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SN Ib 1990I: Clumping and Dust in the Ejecta?,
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Astron. Astrophys. 426 (2004) 963-977,arXiv:astro-ph/0407145.
[Elmhamdi:2004he]
The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope,
Nikolai N. Chugai et al.,
Mon. Not. Roy. Astron. Soc. 352 (2004) 1213,arXiv:astro-ph/0405369.
[Chugai:2004gq]
XMM-Newton observation of Kepler's supernova remnant,
G. Cassam-Chenai et al.,
Astron.Astrophys. (2003),arXiv:astro-ph/0310687.
[Cassam-Chenai:2003lgh]
Twenty Years of Galactic Observations in Searching for Bursts of Collapse Neutrinos with the Baksan Underground Scintillation Telescope,
E.N.Alexeyev, L.N.Alexeyeva,
J. Exp. Theor. Phys. 95 (2002) 5,arXiv:astro-ph/0212499.
[Alekseev:2002ji]
Search for supernova relic neutrinos at Super-Kamiokande,
M. Malek et al.(Super-Kamiokande),
Phys. Rev. Lett. 90 (2003) 061101,arXiv:hep-ex/0209028.
[Super-Kamiokande:2002hei]
The Asiago Supernova Catalogue - 10 years after,
R. Barbon, V. Buondi, E. Cappellaro, M. Turatto,
Astron. Astrophys. 139 (1999) 531-536. [Asiago-Supernova-Catalogue-AA139-1999]
Eleven Year Search for Supernovae with the IceCube Neutrino Observatory,
Robert Cross, Alexander Fritz, Spencer Griswold(IceCube),
PoS ICRC2019 (2020) 889,arXiv:1908.07249.
36th International Cosmic Ray Conference (ICRC 2019), Madison, WI, U.S.A. [Cross:2019jpb]
Improved Detection of Supernovae with the IceCube Observatory,
Lutz Kopke(IceCube),
J.Phys.Conf.Ser. 1029 (2018) 012001,arXiv:1704.03823.
8th international symposium on large TPCs for low-energy rare event detection, Paris, Dec. 5-7, 2016. [Kopke:2017req]
The core collapse supernova rate from 24 years of data of the Large Volume Detector,
G. Bruno, A. Molinario, W. Fulgione, C. Vigorito(LVD),
J.Phys.Conf.Ser. 888 (2017) 012256,arXiv:1701.06765.
XXV ECRS 2016. [Bruno:2017oxg]
The IceCube Neutrino Observatory Part V: Neutrino Oscillations and Supernova Searches,
M. G. Aartsen et al.(IceCube),
arXiv:1309.7008, 2013.33nd International Cosmic Ray Conference, Rio de Janeiro 2013. [IceCube:2013lje]
Supernova Detection in IceCube: Status and Future,
Ronald Bruijn(IceCube),
Nucl. Phys.B, Proc.Suppl.237-238 2013 (2013) 94-97,arXiv:1302.2040.
NOW 2012. [Bruijn:2013ibl]
The IceCube Neutrino Observatory VI: Neutrino Oscillations, Supernova Searches, Ice Properties,
R. Abbasi et al.(IceCube),
arXiv:1111.2731, 2011.32nd International Cosmic Ray Conference, Beijing 2011. [IceCube:2011vzz]
Search for neutrino bursts from core collapse supernovae at the Baksan Underground Scintillation Telescope,
R.V. Novoseltseva et al.,
arXiv:0910.0738, 2009.31 International Cosmic Ray Conference, Lodz, Poland, July 7-15, 2009. [Novoseltseva:2009cr]
Supernova Search with the AMANDA / IceCube Detectors,
Thomas Kowarik, Timo Griesel, Alexander Piegsa(Icecube),
arXiv:0908.0441, 2009.31st ICRC, Lodz, Poland, July 2009. [Kowarik:2009qr]
Search for High Energetic Neutrinos from Supernova Explosions with AMANDA,
Dirk Lennarz, Jan-Patrick Huls, Christopher Wiebusch(IceCube),
arXiv:0907.4621, 2009.31st ICRC, Lodz, Poland, July 2009. [Lennarz:2009xr]
Recent Type II Radio Supernovae,
Christopher J. Stockdale et al.,
AIP Conf. Proc. 937 (2007) 264-268,arXiv:0708.1182.
Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters. [Stockdale:2007pe]
LVD highlights,
Marco Selvi et al.(LVD),
arXiv:hep-ex/0608061, 2006.Vulcano Workshop 2006 'Frontier Objects in Astrophysics and Particle Physics'. [Selvi:2006bi]
SNLS - the Supernova Legacy Survey,
C.J. Pritchet, SNLS(SNLS),
ASP Conf.Ser. (2004),arXiv:astro-ph/0406242.
Observing Dark Energy (NOAO/Tucson proceedings). [Pritchet:2004af]
Evidence for Core Collapse in the Type Ib/c SN 1999ex,
Mario Hamuy et al.,
arXiv:astro-ph/0212368, 2002.From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia. [Hamuy:2002rz]
The dusty type IIn Supernova 1998S,
Peter Meikle et al.,
arXiv:astro-ph/0211144, 2002.ESO/MPA/MPE Workshop 'From Twilight to Highlight: The Physics of Supernovae', Garching, Germany, 29-31 July 2002. [Meikle:2002dn]
A Search for Core-Collapse Supernova Progenitors In Hubble Space Telescope Images,
Schuyler D. Van Dyk, Weidong Li, Alexei V. Filippenko,
Publ.Astron.Soc.Pac. (2002),arXiv:astro-ph/0210347.
PASP (2003 Jan). [VanDyk:2002ry]
An Intermediate Redshift Supernova Search at ESO: Reduction Tools and Efficiency Tests,
M. Riello et al.,
arXiv:astro-ph/0210265, 2002.ESO/MPA/MPE Workshop 'From Twilight to Highlight, The Physics of Supernovae', Garching, Jul 29-31, 2002. [Riello:2002hm]
Search for double degenerate progenitors of supernovae type Ia with SPY,
R. Napiwotzki, H. Drechsel, U. Heber, C. Karl, E.-M. Pauli et al., others, others, others, others, others, others, others, others, others, others,
arXiv:astro-ph/0210155, 2002.'White Dwarfs', Proc. XIII Workshop on White Dwarfs. [Napiwotzki:2002sa]
Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey,
A. Rest et al.,
Astrophys.J. 795 (2014) 44,arXiv:1310.3828.
[Rest:2013mwz]
Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample,
D. Scolnic et al.,
Astrophys.J. 795 (2014) 45,arXiv:1310.3824.
[Scolnic:2013efb]
The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae,
Gaston Folatelli et al.,
Astron. J. 139 (2010) 120-144,arXiv:0910.3317.
