implications for neutrino signal from SN1987A,
Riccardo Barbieri, R. N. Mohapatra, T. Yanagida,
B213
[Barbieri:1988xw] - [18-102]
-
Correlation mass method for analysis of neutrinos from supernova 1987A,
H. Chiu, K. L. Chan, Y. Kondo,
329
[Chiu-Chan-Kondo-1988ApJ-329-326C] - [18-103]
-
neutrino masses and flavors emitted in the supernova SN1987A,
R. Cowsik,
D37
From the abstract: The analysis of the energies and times of arrival of neutrino events in the Kamioka and IMB detectors yelds two mass groupings at $\sim 22 \, \mathrm{eV}$ and the other at $\sim 4 \, \mathrm{eV}$, if all neutrinos were released rapidly at the supernova.
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.).
[Cowsik:1988xr] - [18-104]
-
Neutrino mixing, decays and supernova SN1987a,
Joshua A. Frieman, Howard E. Haber, Katherine Freese,
B200
[Frieman:1988as] - [18-105]
-
Implications of the supernova SN1987A neutrino signals,
I. Goldman, Y. Aharonov, G. Alexander, S. Nussinov,
60
[Goldman:1988fg] - [18-106]
-
Supernova neutrinos and their oscillations,
T. K. Kuo, James T. Pantaleone,
D37
[Kuo:1987qu-SN1987A] - [18-107]
-
limits on the neutrino magnetic moment from SN1987A,
J. M. Lattimer, J. Cooperstein,
61
[Lattimer:1988mf] - [18-108]
-
New Bounds on Neutrino Magnetic Moments From Stellar Collapse,
Dirk Notzold,
D38
[Notzold:1988kz] - [18-109]
-
bounds on exotic particle interactions from SN1987A,
Georg Raffelt, David Seckel,
60
[Raffelt:1988yt] - [18-110]
-
Remarks on the first two events in the supernova burst observed by Kamiokande-ii,
S. P. Rosen,
D37
[Rosen:1988yh] - [18-111]
-
The mass of the electron-neutrino: monte carlo studies of SN1987A observations,
David N. Spergel, J. N. Bahcall,
B200
[Spergel:1988ex] - [18-112]
-
Statistical analysis of the neutrino burst from SN1987A,
Hideyuki Suzuki, Katsuhiko Sato,
79
[Suzuki:1988qi] - [18-113]
-
Neutrino mass limits from SN1987A,
W. David Arnett, Jonathan L. Rosner,
58
[Arnett:1987iz] - [18-114]
-
Neutrinos from the supernova in the LMC,
J. N. Bahcall, A. Dar, T. Piran,
326
[Bahcall:1987fz] - [18-115]
-
Upper limit on the mass of the electron-neutrino,
J. N. Bahcall, S. L. Glashow,
326
[Bahcall:1987nx] - [18-116]
-
Neutrino temperatures and fluxes from the LMC supernova,
J. N. Bahcall, T. Piran, W. H. Press, D. N. Spergel,
327
[Bahcall:1987ua] - [18-117]
-
Electric Charge of the Neutrinos from SN1987A,
G. Barbiellini, G. Cocconi,
329
[Barbiellini:1987zz] - [18-118]
-
constraints on the lifetime of massive neutrinos from SN1987A,
Arnon Dar, Shlomo Dado,
59
[Dar:1987nq] - [18-119]
-
May a supernova bang twice?,
A. De Rujula,
B193
[DeRujula:1987pg] - [18-120]
-
Constraints on light particles from supernova SN1987A,
John R. Ellis, Keith A. Olive,
B193
[Ellis:1987pk] - [18-121]
-
Neutrino mass speculation on the neutrino events from the supernova LMC 1987 A,
H. Huzita,
A2
From the abstract: ... time to energy correlation in Kamiokande detector has 2 separate groups. Each group correspond to non zero neutrino mass $3.4 \pm 0.6$ and $23 \pm 4$ eV.
[Huzita:1987cg] - [18-122]
-
How Reliable Are Neutrino Mass Limits Derived from SN 1987a?,
Edward W. Kolb, Albert J. Stebbins, Michael S. Turner,
D35
[Addendum: Phys. Rev.D36,3820(1987)].
[Kolb:1987dda] - [18-123]
-
Neutrino spectroscopy of the supernova SN1987A,
Lawrence M. Krauss,
329
[Krauss:1987re] - [18-124]
-
SN1987A: a black hole precursor?,
S. Nussinov, I. Goldman, G. Alexander, Y. Aharonov,
329
[Nussinov:1987hk] - [18-125]
-
Analysis of neutrino burst from the supernova in LMC,
Katsuhiko Sato, Hideyuki Suzuki,
58
[Sato:1987rd] - [18-126]
-
Total energy of neutrino burst from the supernova SN1987A and the mass of neutron star just born,
Katsuhiko Sato, Hideyuki Suzuki,
B196
[Sato:1987yi] - [18-127]
-
Neutrinos from supernova SN1987A,
David N. Schramm,
17
From the article: ... without making specific model assumptions, all that can be safely said is $m_{\bar\nu_e} < 30 \, \mathrm{eV}$.
[Schramm:1987ra] - [18-128]
-
A simple model for neutrino cooling of the LMC supernova,
D. N. Spergel, T. Piran, A. Loeb, J. Goodman, J. N. Bahcall,
237
[Spergel:1987ch] - [18-129]
-
Constraint on the mass and lifetime of heavy neutrinos from the supernova SN1987A in the Large Magellanic Cloud,
Mariko Takahara, Katsuhiko Sato,
A2
[Takahara:1987gb]
- [19-1]
-
Neutrinos from SN 1987a. A Puzzle Revisited,
Gerd Schatz,
632
arXiv:1507.07107.
24th European Cosmic Ray Symposium Kiel 2014.
[Schatz:2015qxa] - [19-2]
-
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,
XVI International Seminar Quarks'2010, Kolomna, Moscow Region, June 6-12, 2010.
[Kuznetsov:2010fe] - [19-3]
-
What is the issue with SN1987A neutrinos?,
F. Vissani, M.L. Costantini, W. Fulgione, A. Ianni, G. Pagliaroli,
103
arXiv:1008.4726.
Vulcano Workshop 2010: Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, May 24-29, 2010.
[Vissani:2010zi] - [19-4]
-
Analysis of Neutrino Signals from SN1987A,
G. Pagliaroli, M. L. Costantini, F. Vissani,
arXiv:0804.4598,
IFAE 2007, 19th Conference on High Energy Physics: April 11-13 2007, Naples, Italy.
[Pagliaroli:2008qi] - [19-5]
-
Analysis of the SN1987A two-stage explosion hypothesis with account for the MSW neutrino flavour conversion,
Oleg Lychkovskiy,
arXiv:0707.2508,
Rencontres de Moriond EW 2007, 10-17 March 2007.
[Lychkovskiy:2007ru] - [19-6]
-
Neutrino events from SN1987A revisited,
B. Bekman, J. Holeczek, J. Kisiel,
B37
arXiv:hep-ph/0511271.
XXIX Mazurian Lakes Conference on Physics, August 30 - September 6, 2005, Piaski, Poland.
[Bekman:2005rp] - [19-7]
-
SN 1987A: The Unusual Explosion of a Normal Type II Supernova,
Nino Panagia,
arXiv:astro-ph/0410275.
International Conference '1604-2004 Supernovae as Cosmological Lighthouses' (Padova, Italy, June 16-19, 2004).
[Panagia:2004ii] - [19-8]
-
SN1987A: Temporal Models,
M.I.Wanas, M.Melek, M.E.Kahil,
arXiv:gr-qc/0306086,
MG IX (2002).
[Wanas:2003qq] - [19-9]
-
The precious information from supernova LMC-87A on the neutrino masses and neutrino mixing angles among the flavor states and the mass states,
H. Huzita,
63
2nd International Conference on Nonaccelerator New Physics (NANP 99), Dubna, Moscow Region, Russia, 28 June - 3 Jul 1999.
[Huzita:2000vd] - [19-10]
-
Analysis of Neutrinos from Supernova 1987A,
H. Y. Chiu, K. L. Chan, Y. Kondo,
422
[Chiu-Chan-Kondo-1988adse-conf-422C] - [19-11]
-
A Look at the Supernova SN 1987a,
David N. Schramm,
3
Lepton and photon interactions at high-energies. International symposium, Hamburg, F.R. Germany, July 27-31, 1987.
[Schramm:1987bv] - [19-12]
-
Mass determination of neutrinos,
H. Y. Chiu,
IN 'FAIRFAX 1987, PROCEEDINGS, SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD' 185-193.
[Chiu:1987cf] - [19-13]
-
Neutrino masses from SN1987a,
Jerrold Franklin,
IN 'FAIRFAX 1987, PROCEEDINGS, SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD' 197-199.
[Franklin:1987nz]
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Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A,
C. Fransson et al.,
383
arXiv:2403.04386.
[Fransson:2024csf] - [20-2]
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Favorable conditions for heavy element nucleosynthesis in rotating proto-magnetar winds,
Tejas Prasanna, Matthew S. B. Coleman, Todd A. Thompson,
arXiv:2402.06003,
[Prasanna:2024pcq] - [20-3]
-
Long-rising Type II supernovae resembling supernova 1987A - I. A comparative study through scaling relations,
M. L. Pumo, S. P. Cosentino, A. Pastorello, S. Benetti, S. Cherubini, G. Manico, L. Zampieri,
521
arXiv:2303.10478.
[Pumo:2023qoy] - [20-4]
-
Proto-Neutron Star Convection and the Neutrino-Driven Wind: Implications for the r-Process,
Brian Nevins, Luke F. Roberts,
520
arXiv:2302.01249.
[Nevins:2023tug] - [20-5]
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Updating the $^{56}$Ni Problem in Core-collapse Supernova Explosion,
Ryo Sawada, Yudai Suwa,
arXiv:2301.03610,
[Sawada:2023iau] - [20-6]
-
On the maximum luminosities of normal stripped-envelope supernovae - brighter than explosion models allow,
J. Sollerman, S. Yang, D. Perley, S. Schulze, C. Fremling, M. Kasliwal, K. Shin, B. Racine,
657
arXiv:2109.14339.
[Sollerman:2021svd] - [20-7]
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Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae,
Oliver Eggenberger Andersen, Shuai Zha, Andre da Silva Schneider, Aurore Betranhandy, Sean M. Couch, Evan P. O'Connor,
923
arXiv:2106.09734.
[Andersen:2021vzo] - [20-8]
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Comparing Compact Object Distributions from Mass- and Presupernova Core Structure-based Prescriptions,
Rachel A. Patton, Tuguldur Sukhbold, J.J. Eldridge,
511
arXiv:2106.05978.
[Patton:2021gwh] - [20-9]
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Chiral Selection, Isotopic Abundance Shifts, and Autocatalysis of Meteoritic Amino Acids,
Michael A. Famiano, Richard N. Boyd, Takashi Onaka, Toshitaka Kajino,
3
arXiv:2106.01531.
[Famiano:2021qqq] - [20-10]
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Failed Supernova Remnants,
Daichi Tsuna,
73
arXiv:2104.10512.
[Tsuna:2021wee] - [20-11]
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The Impact of Black Hole Formation on Population Averaged Supernova Yields,
Emily J. Griffith, Tuguldur Sukhbold, David H. Weinberg, Jennifer A. Johnson, James W. Johnson, Fiorenzo Vincenzo,
arXiv:2103.09837,
[2103.09837] - [20-12]
-
The Nucleosynthetic Yields of Core-Collapse Supernovae, prospects for the Next Generation of Gamma-Ray Astronomy,
Sydney Andrews, Chris L. Fryer, Samuel W. Jones, Wesley P. Even, Marco Pignatari,
arXiv:1912.10542,
[Andrews:2019spm]
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Nucleosynthesis in the Innermost Ejecta of Magnetorotational Supernova Explosions in 3-dimensions,
Shuai Zha, Bernhard Muller, Jade Powell,
arXiv:2403.02072,
[Zha:2024fyo] - [21-2]
-
Grey Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations,
Haakon Andresen, Evan P. O'Connor, Oliver Eggenberger Andersen, Sean M. Couch,
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M. Liebendoerfer, M. Rampp, H.-Th. Janka, A. Mezzacappa,
620
arXiv:astro-ph/0310662.
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.
[Liebendoerfer:2003es] - [21-312]
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Core-Collapse Supernova Mechanism - Importance of Rotation,
A. Odrzywolek, M. Kutschera, M. Misiaszek, K. Grotowski,
arXiv:astro-ph/0310047.