[Folatelli:2009nm]
Asymmetric Explosion of Type Ia Supernovae as Seen from Near Infrared Observations,
K. Motohara et al.,
Astrophys. J. 652 (2006) L101-L104,arXiv:astro-ph/0610303.
[Motohara:2006tg]
The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey,
A. Conley et al.(SNLS),
Astron. J. 132 (2006) 1707-1713,arXiv:astro-ph/0607363.
[SNLS:2006vah]
Nonlinear Decline-Rate Dependence and Intrinsic Variation of Type Ia Supernova Luminosities,
Lifan Wang et al.,
Astrophys. J. 641 (2006) 50-69,arXiv:astro-ph/0512370.
[Wang:2005bw]
The Supernova Legacy Survey: Measurement of $\Omega_\text{M}$, $\Omega_{\Lambda}$ and $w$ from the First Year Data Set,
P. Astier et al.(SNLS),
Astron. Astrophys. 447 (2006) 31,arXiv:astro-ph/0510447. From the abstract:With this data set, we have built a Hubble diagram extending to $z=1$, with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: $ \Omega_{\text{M}} = 0.263 \pm 0.042 \pm 0.032 $ for a flat $\Lambda\text{CDM}$; and $w = -1.023 \pm 0.090 \pm 0.054 $ for a flat cosmology with constant equation of state $w$ when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations. [SNLS:2005qlf]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications,
A. Clocchiatti et al.(High Z SN Search),
Astrophys. J. 642 (2006) 1-21,arXiv:astro-ph/0510155.
[HighZSNSearch:2005xhg]
Spectroscopy of twelve Type Ia supernovae at intermediate redshift,
C. Balland et al.,
Astron.Astrophys. (2005),arXiv:astro-ph/0507703.
[Balland:2005rw]
First results from the Canada-France High-z Quasar Survey: Constraints on the z=6 quasar luminosity function and the quasar contribution to reionization,
Chris J. Willott et al.,
Astrophys. J. 633 (2005) 630,arXiv:astro-ph/0507183.
[Willott:2005zr]
Evidence for Spectropolarimetric Diversity in Type Ia Supernovae,
Douglas C. Leonard et al.,
Astrophys. J. 632 (2005) 450,arXiv:astro-ph/0506470.
[Leonard:2005td]
A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex,
R. J. Foley et al.,
Astrophys. J. 626 (2005) L11,arXiv:astro-ph/0504481.
[Foley:2005qu]
Restframe I-band Hubble diagram for type Ia supernovae up to redshift $z \sim 0.5$,
Serena Nobili et al.(Supernova Cosmology Project),
Astron.Astrophys. (2005),arXiv:astro-ph/0504139.
[SupernovaCosmologyProject:2005zcy]
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant,
Adam G. Riess et al.,
Astrophys. J. 627 (2005) 579,arXiv:astro-ph/0503159. From the abstract:$H_0 = 73 +\pm 4 \pm 5 \, \text{km} \, \text{s}^{-1} \, \text{Mps}^{-1}$. [Riess:2005zi]
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey,
Louis-Gregory Strolger, Adam G. Riess,
Astron. J. 131 (2006) 1629-1638,arXiv:astro-ph/0503093.
[Strolger:2005uk]
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT,
C. Lidman et al.(Supernova Cosmology Project),
Astron.Astrophys. (2004),arXiv:astro-ph/0410506.
[SupernovaCosmologyProject:2004akn]
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models,
L. G. Strolger et al.,
Astrophys. J. 613 (2004) 200-223,arXiv:astro-ph/0406546.
[Strolger:2004kk]
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa,
Gabriele Garavini et al.(The Supernova Cosmology Project),
Mon. Not. Roy. Astron. Soc. 356 (2004) 456,arXiv:astro-ph/0404393.
[SupernovaCosmologyProject:2004yms]
Type Ia Supernova Discoveries at z > 1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution,
Adam G. Riess et al.(Supernova Search Team),
Astrophys. J. 607 (2004) 665,arXiv:astro-ph/0402512. From the abstract:We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration. ... A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99\% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at $z=0.46 \pm 0.13$. The data are consistent with the cosmic concordance model of $\Omega_M \approx 0.3, \Omega_\Lambda \approx 0.7$ ($\chi^2_{dof}=1.06$), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy. For a flat Universe with a cosmological constant, we measure $\Omega_M = 0.29 {}^{+0.05}_{-0.03}$ (equivalently, $\Omega_\Lambda=0.71$). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find $w = -1.02 {}^{+0.13}_{-0.19}$ (and $w<-0.76$ at the 95\% confidence level) for an assumed static equation of state of dark energy, $P = w\rho c^2$. ... Our constraints are consistent with the static nature of and value of $w$ expected for a cosmological constant (i.e., $w_0 = -1.0$, $dw/dz = 0$), and are inconsistent with very rapid evolution of dark energy. [Ivanov:2004qa]
23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at $z > 0.7$,
Brian J. Barris et al.,
Astrophys. J. 602 (2004) 571,arXiv:astro-ph/0310843. From the abstract:This sample of 23 high-redshift supernovae includes 15 at $z\geq0.7$, doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry and others (2003), we calculate cosmological parameter density contours which are consistent with the flat universe indicated by the CMB [Go]. Adopting the constraint that $\Omega_{total} = 1.0$, we obtain best-fit values of ($\Omega_{m}$,$\Omega_{\Lambda}$)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation. [Barris:2003dq]
New Constraints on $\Omega_M$, $\Omega_\Lambda$, and $w$ from an Independent Set of Eleven High-Redshift Supernovae Observed with HST,
Robert A. Knop et al.(The Supernova Cosmology Project),
Astrophys. J. 598 (2003) 102,arXiv:astro-ph/0309368. From the abstract:We report measurements of $\Omega_{\mathrm{M}}$, $\Omega_{\Lambda}$, and $w$ from eleven supernovae at $z=0.36$-$0.86$ with high-quality lightcurves measured using WFPC2 on the HST. This is an independent set of high-redshift supernovae that confirms previous supernova evidence for an accelerating Universe. The high-quality lightcurves available from photometry on \wfpc\ make it possible for these eleven supernovae alone to provide measurements of the cosmological parameters comparable in statistical weight to the previous results. Combined with earlier Supernova Cosmology Project data, the new supernovae yield a measurement of the mass density $\Omega_{\mathrm{M}}=0.25^{+0.07}_{-0.06}$ (statistical) $\pm0.04$ (identified systematics), or equivalently, a cosmological constant of $\Omega_{\Lambda}=0.75^{+0.06}_{-0.07}$ (statistical) $\pm0.04$ (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value $w=-1$. When the supernova results are combined with independent flat-universe measurements of $\Omega_{\mathrm{M}}$ from CMB and galaxy redshift distortion data, they provide a measurement of $w=-1.05^{+0.15}_{-0.20}$ (statistical) $\pm0.09$ (identified systematic), if $w$ is assumed to be constant in time.... dark energy is required with $P(\Omega_{\Lambda}>0)>0.99$. [SupernovaCosmologyProject:2003dcn]
Cosmological Results from High-z Supernovae,
John L. Tonry et al.(Supernova Search Team),
Astrophys. J. 594 (2003) 1,arXiv:astro-ph/0305008. From the abstract:The High-$ z$ Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval $ z=0.3-1.2$. These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to $ z\approx 1$, where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is $ w=-1$, then $ H_0\,t_0 = 0.96\pm0.04$, and $ \Omega_\Lambda-1.4\Omega_M=0.35\pm0.14$. Including the constraint of a flat Universe, we find $ \Omega_M=0.28\pm0.05$, independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on $ \Omega_M$ and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range $ -1.48-1$, we obtain $ w<-0.73$ at 95% confidence. [SupernovaSearchTeam:2003cyd]
SN 2002cx: The Most Peculiar Known Type Ia Supernova,
Weidong Li et al.,
Publ. Astron. Soc. Pac. 115 (2003) 453-473,arXiv:astro-ph/0301428.
[Li:2003wja]
Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el,
Kevin Krisciunas et al.,
Astron. J. 125 (2003) 166,arXiv:astro-ph/0210327.
[Krisciunas:2002rc]
The distant Type Ia supernova rate,
R. Pain et al.(Supernova Cosmology Project),
Astrophys. J. 577 (2002) 120,arXiv:astro-ph/0205476.
[SupernovaCosmologyProject:2002nuh]
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration,
Adam G. Riess et al.(Supernova Search Team),
Astrophys. J. 560 (2001) 49-71,arXiv:astro-ph/0104455.
[SupernovaSearchTeam:2001qse]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae,
S. Perlmutter et al.(Supernova Cosmology Project),
Astrophys. J. 517 (1999) 565-586,arXiv:astro-ph/9812133. From the abstract:The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation $0.8 \,\Omega_{\rm M}- 0.6\,\Omega_\Lambda \approx -0.2 \pm 0.1$ in the region of interest ($\Omega_{\rm M} \lesssim 1.5$). For a flat ($\Omega_{\rm M}+\Omega_\Lambda = 1$) cosmology we find $\Omega_{\rm M}^{\rm flat} = 0.28^{+0.09}_{-0.08}$ (1$\sigma$ statistical) $^{+0.05}_{-0.04}$ (identified systematics). The data are strongly inconsistent with a $\Lambda = 0$ flat cosmology, the simplest inflationary universe model. An open, $\Lambda = 0$ cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of $P(\Lambda > 0) = 99$\%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is $t_0^{\rm flat}=14.9^{+1.4}_{-1.1}\,(0.63/h)$ Gyr for a flat cosmology. [SupernovaCosmologyProject:1998vns]
Supernova Limits on the Cosmic Equation of State,
Peter M. Garnavich et al.(Supernova Search Team),
Astrophys. J. 509 (1998) 74-79,arXiv:astro-ph/9806396.
[SupernovaSearchTeam:1998cav]
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,
Adam G. Riess et al.(Supernova Search Team),
Astron. J. 116 (1998) 1009-1038,arXiv:astro-ph/9805201.
[SupernovaSearchTeam:1998fmf]
Exploring the Physics of Type Ia Supernovae Through the X-ray Spectra of their Remnants,
C. Badenes et al.,
Mem.Soc.Ast.It. (2005),arXiv:astro-ph/0506576.
"Stellar end products" workshop, 13-15 April 2005, Granada, Spain. [Badenes:2005kx]
A 'Missing' Supernova Remnant revealed by the 21-cm Line of Atomic Hydrogen,
B-C Koo, J-h Kang, C.J. Salter,
Astrophys. J. 643 (2006) L49-L52,arXiv:astro-ph/0604186.
[Koo:2006sr]
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,
Astrophys.J. 873 (2019) 15,arXiv:1901.11235.
[Larsson:2019uwm]
Time evolution of the line emission from the inner circumstellar ring of SN 1987A and its hot spots,
Per Groeningsson et al.,
Astron.Astrophys. 492 (2008) 481,arXiv:0810.2661.
[Groeningsson:2008nc]
Chandra HETG Spectra of SN 1987A at 20 years,
D. Dewey, S. A. Zhekov, R. McCray, C. R. Canizares,
Astrophys.J. 676 (2008) L131,arXiv:0802.2340.
[Dewey:2008gy]
Discovery of a nearby twin of SN1987A's nebula around the luminous blue variable HD168625: Was Sk-69 202 an LBV?,
Nathan Smith,
Astron. J. 133 (2007) 1034-1040,arXiv:astro-ph/0611544.
[Smith:2006es]
On the Progenitor of Supernova 1987A,
M. Parthasarathy, David Branch, E. Baron, David J. Jeffery,
Bull.Astron.Soc.India (2006),arXiv:astro-ph/0611033.
[Parthasarathy:2006jr]
Evolutionary Status of SNR 1987A at the Age of Eighteen,
Sangwook Park et al.,
Astrophys. J. 646 (2006) 1001-1008,arXiv:astro-ph/0604201.
[Park:2006tg]
Coronal emission from the shocked circumstellar ring of SN 1987A,
Per Groningsson et al.,
Astron.Astrophys. (2006),arXiv:astro-ph/0603815.
[Groningsson:2006cb]
SN 1987A After 18 Years: Mid-Infrared GEMINI and SPITZER Observations of the Remnant,
Patrice Bouchet et al.,
Astrophys. J. 650 (2006) 212-227,arXiv:astro-ph/0601495.
[Bouchet:2006ff]
Supernova Remnant 1987A: Opening the Future by Reaching the Past,
Sangwook Park, Svetozar A. Zhekov, David N. Burrows, Richard McCray,
Astrophys. J. 634 (2005) L73,arXiv:astro-ph/0510442.
[Park:2005qj]
Imaging of the Radio Remnant of SN 1987A at 12 mm Wavelength,
R. N. Manchester et al.,
Astrophys. J. 628 (2005) L131,arXiv:astro-ph/0506475.
[Manchester:2005ti]
Chandra Observations of Shock Kinematics in Supernova Remnant 1987A,
S.A. Zhekov et al.,
Astrophys. J. 628 (2005) L127,arXiv:astro-ph/0506443.
[Zhekov:2005ni]
Limits from the Hubble Space Telescope on a Point Source in SN 1987A,
G. J. M. Graves et al.,
Astrophys. J. 629 (2005) 944,arXiv:astro-ph/0505066.