[Odrzywolek:2003qc] - [21-313]
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3-Dimensional Core-Collapse,
Chris L. Fryer, Michael S. Warren,
601
arXiv:astro-ph/0309539.
[Fryer:2003jj] - [21-314]
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Pulsar Recoil by Large-Scale Anisotropies in Supernova Explosions,
L. Scheck, T. Plewa, Hans-Thomas Janka, K. Kifonidis, E. Mueller,
92
arXiv:astro-ph/0307352.
[Scheck:2003rw] - [21-315]
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Evolution, Explosion and Nucleosynthesis of Core Collapse Supernovae,
M. Limongi, A. Chieffi,
592
arXiv:astro-ph/0304185.
[Limongi:2003ui] - [21-316]
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Improved Models of Stellar Core Collapse and Still no Explosions: What is Missing?,
R. Buras, M. Rampp, H.-Th. Janka, K. Kifonidis,
90
arXiv:astro-ph/0303171.
[Buras:2003sn] - [21-317]
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Electron capture rates on nuclei and implications for stellar core collapse,
K. Langanke et al.,
90
arXiv:astro-ph/0302459.
[Langanke:2003ii] - [21-318]
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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,
408
arXiv:astro-ph/0302239.
[Kifonidis:2003fv] - [21-319]
-
Shock breakout in core-collapse supernovae and its neutrino signature,
Todd A. Thompson, Adam Burrows, Philip A. Pinto,
592
arXiv:astro-ph/0211194.
[Thompson:2002mw] - [21-320]
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Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae,
J. M. Blondin, A. Mezzacappa, C. DeMarino,
584
arXiv:astro-ph/0210634.
[Blondin:2002sm] - [21-321]
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A finite difference representation of neutrino radiation hydrodynamics for spherically symmetric general relativistic supernova simulations,
M. Liebendoerfer et al.,
150
arXiv:astro-ph/0207036.
[Liebendoerfer:2002xn] - [21-322]
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Modeling Core-Collapse Supernovae in Three Dimensions,
C.L. Fryer, M.S. Warren,
574
arXiv:astro-ph/0206017.
[Fryer:2002zw] - [21-323]
-
Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations,
H.-T. Janka M. Rampp,
396
arXiv:astro-ph/0203101.
[Rampp:2002bq] - [21-324]
-
NewtonPlus: Approximate Relativity for Supernova Simulations,
Christian Y. Cardall, Anthony Mezzacappa, Matthias Liebendorfer,
arXiv:astro-ph/0106105.
[Cardall:2001fu] - [21-325]
-
Spherical collapse of supermassive stars: neutrino emission and gamma-ray bursts,
Felix Linke, Jose A. Font, Hans-Thomas Janka, E. Mueller, Philippos Papadopoulos,
arXiv:astro-ph/0103144.
[Linke:2001mq] - [21-326]
-
General Relativistic Effects in the Core Collapse Supernova Mechanism,
S. W. Bruenn, K. R. De Nisco, A. Mezzacappa,
560
arXiv:astro-ph/0101400.
[Bruenn:2001vu] - [21-327]
-
Conservative General Relativistic Radiation Hydrodynamics in Spherical Symmetry and Comoving Coordinates,
Matthias Liebendorfer, Anthony Mezzacappa, Friedrich-Karl Thielemann,
D63
arXiv:astro-ph/0012201.
[Liebendoerfer:2000fw] - [21-328]
-
Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae,
H.-Th. Janka,
368
arXiv:astro-ph/0008432.
[Janka:2000bt] - [21-329]
-
Probing the gravitational well: No supernova explosion in spherical symmetry with general relativistic Boltzmann neutrino transport,
Matthias Liebendorfer et al.,
D63
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 [21-330], Mezzacappa and others [21-331], Bruenn and others [21-326]).
[Liebendoerfer:2000cq] - [21-330]
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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,
539
arXiv:astro-ph/0005438.
[Rampp:2000ws] - [21-331]
-
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.,
86
arXiv:astro-ph/0005366.
From the abstract: In this model, a supernova explosion is not obtained.
[Mezzacappa:2000jb] - [21-332]
-
A new algorithm for supernova neutrino transport and some applications,
A. Burrows, T. Young, P. Pinto, R. Eastman, T. A. Thompson,
539
[Burrows:2000xsm] - [21-333]
-
Future detection of supernova neutrino burst and explosion mechanism,
T. Totani, K. Sato, H. E. Dalhed, J. R. Wilson,
496
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.
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An investigation of neutrino-driven convection and the core collapse supernova mechanism using multigroup neutrino transport,
A. Mezzacappa et al.,
arXiv:astro-ph/9612107.
[Mezzacappa:1996ae] - [21-335]
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On the nature of core collapse supernova explosions,
Adam Burrows, John Hayes, Bruce A. Fryxell,
450
arXiv:astro-ph/9506061.
[Burrows:1995ww] - [21-336]
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Neutrino Emission from Type II Supernovae: The First 100 Milliseconds,
E. Myra, A. Burrows,
364
[Myra-Burrows-ApJ364-222-1989] - [21-337]
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The Hydrodynamic Behavior of Supernovae Explosions,
S. A. Colgate, R. H. White,
143
[Colgate-White-ApJ143-1966]
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Core-Collapse Supernova Simulations including Neutrino Interactions from the Virial EOS,
Evan O'Connor, C.J. Horowitz, Zidu Lin, Sean Couch,
331
arXiv:1712.08253.
IAU Symposium 331, SN 1987A, 30 years later - Cosmic Rays and Nuclei from Supernovae and Their Aftermaths.
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Gravitational wave signals from multi-dimensional core-collapse supernova explosion simulations,
K.N. Yakunin et al.,
arXiv:1710.08372,
52nd Rencontres de Moriond.
[Yakunin:2017sls] - [22-3]
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Simulations of Electron Capture and Low-Mass Iron Core Supernovae,
B. Muller et al.,
88
arXiv:1710.02641.
The AGB-Supernova Mass Transition.
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Spatial distribution of radionuclides in 3D models of SN 1987A and Cas A,
H.-Thomas Janka, Michael Gabler, Annop Wongwathanarat,
324
arXiv:1705.01159.
SN 1987A, 30 years later, IAU Symposium No. 331, 2017.
[Janka:2017nhh] - [22-5]
-
Multi-dimensional Core-Collapse Supernova Simulations with Neutrino Transport,
Kuo-Chuan Pan, Matthias Liebendorfer, Matthias Hempel, Friedrich-Karl Thielemann,
14
arXiv:1701.06701.