[Graves:2005xy]
A New View of the Circumstellar Environment of SN 1987A,
Ben E. K. Sugerman et al.,
Astrophys. J. 627 (2005) 888,arXiv:astro-ph/0502268.
[Sugerman:2005dk]
Supernova Remnant 1987A: The Latest Report from the Chandra X-Ray Observatory,
Sangwook Park et al.,
Adv. Space Res. 35 (2005) 991-995,arXiv:astro-ph/0501561.
[Park:2005ic]
Constraints on the luminosity of the stellar remnant in SNR1987A,
P. Shtykovskiy, A. Lutovinov, M. Gilfanov, R. Sunyaev,
Astron. Lett. 31 (2005) 258,arXiv:astro-ph/0411731.
[Shtykovskiy:2004uj]
Young Stellar Populations Around SN1987A,
Nino Panagia, Martino Romaniello, Salvatore Scuderi, Robert P. Kirshner,
Astrophys. J. 539 (2000) 197-208,arXiv:astro-ph/0001476.
[Panagia:2000ga]
A Second Bright Source Detected Near SN1987A,
Peter Nisenson, Costas Papaliolios,
Astrophys.J. 518 (1999) L29,arXiv:astro-ph/9904109.
[Nisenson:1999qd]
The X-ray lightcurve of SN 1987A,
G. Hasinger, B. Aschenbach, J. Trumper,
Astron. Astrophys. 312 (1996) L9-L12,arXiv:astro-ph/9606149.
[Hasinger:1996rj]
Ultraviolet observations of SN 1987A,
Robert P. Kirshner, George Sonneborn, D. Michael Crenshaw, George E. Nassiopoulos,
Astrophys. J. 320 (1987) 602-608. [Kirshner-ApJ320-1987]
The progenitor of SN 1987A - Spatially resolved ultraviolet spectroscopy of the supernova field,
George Sonneborn, Bruce Altner, Robert P. Kirshner,
Astrophys. J. 323 (1987) L35-L39. [Kirshner-ApJ323-1987]
11 - Experiment - Type II - SN1987A - Conference Proceedings
SN1987A: Revisiting the Data and the Correlation between Neutrino and Gravitational Detectors,
P. Galeotti, G. V. Pallottino, G. Pizzella,
Italian Phys.Soc.Proc. 98 (2009) 233-242,arXiv:0810.3759.
Vulcano Wokshop 2008, Frontier Objects in Astrophysics and Particle Physics, May 26-31. [Galeotti:2008wc]
Chandra Observations of Supernova 1987A,
Sangwook Park et al.,
AIP Conf. Proc. 937 (2007) 43-50,arXiv:0704.0209.
Supernova 1987A: 20 Years after Supernovae and Gamma-Ray Bursters, Aspen, CO, USA, Feb 19-23, 2007. [Park:2007nr]
Supernova Remnant 1987A: High Resolution Images and Spectrum from Chandra Observations,
Sangwook Park et al.,
ESA Spec.Publ. 604 (2006) 335,arXiv:astro-ph/0511355.
The X-Ray Universe 2005, Sept 26-30, 2005, El Escorial, Madrid, Spain. [Park:2005vu]
A 2.14 ms Candidate Optical Pulsar in SN1987A,
J. Middleditch et al.,
arXiv:astro-ph/0010044, 2000.5th CTIO/ESO Workshop and 1st CTIO/ESO/LCO Workshop: SN 1987A: Ten Years After, La Serena, Chile, 22-28 Feb 1997. [Middleditch:2000it]
DETECTION OF THE NEUTRINO SIGNAL FROM SN1987A IN THE LMC USING THE INR BAKSAN UNDERGROUND SCINTILLATION TELESCOPE,
E. N. Alekseev, L. N. Alekseeva, I. V. Krivosheina, V. I. Volchenko,
Phys. Lett. B205 (1988) 209-214. [Alekseev:1988gp]
POSSIBLE DETECTION OF A NEUTRINO SIGNAL ON 23 FEBRUARY 1987 AT THE BAKSAN UNDERGROUND SCINTILLATION TELESCOPE OF THE INSTITUTE OF NUCLEAR RESEARCH,
E. N. Alekseev, L. N. Alekseeva, V. I. Volchenko, I. V. Krivosheina,
JETP Lett. 45 (1987) 589-592.[Pisma Zh. Eksp. Teor. Fiz. 45, 461-464 (1987)]. [Alekseev:1987ej]
CHARACTERISTICS OF THE NEUTRINO EMISSION FROM SUPERNOVA SN1987A,
A. E. Chudakov, Ya. S. Elensky, S. P. Mikheev,
JETP Lett. 46 (1987) 373-377.[Pisma Zh. Eksp. Teor. Fiz. 46, 297 (1987)]. [Chudakov:1987my]
OBSERVATION OF A NEUTRINO BURST IN COINCIDENCE WITH SUPERNOVA SN1987A IN THE LARGE MAGELLANIC CLOUD,
R. M. Bionta et al.(IMB),
Phys. Rev. Lett. 58 (1987) 1494. [Bionta:1987qt]
Observation in the Kamiokande-II detector of the neutrino burst from supernova SN1987A,
K. S. Hirata et al.(Kamiokande),
Phys. Rev. D38 (1988) 448-458. [Hirata:1988ad]
Observation of a neutrino burst from the supernova SN1987a,
K. Hirata et al.(Kamiokande),
Phys. Rev. Lett. 58 (1987) 1490-1493. [Kamiokande-II:1987idp]
A search for high-energy neutrinos from SN1987a: first six months,
Y. Oyama et al.(Kamiokande),
Phys. Rev. Lett. 59 (1987) 2604. [Kamiokande-II:1987ive]
Correlations between low-energy and high-energy pulses detected by the LSD installation under Mt. Blanc from 10 February 1987 to 1 July 1987,
V. L. Dadykin et al.,
JETP Lett. 56 (1992) 426-429. [Dadykin:1992yi]
Coincidences among the data recorded by the Baksan, Kamioka and Mont Blanc underground neutrino detectors, and by the Maryland and Rome gravitational wave detectors during supernova SN1987A,
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Phys. Rev. D81 (2010) 083001,arXiv:1001.3678.
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JINST 4 (2009) P01002,arXiv:0812.2713.
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Astrophys.J. 689 (2008) 371,arXiv:0809.0526.
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JCAP 0808 (2008) 033,arXiv:0805.4225.
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Phys. Atom. Nucl. 71 (2008) 2165-2168,arXiv:0804.1916.
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Parameter Degeneracy in Flavor-Dependent Reconstruction of Supernova Neutrino Fluxes,
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JCAP 0812 (2008) 006,arXiv:0802.1489.
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The primary cosmic ray spectrum in supernova remnants from very high energy gamma-ray data,
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Phys. Rev. D76 (2007) 125019,arXiv:0707.0471.
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In which shell-type SNRs should we look for gamma-rays and neutrinos from p-p collisions?,
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JCAP 0801 (2008) 018,arXiv:0706.3485.
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Impact of the Neutrino Magnetic Moment on Supernova r-process Nucleosynthesis,
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JCAP 0709 (2007) 016,arXiv:0706.3023.
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Probing non-standard neutrino interactions with supernova neutrinos,
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A Probabilistic Approach to Classifying Supernovae Using Photometric Information,
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Neutrinos from supernova remnants after the first HESS observations,
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Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field,
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Astrophys. J. 648 (2006) L29-L32,arXiv:astro-ph/0607344.
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Probing Dark Energy via Neutrino and Supernova Observatories,
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Supernova Neutrinos: The Accretion Disk Scenario,
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Reconstructing supernova-neutrino spectra using low-energy beta-beams,
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Astropart. Phys. 25 (2006) 328-341,arXiv:astro-ph/0603599.
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Towards a Cosmological Hubble Diagram for Type II-P Supernovae,
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Astrophys. J. 645 (2006) 841-850,arXiv:astro-ph/0603535.
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TeV Gamma-Rays from Old Supernova Remnants,
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Study of core collapse neutrino signals and constraints on neutrino masses from a future Galactic Supernova,
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Direct measurement of supernova neutrino emission parameters with a gadolinium enhanced Super-Kamiokande detector,
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New Test of Supernova Electron Neutrino Emission using Sudbury Neutrino Observatory Sensitivity to the Diffuse Supernova Neutrino Background,
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New Estimates of the Solar-Neighborhood Massive-Stars Birthrate and the Galactic Supernova Rate,
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Astronomical J. 130 (2005) 1652-1657,arXiv:astro-ph/0506708.
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The supernova rate-velocity dispersion relation in the interstellar medium,
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Rates of Neutrino Absorption on Nucleons and the Reverse Processes in Strong Magnetic Fields,
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Mini Z' Burst from Relic Supernova Neutrinos and Late Neutrino Masses,
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Constraining the Spectrum of Supernova Neutrinos from Neutrino-Process-Induced Light-Element Synthesis,
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The Concordance Cosmic Star Formation Rate: Implications from and for the Supernova Neutrino and Gamma Ray Backgrounds,
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JCAP 0504 (2005) 017,arXiv:astro-ph/0502150.
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The Neutrino Bubble Instability: A Mechanism for Generating Pulsar Kicks,
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Nucleosynthesis in the Hot Convective Bubble in Core-Collapse Supernovae,
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The Progenitors of Core-Collapse Supernovae,
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Redshift Accuracy Requirements for Future Supernova and Number Count Surveys,
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Astrophys. J. 615 (2004) 595,arXiv:astro-ph/0402002.
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The Supernova Relic Neutrino Backgrounds at KamLAND and Super-Kamiokande,
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JCAP 0403 (2004) 007,arXiv:astro-ph/0312346.
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Gravitational Waves from a Pulsar Kick Caused by Neutrino Conversions,
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Supernova Neutrinos, Neutrino Oscillations, and the Mass of the Progenitor Star,
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On the relative frequencies of core-collapse supernovae sub-types: the role of progenitor metallicity,
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The First Supernova Explosions in the Universe,
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Supernovae and Light Neutralinos: SN1987A Bounds on Supersymmetry Revisited,
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Astrophys. J. 598 (2003) 1163,arXiv:astro-ph/0304172.
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Detecting the Neutrino Mass Hierarchy with a Supernova at IceCube,
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JCAP 0306 (2003) 005,arXiv:hep-ph/0303210.
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Signatures of Supernova Neutrino Oscillations into Extra Dimensions,
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Astrophys. J. 592 (2003) 1035,arXiv:astro-ph/0302015.
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Effects of the Sound Speed of Quintessence on the Microwave Background and Large Scale Structure,
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Phys. Rev. D67 (2003) 103509,arXiv:astro-ph/0301284.
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Astrophys. J. 594 (2003) 390,arXiv:astro-ph/0301120.
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Asymmetric Explosions of Thermonuclear Supernovae,
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Gravitational lens time delays for distant supernovae: break the degeneracy between radial mass profiles and the Hubble constant,
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Mon. Not. Roy. Astron. Soc. 338 (2003) L25-L29,arXiv:astro-ph/0211499.
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Three-generation study of neutrino spin-flavor conversion in supernova and implication for neutrino magnetic moment,
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Phys. Rev. D67 (2003) 023004,arXiv:hep-ph/0211053.
[Ando:2002sk]
Mirror model for sterile neutrinos,
Veniamin Berezinsky, Mohan Narayan, Francesco Vissani,
Nucl. Phys. B658 (2003) 254,arXiv:hep-ph/0210204. From the abstract:... The considered subdominant neutrino oscillations (active <-> sterile) nu_a <-> nu_s can reveal itself as the big effects in observations of supernova neutrinos. [Berezinsky:2002fa]
The high energy gamma-ray emission expected from Tycho's supernova remnant,
H.J. Voelk, E.G. Berezhko, L.T. Ksenofontov, G.P. Rowell,
Astron. Astrophys. 396 (2002) 649,arXiv:astro-ph/0210176.
[Volk:2002nq]
Peculiar, Low Luminosity Type II Supernovae: Low Energy Explosions in Massive Progenitors?,
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[Zampieri:2002nj]
Gravitational Lensing Magnification and Time Delay Statistics for Distant Supernovae,
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Astrophys. J. 583 (2003) 584,arXiv:astro-ph/0210107.
[Oguri:2002hv]
Photometry and Spectroscopy of the Type IIP SN 1999em from Outburst to Dust Formation,
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Mon. Not. Roy. Astron. Soc. 338 (2003) 939-956,arXiv:astro-ph/0209623.
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What Can Be Learned with a Lead-Based Supernova-Neutrino Detector?,
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[Engel:2002hg]
Bulk neutrinos and core collapse supernovae,
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[Cacciapaglia:2002qr]
Monte Carlo study of supernova neutrino spectra formation,
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Astrophys.J. 590 (2003) 971-991,arXiv:astro-ph/0208035.
[Keil:2002in]
Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background,
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Phys. Rev. Lett. 89 (2002) 191101,arXiv:astro-ph/0207281.
[Pastor:2002we]
Tomography of the Earth's Core Using Supernova Neutrinos,
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Astropart. Phys. 19 (2003) 755,arXiv:hep-ph/0207238.
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Neutrino oscillation mechanism for pulsar kicks revisited,
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Phys. Rev. D66 (2002) 123005,arXiv:astro-ph/0206471.