Nuclei in the Cosmos XIV, Niigata, Japan (2016).
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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,
14
arXiv:1701.05203.
14th International Symposium on Nuclei in the Cosmos (NIC-XIV).
[Sinha:2017hnn] - [22-7]
-
Constraining the supersaturation density equation of state from core-collapse supernova simulations - Excluded volume extension of the baryons,
Tobias Fischer,
A52
arXiv:1604.01629.
EPJA topical issue 'Exotic Matter in Neutron Stars'.
[Fischer:2016jkc] - [22-8]
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Expected impact from weak reactions with light nuclei in core-collapse supernova simulations,
T. Fischer et al.,
109
arXiv:1512.00193.
OMEG 2015.
[Fischer:2015sll] - [22-9]
-
Multimessengers from 3D Core-Collapse Supernovae,
Konstantin N. Yakunin et al.,
arXiv:1507.05901,
50th Rencontres de Moriond on Gravitation: La Thuile, Italy, March 21-28, 2014.
[Yakunin:2015nma] - [22-10]
-
A Neutrino-Driven Core Collapse Supernova Explosion of a 15 M Star,
Anthony Mezzacappa et al.,
arXiv:1507.05680,
ASTRONUM 2014.
[Mezzacappa:2015bma] - [22-11]
-
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.,
488
arXiv:1405.7075.
ASTRONUM 2013.
[Mezzacappa:2014era] - [22-12]
-
Towards Petaflops Capability of the VERTEX Supernova Code,
Andreas Marek, Markus Rampp, Florian Hanke, Hans-Thomas Janka,
arXiv:1404.1719,
[1404.1719] - [22-13]
-
Two- and three-dimensional simulations of core-collapse supernovae with CHIMERA,
Eric J. Lentz et al.,
NICXII
arXiv:1301.1326.
12th Symposium on Nuclei in the Cosmos. 5-12 August 2012.
[Lentz:2012tel] - [22-14]
-
Numerical modeling of core-collapse supernovae and compact objects,
K. Sumiyoshi,
291
arXiv:1212.6131.
IAUS 291 'Neutron Stars and Pulsars: Challenges and Opportunities after 80 years'.
[Sumiyoshi:2012un] - [22-15]
-
Exploding SNe with jets: time-scales,
Oded Papish, Noam Soker,
279
arXiv:1204.2560.
IAU Symposium No. 279, 2012.
[Papish:2012qx] - [22-16]
-
General Relativistic Explosion Models of Core-Collapse Supernovae,
Bernhard Mueller, Andreas Marek, Hans-Thomas Janka, Harald Dimmelmeier,
459
arXiv:1112.1920.
[Mueller:2011aa] - [22-17]
-
Studies of Stellar Collapse and Black Hole Formation with the Open-Source Code GR1D,
Christian D. Ott, Evan O'Connor,
1269
arXiv:1011.0005.
OMEG10 Symposium, Osaka, Japan, March 8-10, 2010.
[Ott:2010mk] - [22-18]
-
Mechanisms of Core-Collapse Supernovae $\text{\&}$ Simulation Results from the CHIMERA Code,
S. W. Bruenn et al.,
1111
arXiv:1002.4909.
Probing Stellar Populations Out To The Distant Universe: Cefalu 2008.
[Bruenn:2009mgs] - [22-19]
-
NICXI
[Arcones:2010nj] - [22-20]
-
Computational Models of Stellar Collapse and Core-Collapse Supernovae,
C. D. Ott et al.,
180
arXiv:0907.4043.
DOE/SciDAC 2009.
[Ott:2009ii] - [22-21]
-
Nucleosynthesis Calculations from Core-Collapse Supernovae,
Christopher L. Fryer et al.
(The NuGrid),
arXiv:0811.4648,
10th Symposium on Nuclei in the Cosmos (NIC X), July 27 - August 1 2008, Mackinack Island, Michigan, USA.
[NuGrid:2008iti] - [22-22]
-
Supernova explosions and the birth of neutron stars,
H.-Th. Janka, A. Marek, B. Mueller, L. Scheck,
983
arXiv:0712.3070.
40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More, August 12-17, 2007, McGill Univ., Montreal, Canada.
[Janka:2007hi] - [22-23]
-
Nuclear physics with spherically symmetric supernova models,
M. Liebendoerfer, T. Fischer, C. Frohlich, F.-K. Thielemann, S. Whitehouse,
G35
arXiv:0708.4296.
NPA III, Dresden 2007.
[Liebendoerfer:2007hq] - [22-24]
-
Multi-Dimensional Explorations in Supernova Theory,
Adam Burrows, Luc Dessart, Christian D. Ott, Eli Livne,
442
arXiv:astro-ph/0612460.
Centennial Festschrift for Hans Bethe, 2006.
[Burrows:2006ci] - [22-25]
-
Collapse and black hole formation in magnetized, differentially rotating neutron stars,
Branson C. Stephens et al.,
24
arXiv:gr-qc/0610103.
New Frontiers in Numerical Relativity, the Albert Einstein Institute, Potsdam, July 17-21, 2006.
[Stephens:2006cn] - [22-26]
-
Efficient approximations of neutrino physics for three-dimensional simulations of stellar core collapse,
M. Liebendoerfer, U.-L. Pen, C. Thompson,
NIC-IX
arXiv:astro-ph/0609651.
Nuclei in the Cosmos IX, Geneva, June 25-30.
[Liebendorfer:2006et] - [22-27]
-
Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae,
Kei Kotake, Naofumi Ohnishi, Shoichi Yamada, Katsuhiko Sato,
31
arXiv:astro-ph/0511826.
Third 21COE Symposium : Astrophysics as Interdisciplinary Science, Waseda University, Japan, September 1-3, 2005.
[Kotake:2005ng] - [22-28]
-
Toward Five-dimensional Core-collapse Supernova Simulations,
Christian Y. Cardall et al.,
16
arXiv:astro-ph/0510706.
SciDAC 2005, Scientific Discovery through Advanced Computing, San Francisco, CA, 26-30 June 2005.
[Cardall:2005id] - [22-29]
-
The Long Term: Six-dimensional Core-collapse Supernova Models,
Christian Y. Cardall, Alexei O. Razoumov, Eirik Endeve, Anthony Mezzacappa,
arXiv:astro-ph/0510704,
Open Issues in Understanding Core Collapse Supernovae, National Institute for Nuclear Theory, University of Washington, 22-24 June 2004.