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Connection between supernova shocks, flavor transformation, and the neutrino signal,
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Detection of supernova neutrinos by neutrino proton elastic scattering,
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Effects of neutrino oscillation on supernova neutrino: inverted mass hierarchy,
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Potential for supernova neutrino detection in MiniBooNE,
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Phys. Rev. D66 (2002) 013012,arXiv:hep-ph/0205035.
[Sharp:2002as]
Electron neutrino pair annihilation: A New source for muon and tau neutrinos in supernovae,
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Astrophys.J. 587 (2003) 320-326,arXiv:astro-ph/0205006.
[Buras:2002wt]
Detectability of the supernova relic neutrinos and neutrino oscillation,
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[Ando:2002ky]
Revisiting nonstandard interaction effects on supernova neutrino flavor oscillations,
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Determining the supernova direction by its neutrinos,
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[Ando:2001zi]
Time Delay Between Gravitational Waves and Neutrino Burst From a Supernova Explosion: a Test for the Neutrino Mass,
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Seeing double: strong gravitational lensing of high- redshift supernovae,
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Supernova neutrino detection in Borexino,
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Astropart. Phys. 16 (2002) 361-372,arXiv:hep-ph/0012082.
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Black hole formation in core collapse supernovae and time- of-flight measurements of the neutrino masses,
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Phys. Rev. D63 (2001) 073011,arXiv:astro-ph/0010398.
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Technique for direct eV scale measurements of the mu and tau neutrino masses using supernova neutrinos,
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Discovering ultra high energy neutrinos by horizontal and upward tau air-showers: First evidences in terrestrial gamma flashes,
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Astrophys. J. 570 (2002) 909-925,arXiv:astro-ph/0002453.
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Right-handed neutrino production in dense and hot plasmas,
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Nucl. Phys. B564 (2000) 204-222,arXiv:hep-ph/9907398.
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A new determination of supernova rates and a comparison with indicators for galactic star formation,
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Astron. Astrophys. 351 (1999) 459-466,arXiv:astro-ph/9904225.
[Cappellaro:1999qy]
Why are supernovae in our Galaxy so frequent?,
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Bound on the neutrino magnetic moment from chirality flip in supernovae,
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Electron neutrino mass measurement by supernova neutrino bursts and implications on hot dark matter,
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Constraints from $^{26}$Al Measurements on the Galaxy's Recent Global Star Formation Rate and Core Collapse Supernovae Rate,
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The rate of Supernovae from the combined sample of five searches,
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Resonant Neutrino Spin-Flavor Precession and Supernova Nucleosynthesis and Dynamics,
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Resonant spin-flavor conversion of supernova neutrinos and deformation of the electron antineutrino spectrum,
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Spectrum of the Supernova Relic Neutrino Background and Evolution of Galaxies,
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Astrophys. J. 460 (1996) 303-312,arXiv:astro-ph/9509130.
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Effects of random density fluctuations on matter enhanced neutrino flavor transitions in supernovae and implications for supernova dynamics and nucleosynthesis,
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Cherenkov radiation by neutrinos in a supernova core,
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Spectrum of the relic neutrino background from past supernovae and cosmological models,
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Neutrino oscillations in the magnetic field of the sun, supernovae, and neutron stars,
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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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Probing Efficient Cosmic-Ray Acceleration in Young Supernovae,
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34th International Cosmic Ray Conference (ICRC). [Dwarkadas:2015ppa]
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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IFAE 2012. [Vissani:2012dm]
Estimations of the Distances of Stellar Collapses in the Galaxy by Analyzing the Energy Spectrum of Neutrino Bursts,
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Astrophysical Models of r-Process Nucleosynthesis: An Update,
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11th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG11), Wako, Japan. [Qian:2012pe]
Neutral Current Coherent Cross Sections- Implications on Gaseous Spherical TPC's for detecting SN and Earth neutrinos,
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J. Phys. Conf. Ser. 309 (2011) 012031,arXiv:1103.1107.
Fifth symposium on large TPCs for low energy rare event detection and workshop on neutrinos from Supernovae, Paris Dec. 14-18, 2010. [Vergados:2011ym]
Lepton flavor violating New Physics and supernova explosion,
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Dirac neutrino magnetic moment and a possible time evolution of the neutrino signal from a supernova,
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XVI International Seminar Quarks'2010, Kolomna, Moscow Region, June 6-12, 2010. [Anikin:2010rh]
Can a supernova bang twice?,
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Yukawa International Program for Quark-Hadron Sciences: New Frontiers in QCD 2010, Kyoto, Japan. [Schaffner-Bielich:2010eyw]
The r-Process in Black Hole Winds,
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AIP Conf. Proc. 1269 (2010) 120-125,arXiv:1006.2277.
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Using supernova neutrinos to monitor the collapse, to search for gravity waves and to probe neutrino masses,
F. Vissani, G. Pagliaroli, F. Rossi-Torres,
arXiv:1005.3682, 2010.Galileo-Xu Guangqi meeting: The Sun, the Stars, the Universe and General Relativity; October 26-30, 2009, Shanghai (China). [Vissani:2010kwv]
Implication of the Steady State Equilibrium Condition for Electron-Positron Gas in the Neutrino-driven Wind from Proto-Neutron Star,
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arXiv:1005.1845, 2010.Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, Beijing, P. R. China. [Liu:2010pk]
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Probing the Core-Collapse Supernova Mechanism with Gravitational Waves,
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13th Gravitational Wave Data Analysis Workshop. [Ott:2009bw]
The Strange Prospects for Astrophysics,
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Supernova neutrinos: Strong coupling effects of weak interactions,
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arXiv:0809.2940, 2008.NO-VE 2008, IV International Workshop on. [Fogli:2008cz]
Formation of quark phases in compact stars and SN explosion,
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AIP Conf. Proc. 1056 (2008) 256-263,arXiv:0809.0518.
6th International Conference on Perspectives in Hadronic Physics, May 2008, Trieste. [Drago:2008tb]
Core-collapse supernova neutrinos and neutrino properties,
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Three days of Strong Interactions and Astrophysics HLPW08, 6-8 March 2008. [Gava:2008st]
Nucleosynthesis in Early Neutrino Driven Winds,
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CNR 2007 Compound-Nuclear Reactions and Related Topics Workshop. [Hoffman:2008jm]
Plasma induced neutrino spin-flip in a supernova and new bounds on the neutrino magnetic moment,
A.V. Kuznetsov, N.V. Mikheev,
arXiv:0708.2802, 2007.XIV International School 'Particles and Cosmology', Baksan Valley, Kabardino Balkaria, Russia, April 16-21, 2007. [Kuznetsov:2007np]
Spectral Modeling of Type II Supernovae,
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The Multicoloured Landscape of Compact Objects and their Explosive Progenitors: Theory vs Observations. [Baron:2006et]
Time-dependence Effects in Photospheric-Phase Type II Supernova Spectra,
Luc Dessart, John Hillier,
AIP Conf.Proc. 924 (2007) 441,arXiv:astro-ph/0610136.