[Cardall:2005ib] - [22-30]
-
Multigroup Models of the Convective Epoch in Core Collapse Supernovae,
F. Douglas Swesty, Eric S. Myra,
16
arXiv:astro-ph/0507294.
SciDAC 2005, San Francisco, CA, USA, 26-30 June 2005.
[Swesty:2005jv] - [22-31]
-
An approach toward the successful supernova explosion by physics of unstable nuclei,
K. Sumiyoshi et al.,
A758
arXiv:astro-ph/0506619.
Nuclei in the Cosmos 8.
[Sumiyoshi:2005rh] - [22-32]
-
Issues with Core-Collapse Supernova Progenitor Models,
Stephen W. Bruenn,
arXiv:astro-ph/0506313,
Workshop on Open Issues in Understanding Core Collapse Supernovae, Seattle, Washington, 22-24 June 2004.
[Bruenn:2005hv] - [22-33]
-
Magnetic Fields in Core Collapse Supernovae: Possibilities and Gaps,
J. Craig Wheeler, Shizuka Akiyama,
arXiv:astro-ph/0412382,
INT workshop 'Open Issues in Understanding Core Collapse Supernovae,' Seattle, 2004.
[Wheeler:2004ff] - [22-34]
-
Neutrino-Driven Supernovae: an Accretion Instability in a Nuclear Physics Controlled Environment,
Hans-Thomas Janka et al.,
A758
arXiv:astro-ph/0411347.
8th Symposium on Nuclei in the Cosmos, Vancouver, BC, Canada, 19-23 Jul 2004.
[Janka:2004an] - [22-35]
-
Magnetorotational supernova simulations,
S.G. Moiseenko, G.S. Bisnovatyi-Kogan, N.V. Ardeljan,
arXiv:astro-ph/0410330.
International Conference '1604-2004 Supernovae as Cosmological Lighthouses' (Padova, Italy, June 16-19, 2004).
[Moiseenko:2004vg] - [22-36]
-
The Core Collapse Supernova Mechanism: Current Models, Gaps, and the Road Ahead,
Anthony Mezzacappa,
342
arXiv:astro-ph/0410085.
Supernovae as Cosmological Lighthouses, Padua, Italy, June 16-19, 2004.
[Mezzacappa:2004ic] - [22-37]
-
Early Spectra of Supernovae,
E. Baron, Peter Nugent, David Branch, Peter H. Hauschildt,
arXiv:astro-ph/0409659.
1604-2004 Supernovae As Cosmological Lighthouses, San Francisco.
[Baron:2004nw] - [22-38]
-
Rotating Core Collapse and Bipolar Supernova Explosions,
Adam Burrows, Rolf Walder, Christian D. Ott, Eli Livne,
arXiv:astro-ph/0409035.
Fate of the Most Massive Stars, Grand Teton National Park, Wyoming, 23-28 May 2004.
[Burrows:2004va] - [22-39]
-
Understanding Core-Collapse Supernovae,
Adam Burrows,
arXiv:astro-ph/0405427,
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] - [22-40]
-
Core-Collapse Supernovae: Modeling between Pragmatism and Perfectionism,
H.-Th. Janka et al.,
arXiv:astro-ph/0405289,
12th Workshop on Nuclear Astrophysics, Ringberg Castle, March 22-27, 2004.
[Janka:2004tt] - [22-41]
-
Fifty-Nine Reasons for a Supernova to not Explode,
M. Liebendoerfer,
arXiv:astro-ph/0405029,
12th Workshop on 'Nuclear Astrophysics', Ringberg Castle, March 22-27, 2004.
[Liebendoerfer:2004fk] - [22-42]
-
An Approach to Neutrino Radiative Transfer in Supernova Simulations,
Christian Y. Cardall,
arXiv:astro-ph/0404401,
Numerical Methods for Multidimensional Radiative Transfer Problems (RadConf2003), Heidelberg, Germany, 24-26 September 2003.
[Cardall:2004nd] - [22-43]
-
Synthetic Spectrum Methods for Three-Dimensional Supernova Models,
R. C. Thomas,
arXiv:astro-ph/0310619,
'3-D Signatures in Stellar Explosions', Austin, Texas.
[Thomas:2003ue] - [22-44]
-
Effects of Small-Scale Fluctuations of Neutrino Flux in Supernova Explosions,
H. Madokoro, T. Shimizu, Y. Motizuki,
99
arXiv:astro-ph/0310481.
IAU Colloquium 192, SUPERNOVAE (10 years of SN1993J), Valencia, Spain.
[Madokoro:2003hh] - [22-45]
-
Topics in Core-Collapse Supernova Theory,
A. Burrows, C. D. Ott, C. Meakin,
arXiv:astro-ph/0309684,
3-D Signatures in Stellar Explosions: A Workshop honoring J. Craig Wheeler's 60th birthday, June 10-13, 2003, Austin, Texas, USA.
[Burrows:2003br] - [22-46]
-
The Status of Core-collapse Supernova Simulations,
C. Y. Cardall,
arXiv:astro-ph/0212438,
4th International Workshop on the Identification of Dark Matter (IDM2002), York, England 2-6 September 2002.
[Cardall:2002sq] - [22-47]
-
The Mechanism of Core-Collapse Supernova Explosions: A Status Report,
A. Burrows, T. A. Thompson,
arXiv:astro-ph/0210212,
ESO/MPA/MPE Workshop (an ESO Astrophysics Symposium) 'From Twilight to Highlight: The Physics of Supernovae', Garching bei Munchen, Germany, July 29-31, 2002.
[Burrows:2002bz] - [22-48]
-
The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models,
M. Liebendorfer et al.,
arXiv:astro-ph/0203260,
11th Workshop on Nuclear Astrophysics, Ringberg Caste, Lake Tegernsee, Germany, 11-16 Feb 2002.
[Liebendoerfer:2002ef] - [22-49]
-
Neutrinos from supernovae: experimental status and perspectives,
F. Cei,
A17
arXiv:hep-ex/0202043.
Second International Workshop on Matter, Anti-Matter and Dark Matter, Trento (Italy), 29-30 October 2001.
[Cei:2002mq] - [22-50]
-
Toward a Standard Model of Core Collapse Supernovae,
A. Mezzacappa,
A688
arXiv:astro-ph/0010580.
Nuclei in the Cosmos 2000, University of Aarhus, Aarhus, Denmark, June 27-July 1, 2000.
[Mezzacappa:2000jj]
- [23-1]
-
Fast neutrino flavor conversions in a supernova: emergence, evolution, and effects,
Zewei Xiong, Meng-Ru Wu, Manu George, Chun-Yu Lin, Noshad Khosravi Largani, Tobias Fischer, Gabriel Martinez-Pinedo,
arXiv:2402.19252,
[Xiong:2024tac] - [23-2]
-
Application of Neural Networks for the Reconstruction of Supernova Neutrino Energy Spectra Following Fast Neutrino Flavor Conversions,
Sajad Abbar, Meng-Ru Wu, Zewei Xiong,
109
arXiv:2401.17424.
[Abbar:2024ynh] - [23-3]
-
Machine Learning-Based Detection of Non-Axisymmetric Fast Neutrino Flavor Instabilities in Core-Collapse Supernovae,
Sajad Abbar, Akira Harada, Hiroki Nagakura,
arXiv:2401.10915,
[Abbar:2024chh] - [23-4]
-
Collisional flavor pendula and neutrino quantum thermodynamics,
Lucas Johns, Santiago Rodriguez,
arXiv:2312.10340,
[Johns:2023xae] - [23-5]
-
Collisions and collective flavor conversion: Integrating out the fast dynamics,
Damiano F. G. Fiorillo, Ian Padilla-Gay, Georg G. Raffelt,
109
arXiv:2312.07612.
[Fiorillo:2023ajs] - [23-6]
-
Fast Conversion of Neutrinos: Energy Dependence of Flavor Instabilities,
Pedro Dedin Neto, Irene Tamborra, Shashank Shalgar,
arXiv:2312.06556,
[DedinNeto:2023ykt] - [23-7]
-
Perturbing Fast Neutrino Flavor Conversion,
Marie Cornelius, Shashank Shalgar, Irene Tamborra,
02
arXiv:2312.03839.
[Cornelius:2023eop] - [23-8]
-
Physics-Informed Neural Networks for Predicting the Asymptotic Outcome of Fast Neutrino Flavor Conversions,
Sajad Abbar, Meng-Ru Wu, Zewei Xiong,
109
arXiv:2311.15656.
[Abbar:2023ltx] - [23-9]
-
Fast neutrino-flavor swap in high-energy astrophysical environments,
Masamichi Zaizen, Hiroki Nagakura,
arXiv:2311.13842,
[Zaizen:2023wht] - [23-10]
-
Collisional and Fast Neutrino Flavor Instabilities in Two-dimensional Core-collapse Supernova Simulation with Boltzmann Neutrino Transport,
Ryuichiro Akaho, Jiabao Liu, Hiroki Nagakura, Masamichi Zaizen, Shoichi Yamada,
109
arXiv:2311.11272.
[Akaho:2023brj] - [23-11]
-
Collective neutrino oscillations and heavy-element nucleosynthesis in supernovae: exploring potential effects of many-body neutrino correlations,
A. Baha Balantekin, Michael J. Cervia, Amol V. Patwardhan, Rebecca Surman, Xilu Wang,
arXiv:2311.02562,
[Balantekin:2023ayx] - [23-12]
-
Universality of the Neutrino Collisional Flavor Instability in Core Collapse Supernovae,
Jiabao Liu, Hiroki Nagakura, Ryuichiro Akaho, Akira Ito, Masamichi Zaizen, Shoichi Yamada,
108
arXiv:2310.05050.
[Liu:2023vtz] - [23-13]
-
Detecting Fast Neutrino Flavor Conversions with Machine Learning,
Sajad Abbar, Hiroki Nagakura,
109
arXiv:2310.03807.
[Abbar:2023zkm] - [23-14]
-
On the Effects of Quantum Decoherence in a Future Supernova Neutrino Detection,
Marcos V. dos Santos, Pedro C. de Holanda, Pedro Dedin Neto, Ernesto Kemp,
108
arXiv:2306.17591.
[dosSantos:2023skk] - [23-15]
-
Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions,
Jakob Ehring, Sajad Abbar, Hans-Thomas Janka, Georg Raffelt, Irene Tamborra,
131
arXiv:2305.11207.
[Ehring:2023abs] - [23-16]
-
Applications of Machine Learning to Detecting Fast Neutrino Flavor Instabilities in Core-Collapse Supernova and Neutron Star Merger Models,
Sajad Abbar,
107
arXiv:2303.05560.
[Abbar:2023kta] - [23-17]
-
Fast Neutrino Flavor Conversion in Core-Collapse Supernovae: A Parametric Study in 1D Models,
Jakob Ehring, Sajad Abbar, Hans-Thomas Janka, Georg Raffelt,
107
arXiv:2301.11938.
[Ehring:2023lcd] - [23-18]
-
Roles of fast neutrino-flavor conversion on the neutrino-heating mechanism of core-collapse supernova,
Hiroki Nagakura,
130
arXiv:2301.10785.
[Nagakura:2023mhr] - [23-19]
-
Collisional flavor instability in dense neutrino gases,
Zewei Xiong, Lucas Johns, Meng-Ru Wu, Huaiyu Duan,
108
arXiv:2212.03750.
[Xiong:2022zqz] - [23-20]
-
Simple method for determining asymptotic states of fast neutrino-flavor conversion,
Masamichi Zaizen, Hiroki Nagakura,
107
arXiv:2211.09343.
[Zaizen:2022cik] - [23-21]
-
Connecting small-scale to large-scale structures of fast neutrino-flavor conversion,
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Hydrodynamics of Supernova Evolution in the Winds of Massive Stars,
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A Broader Perspective on the GRB-SN Connection,
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General Relativity and Neutrino-driven Supernova Winds,
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Supernova 1987A: An Empirical and analytic approach,
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Probing nonlinear electrodynamics in slowly rotating spacetimes through neutrino astrophysics,
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Research of the natural neutrino fluxes by use of large volume scintillation detector at Baksan,
I. R. Barabanov, G. Ya. Novikova, V. V. Sinev, E. A. Yanovich,
arXiv:0908.1466,
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Type Ia supernova science 2010-2020,
D. A. Howell et al.,
arXiv:0903.1086,
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Detection potential for the diffuse supernova neutrino background in the large liquid-scintillator detector LENA,
M. Wurm et al.,
D75
arXiv:astro-ph/0701305.