The Multicoloured Landscape of Compact Objects and their Explosive Progenitors: Theory vs Observations, Cefalu, Sicily, June 11-24, 2006. [Dessart:2006ky]
Neutrinos from supernova remnants after the first HESS observations,
Francesco Vissani,
arXiv:astro-ph/0609575, 2006.Vulcano Workshop 2006: Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, 22-27 May 2006. [Vissani:2006pi]
R-process Experimental Campaign at the National Superconducting Cyclotron Laboratory,
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Aspects of Neutrino Production in Supernovae,
Todd A. Thompson,
arXiv:astro-ph/0608231, 2006.International Workshop on the Energy Budget in the High Energy Universe, Kashiwa campus, Univ. of Tokyo, Chiba, Japan, Feb. 2006. [Thompson:2006ar]
Neutrinos, Fisson Cycling, and the r-process,
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PoS NIC-IX (2006) 140,arXiv:astro-ph/0607180.
NIC-IX, International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, CERN, Geneva, Switzerland, 25-30 June, 2006. [Beun:2006vg]
Neutrino chirality flip in a supernova and the bound on the neutrino magnetic moment,
A.V. Kuznetsov, N.V. Mikheev,
arXiv:hep-ph/0606261, 2006.XIV International Seminar Quarks'2006, St.-Petersburg, Repino, Russia, May 19-25, 2006. [Kuznetsov:2006ch]
The Supernova Gamma-Ray Burst Connection,
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AIP Conf. Proc. 836 (2006) 398-407,arXiv:astro-ph/0604131.
AIP Conf. Proc. 'Gamma Ray Bursts in the Swift Era'. [Woosley:2006gw]
Shell-type Supernova Remnants,
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arXiv:astro-ph/0603502, 2006.Cherenkov 2005, Towards a Network of Atmospheric Cherenkov Detectors VII, Ecole Polytechnique, Palaiseau (France), April 27-29, 2005. [Volk:2006nm]
The Relic Neutrino Backround from the First Stars,
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arXiv:astro-ph/0603236, 2006.IIIrd International Workshop on: NO-VE 'Neutrino Oscillations in Venice', Venice Italy, February 2006. [Olive:2006ei]
Nucleosynthesis in Neutrino-Driven Supernovae,
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Astronomy with Radioactivities V, Clemson University, September 5-9, 2005. [Frohlich:2005em]
Neutrinos from Supernovas and Supernova Remnants,
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Aip Conf. Proc. 794 (2005) 219,arXiv:astro-ph/0508152.
IFAE, Catania 2005. [Costantini:2005vh]
Nucleosynthesis of PopIII Core Collapse Supernovae and the Abundances of Extremely Metal Poor Stars,
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IAU Symp. (2005),arXiv:astro-ph/0507340.
6IAU Symp. No. 228 'From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution'. [Limongi:2005yu]
SN/GRB connection: a statistical approach with BATSE and Asiago Catalogues,
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4th workshop on Gamma Ray Bursts in the Afterglow Era, Rome, 2004. [Valenti:2005vh]
Supernova search at intermediate z. II. Host galaxy morphology,
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ASP Conf.Ser. 342 (2005) 488,arXiv:astro-ph/0502397.
1604-2004: Supernovae as Cosmological Lighthouses. [Mendez:2005iu]
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1604-2004: Supernovae as Cosmological Lighthouses. [Altavilla:2005is]
Supernova Rates in Galaxy Clusters,
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1604-2004: Supernovae as Cosmological Lighthouses. [Maoz:2005xu]
Searching for Progenitors of Core-Collapse Supernovae,
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1604-2004: Supernovae as Cosmological Lighthouses. [VanDyk:2005yn]
Nuclear physics and astrophysics of the r-process,
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Nucl. Phys. A752 (2005) 550,arXiv:astro-ph/0501237.
International Nuclear Physics Conference (INPC2004). [Qian:2005am]
IMF variations and their implications for Supernovae numbers,
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'Baryons in Dark Matter Halos', Novigrad, Croatia, October 5-9, 2004. [Weidner:2004ni]
Supernova Neutrinos and the absolute scale of neutrino masses - a Bayesian approach,
Enrico Nardi,
arXiv:hep-ph/0412024, 2004.Fifth Latin American Simposium on High Energy Physics (V-SILAFAE) Lima, Peru, July 12-17, 2004. [Nardi:2004uz]
Supernova Neutrino Process and its Impact on the Galactic Chemical Evolution of the Light Elements,
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Nucl. Phys. A758 (2005) 35,arXiv:astro-ph/0410651.
Nuclei in the Cosmos VIII. [Yoshida:2004fm]
The r-process nucleosynthesis: a continued challenge for nuclear physics and astrophysics,
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Nuclei in the Cosmos. [Goriely:2004qb]
Sterile Neutrinos in astrophysical and cosmological sauce,
Marco Cirelli,
arXiv:astro-ph/0410122, 2004.10th International Symposium on Particles, Strings and Cosmology (PASCOS '04), August 2004, Boston, USA, and XVI Incontri sulla Fisica delle Alte Energie (IFAE), April 2004, Torino, Italy. [Cirelli:2004qs]
Parity Violation in Astrophysics,
C. J. Horowitz,
Eur. Phys. J. A24S2 (2005) 167,arXiv:nucl-th/0410074.
PAVI04 conference in Grenoble, France. [Horowitz:2004pc]
Powerful gravitational-wave bursts from supernova neutrino oscillations,
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'Hadron Physics - RANP 2004', Angra dos Reis - Rio de Janeiro - Brazil, March 28 to April 03. [MosqueraCuesta:2004xd]
Neutrino Oscillations at Supernova Core Bounce Generate the Strongest Gravitational-Wave Bursts,
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Core-Collapse Supernovae Induced by Anisotropic Neutrino Radiation,
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EAS Publ.Ser. 11 (2004) 163,arXiv:astro-ph/0406303.
Int. conf. in hohour of the 60th birthday of Marcel Arnould, The Future Astronuclear Physics, From microscopic puzzles to macroscopic nightmares. [Motizuki:2004jg]
Supernova Neutrino-Nucleus Physics and the r-process,
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Global Anisotropies in Supernova Explosions and Pulsar Recoil,
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Decays of supernova relic neutrinos,
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Sterile neutrinos: from cosmology to experiments,
Guido Marandella,
arXiv:hep-ph/0405090, 2004.39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 21-28 March 2004. [Marandella:2004xv]
Neutrinos from pre-supernova star,
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Acta Phys. Polon. B35 (2004) 1981,arXiv:astro-ph/0405006.