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Probing Dark Energy via Weak Gravitational Lensing with the SuperNova Acceleration Probe (SNAP),
J. Albert et al.
(SNAP),
arXiv:astro-ph/0507460,
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Supernova Acceleration Probe: Studying Dark Energy with Type Ia Supernovae,
J. Albert et al.
(SNAP),
arXiv:astro-ph/0507459,
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Seeing the Nature of the Accelerating Physics: It's a SNAP,
J. Albert et al.
(SNAP),
arXiv:astro-ph/0507458,
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A Network of Neutral Current Spherical TPC's for Dedicated Supernova Detection,
Y. Giomataris, J.D. Vergados,
B634
arXiv:hep-ex/0503029.
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Calculations of liquid helium and neon VUV emission spectra, self-absorption and scattering for a neutrino detector,
I. M. Savukov,
arXiv:physics/0411215,
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Supernova / Acceleration Probe: A Satellite Experiment to Study the Nature of the Dark Energy,
G. Aldering et al.
(SNAP),
arXiv:astro-ph/0405232,
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Neutrino Detection With CLEAN,
D. N. McKinsey, K. J. Coakley,
22
arXiv:astro-ph/0402007.
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A design outline for a Cherenkoff neutrino observatory,
E. P. Bonvin, S. T. Hatamian,
arXiv:physics/0310160,
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GADZOOKS! Antineutrino Spectroscopy with Large Water Cerenkov Detectors,
John F. Beacom, Mark R. Vagins,
93
arXiv:hep-ph/0309300.
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Oscillation effects on supernova neutrino rates and spectra and detection of the shock breakout in a liquid argon TPC,
I. Gil-Botella, A. Rubbia,
0310
arXiv:hep-ph/0307244.
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Supernova neutrino detection in a liquid argon TPC,
A. Bueno, I. Gil-Botella, A. Rubbia,
arXiv:hep-ph/0307222,
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Megaton Modular Multi-Purpose Neutrino Detector for a Program of Physics in the Homestake DUSEL,
M. V. Diwan et al.,
arXiv:hep-ex/0306053,
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Weak Lensing from Space I: Prospects for The Supernova/Acceleration Probe,
Jason Rhodes, Alexandre Refregier, Richard Massey
(SNAP),
20
arXiv:astro-ph/0304417.
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Supernova Observation Via Neutrino-Nucleus Elastic Scattering in the CLEAN Detector,
C. J. Horowitz, K. J. Coakley, D. N. McKinsey,
D68
arXiv:astro-ph/0302071.
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Supernovae with 'Super-Hipparcos',
V. Belokurov, N.W. Evans,
341
arXiv:astro-ph/0210570.
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Study of the backgrounds for the search for proton decay to 10**35-Y at the WIPP site with the LANNDD detector,
David B. Cline, Kevin Lee, Youngho Seo, Peter F. Smith,
arXiv:astro-ph/0208381,
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Lead perchlorate as a neutrino detection medium,
M. K. Bacrania et al.,
A492
arXiv:nucl-ex/0202013.
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LANNDD: A massive liquid argon detector for proton decay, supernova and solar neutrino studies, and a neutrino factory detector,
David B. Cline, Franco Sergiampietri, John G. Learned, Kirk McDonald,
A503
arXiv:astro-ph/0105442.
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Measuring supernova neutrino temperatures using lead perchlorate,
S. R. Elliott,
C62
arXiv:astro-ph/0006041.
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A lead astronomical neutrino detector: LAND,
C. K. Hargrove, I. Batkin, M. K. Sundaresan, J. Dubeau,
5
[Hargrove:1996zv]
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Theia: A multi-purpose water-based liquid scintillator detector,
Vincent Fischer
(Theia),
arXiv:1809.05987,
CIPANP2018.
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Supernova Burst Observations with DUNE,
Jost Migenda
(DUNE),
arXiv:1804.01877,
NuPhys2017 (London, 20-22 December 2017).
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Supernova Neutrino Detection in LZ,
Dev Ashish Khaitan
(LZ),
13
arXiv:1801.05651.
LIDINE 2017.
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Astroparticle Physics in Hyper-Kamiokande,
Jost Migenda,
EPS-HEP2017
arXiv:1710.08345.
EPS-HEP2017.
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Observing the Next Galactic Supernova with the NOvA Detectors,
Justin A. Vasel, Andrey Sheshukov, Alec Habig
(the NOvA),
arXiv:1710.00705,
APS Division of Particles and Fields Meeting (DPF 2017), July 31-August 4, 2017, Fermilab.
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Simulating fast time variations in the supernova neutrino flux in Hyper-Kamiokande,
Jost Migenda
(Hyper-Kamiokande),
888
arXiv:1610.00559.
Neutrino 2016.
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Underground physics with DUNE,
Vitaly A. Kudryavtsev
(DUNE),
718
arXiv:1601.03496.
TAUP2015.
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Prospects of the search for neutrino bursts from Supernovae with Baksan Large Volume Scintillation Detector,
V.B. Petkov,
47
arXiv:1508.01389.
International Workshop on Prospects of Particle Physics: 'Neutrino Physics and Astrophysics', Valday, Russia, January 1 - February 8, 2015. Accepted for publication in Physics of Elementary Particles and Atomic Nuclei.
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Physics Potential of an Advanced Scintillation Detector: Introducing THEIA,
Gabriel D. Orebi Gann, THEIA Interest Group
(Group for the THEIA Interest),
arXiv:1504.08284,
Prospects in Neutrino Physics Conference, 15 - 17 December, 2014, held at Queen Mary University of London, UK.
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TITUS: An Intermediate Distance Detector for the Hyper-Kamiokande Neutrino Beam,
Pierre Lasorak, Nick Prouse
(TIITUS Working Group),
arXiv:1504.08272,
Prospects in Neutrino Physics Conference, 15 - 17 December, 2014, held at Queen Mary University of London, UK.
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The Physics Potential of the LENA Detector,
Michael Wurm et al.,
B41
arXiv:1004.3474.
Cracow Epiphany Conference, 5-8 January 2010.
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The LAGUNA design study- towards giant liquid based underground detectors for neutrino physics and astrophysics and proton decay searches,
D. Angus et al.
(LAGUNA),
arXiv:1001.0077,
Workshop 'European Strategy for Future Neutrino Physics', CERN, Oct. 2009.
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Giant Liquid Argon Observatory for Proton Decay, Neutrino Astrophysics and CP-violation in the Lepton Sector (GLACIER),
A. Badertscher et al.,
arXiv:1001.0076,
Workshop 'European Strategy for Future Neutrino Physics', CERN, Oct. 2009.
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Gadolinium study for a water Cherenkov detector,
Atsuko Kibayashi
(Super-Kamiokande),
arXiv:0909.5528,
DPF-2009, Detroit, MI, July 2009.
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Underground Neutrino Detectors for Particle and Astroparticle Science: the Giant Liquid Argon Charge Imaging ExpeRiment (GLACIER),
A. Rubbia,
171
arXiv:0908.1286.
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The SNO+ Experiment,
Mark C. Chen, SNO+
(SNO+),
arXiv:0810.3694,
ICHEP08.
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Review of Low Energy Neutrinos,
J.D. Vergados,
65
arXiv:hep-ph/0702142.
Third Symposium on Large TPC's for Low Energy Rare Event Detection, Paris, Dec. 11-12, 2006 and NUMMY07 ENTApP Network Meeting, Durham, Jan. 10-12, 2007.
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Low energy neutrino astronomy with the large liquid scintillation detector LENA,
T. Marrodan Undagoitia et al.,
57
arXiv:hep-ph/0605229.
International School of Nuclear Physics, Neutrinos in Cosmology, in Astro, Particle and Nuclear Physics, Erice (SICILY) 16 - 24 Sept. 2005.
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Supernova Detection via a Network of Neutral Current Spherical TPC's,
J.D. Vergados, Y. Giomataris,
847
arXiv:hep-ph/0601093.
International Symposium on Origin of Matter and Evolution of Galaxies (OMEG05)- New Horizon of Nuclear Astrophysics and Cosmology November 8-11, 2005, University of Tokyo, Tokyo, Japan.
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Dedicated Supernova Detection by a Network of Neutral Current Spherical TPC's,
J.D. Vergados, Y. Giomataris,
70
arXiv:astro-ph/0511470.
NANP05, Dubna, Russia.
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Supernova Legacy Survey (SNLS) : real time operations and photometric analysis,
N. Palanque-Delabrouille, SNLS
(SNLS),
arXiv:astro-ph/0509425,
SF2A workshop, Strasbourg, June 27 - July 1 2005.
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Exploring Dark Energy with SNAP,
G. Aldering,
49
arXiv:astro-ph/0507426.
Wide-Field Imaging from Space.
[Aldering:2005qn] - [43-23]
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UNO,
R. Jeffrey Wilkes,
arXiv:hep-ex/0507097,
XI International Workshop on 'Neutrino Telescopes', Feb 22-25, 2005, Venice, Italy.
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-
The SNAP Strong Lens Survey,
Phil Marshall, Roger Blandford, Masao Sako,
49
arXiv:astro-ph/0501328.
Wide Field Imaging from Space.
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-
The Carnegie Supernova Project,
Wendy L. Freedman, Carnegie Supernova Project
(The Carnegie Supernova Project),
339
arXiv:astro-ph/0411176.
NOAO Workshop, Tucson, March, 2004, 'Observing Dark Energy'.
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SNLS: Overview and High-z Spectroscopy,
D. Andrew Howell et al.
(SNLS),
arXiv:astro-ph/0410595,
'1604-2004: Supernovae as Cosmological Lighthouses', Padua, June 16-19 2004.
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The Supernova Legacy Survey,
Mark Sullivan et al.
(SNLS),
342
arXiv:astro-ph/0410594.
'1604-2004: Supernovae as Cosmological Lighthouses', Padua, June 16-19 2004.
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The Caltech Core-Collapse Project (CCCP),
A. Gal-Yam et al.,
342
arXiv:astro-ph/0410038.
'Supernovae as Cosmological Lighthouses', Padua, 2004.
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Probing Dark Energy with SNAP,
Eric V. Linder,
arXiv:astro-ph/0210217,
4th International Workshop on the Identification of Dark Matter (IDM2002), St. William's College, York Minster, York, England, September 2-6, 2002.
http://www.shef.ac.uk/~phys/idm2002/talks/pdfs/linder.pdf.
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Wide-Field Surveys from the SNAP Mission,
A. Kim
(SNAP),
arXiv:astro-ph/0210077.
SPIE Proceedings Vol. 4836.
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Overview of the SuperNova/Acceleration Probe (SNAP),
Greg Aldering
(SNAP),
4835
arXiv:astro-ph/0209550.
SPIE Proceedings Vol. 4835.
[SNAP:2002blf] - [43-32]
-
The SNAP Telescope,
M.Lampton
(SNAP),
arXiv:astro-ph/0209549,
SPIE Proceedings Vol. 4849.
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-
UNO: Underground Nucleon Decay and Neutrino Observatory,
C. McGrew,
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/McGrew_C/mcgrew_thurs_protondecaywg.pdf.
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Future Supernova Neutrino Detector,
K. Scholberg,
International Workshop on Neutrinos andSubterranean Science - NeSS 02, Washington, DC, September 19-21, 2002.
http://mocha.phys.washington.edu/~int_talk/WorkShops/Neutrino02/Working_Groups/People/Scholberg_K/scholberg_thurs_solarstellarwg.pdf.
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Feasibility of a next generation underground water Cherenkov detector: UNO,
Chang Kee Jung,
533
arXiv:hep-ex/0005046.
International Workshop on Next Generation Nucleon Decay and Neutrino Detector (NNN 99), Stony Brook, New York, 23-25 Sep 1999.
[Jung:1999jq]
Supernova Neutrino Database, - SUNG, SUpernova Neutrino Generation tool by Jorge Zuluaga
- The Asiago Supernova Catalogue
- International Supernovae Network
- Supernova Taxonomy by Marcos J. Montes
- Supernova Taxonomy by Michael Richmond
- SNEWS: SuperNova Early Warning System
- J. Font, Numerical Hydrodynamics in General Relativity Living Rev. Relativity 3 (2000) 2
- Supernova and Supernova Remnant Pages on the WWW
- X-Ray Astronomy Field Guide: Supernovae and Supernova Remnants
- MPA Hydro Gang
- Supernova Science Center - LANL
- APS Neutrino Study
- Adam Burrows Home Page
- OAT-INAF Supernovae Home Page