Epiphany Conference on Astroparticle Physics, 8-11 January 2004, Cracow, Poland. [Odrzywolek:2004em]
An Approach to Neutrino Radiative Transfer in Supernova Simulations,
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arXiv:astro-ph/0404401, 2004.Numerical Methods for Multidimensional Radiative Transfer Problems (RadConf2003), Heidelberg, Germany, 24-26 September 2003. [Cardall:2004nd]
The Evolution of Supernovae in the Winds of Massive Stars,
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Detection of Supernova Neutrinos,
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Acta Phys. Polon. B35 (2004) 1215,arXiv:hep-ph/0403117.
XXVIII Mazurian Lakes School of Physics, Krzyze, Poland, August 31 - September 7, 2003. [Bekman:2004qj]
Neutrino Processes in Supernovae and Neutrons Stars in Their Infancy and Old Age,
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arXiv:astro-ph/0403038, 2004.KIAS-APCTP International Symposium in Astro-Hadron Physics, November 10-14, 2003. [Prakash:2004wv]
Measuring neutrino masses with supernova neutrinos,
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arXiv:astro-ph/0401624, 2004.X Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July 2003. [Nardi:2004ms]
Low frequency radio and X-ray properties of core-collapse supernovae,
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Springer Proc.Phys. 99 (2005) 145-150,arXiv:astro-ph/0311419.
IAU Colloquium 192 'Supernovae (10 years of SN 1993J)', April 2003, Valencia, Spain. [Ray:2003nu]
Pulsar velocities and dark matter hint at a singlet neutrino,
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arXiv:astro-ph/0311240, 2003.Sixth RESCEU International Symposium 'Frontier in Astroparticle Physics and Cosmology', Tokyo, Japan, November 4 - 7, 2003. [Kusenko:2003ff]
Expected Changes of Supernovae with Redshift due to Evolution of their Progenitors,
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IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003. [Dominguez:2003rx]
44Ti radioactivity in young supernova remnants: Cas A and SN 1987A,
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New Astron. Rev. 48 (2004) 69,arXiv:astro-ph/0311080.
'Astronomy with Radioactivities IV', Seeon, Germany, June 2003. [Motizuki:2003dx]
Supernova Statistics,
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Springer Proc.Phys. 99 (2005) 347-354,arXiv:astro-ph/0310859.
IAU Colloquium 192, Supernovae: 10 Years of 1993J Valencia, Spain 22-26 April 2003. [Cappellaro:2003eg]
Type Ia Supernovae: Spectroscopic Surprises,
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arXiv:astro-ph/0310685, 2003.3-D Signatures of Stellar Explosions: A Workshop Honoring J. Craig Wheeler's 60th Birthday. [Branch:2003fr]
Effects of Small-Scale Fluctuations of Neutrino Flux in Supernova Explosions,
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Springer Proc.Phys. 99 (2005) 309-314,arXiv:astro-ph/0310481.
IAU Colloquium 192, SUPERNOVAE (10 years of SN1993J), Valencia, Spain. [Madokoro:2003hh]
Understanding Type II Supernovae,
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Springer Proc.Phys. 99 (2005) 275-280,arXiv:astro-ph/0310057.
IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003. [Zampieri:2003qn]
Observational Properties of Type II Plateau Supernovae,
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Springer Proc.Phys. 99 (2005) 195-199,arXiv:astro-ph/0310056.
IAU Colloquium 192, 'Supernovae (10 years of 1993J)', Valencia, Spain 22-26 April 2003. [Pastorello:2003qm]
Cosmic rays, stellar evolution, and supernova physics,
P. L. Biermann,
New Astron. Rev. 48 (2004) 41,arXiv:astro-ph/0309810.
'Astronomy With Radioactivities IV - Filling the Sensitivty Gap in MEV Astronomy', Seeon Conference, Bavaria, Germany, May 2003. [Biermann:2003et]
A Geometric Determination of the Distance to SN 1987A and the LMC,
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IAU Colloquium 192 'Supernovae (10 years of SN1993J)', Valencia, Spain. [Panagia:2003rt]
$^{56}\mathrm{Ni}$ mass in type IIP SNe: Light curves and H-alpha luminosities diagnostics,
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Springer Proc.Phys. 99 (2005) 303-308,arXiv:astro-ph/0309286.
IAU Colloquium 192: Supernovae (10 Years after SN1993J), Valencia, Spain, 22-26 Apr 2003. [Elmhamdi:2003wu]
Neutrinos and (anti)neutrinos from supernovae and from the earth in the Borexino detector,
L. Miramonti,
arXiv:hep-ex/0307029, 2003.1st Yamada Symposium on Neutrinos and Dark Matter in Nuclear Physics June 9-14, 2003, Nara, Japan. [Miramonti:2003hw]
Neutrinos in Extra Dimensions and Supernovae,
M. Cirelli,
arXiv:hep-ph/0305141, 2003.38th Rencontres de Moriond - Electroweak Interactions and Unified Theories, March 15-22, 2003, Les Arcs, France. [Cirelli:2003vh]
Neutrinos and Nucleosynthesis in Supernova,
U. Solis, J. C. D'Olivo, L. G. Cabral-Rosetti,
J. Phys. Conf. Ser. 37 (2006) 127-130,arXiv:hep-ph/0302015.
Mexican School of Astrophysics (EMA), Guanajuato, Mexico, July 31 - August 7, 2002. [Solis:2003ak]
Supernova Explosions from Accretion Disk Winds,
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arXiv:astro-ph/0301425, 2003.'From Twilight to Highlight - The Physics of Supernovae' ESO/MPA/MPE Workshop, Garching July 2002. [MacFadyen:2003wg]
Presupernova Evolution of Rotating Massive Stars and the Rotation Rate of Pulsars,
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IAU Symp. 215 (2004) 591,arXiv:astro-ph/0301374.
IAU 215 'Stellar Rotation'. [Heger:2003nh]
Supernovae, Gamma-Ray Bursts, and Stellar Rotation,
S. E. Woosley, A. Heger,
IAU Symp. (2003),arXiv:astro-ph/0301373.
IAU 215 'Stellar Rotation'. [Woosley:2003ng]
Circumstellar Interaction Around Supernovae,
Roger A. Chevalier,
arXiv:astro-ph/0301368, 2003.'From Twilight to Highlight - The Physics of Supernovae' ESO/MPA/MPE Workshop, Garching July 2002. [Chevalier:2003nb]
Observable Effects of Shocks in Compact and Extended Presupernovae,
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arXiv:astro-ph/0212569, 2002.ESO/MPA/MPE Workshop 'From Twilight to Highlight: The Physics of Supernovae', Garching, July 2002. [Blinnikov:2002tk]
Light Curves of Type Ia Supernovae as a Probe for an Explosion Model,
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arXiv:astro-ph/0212527, 2002.From Twilight to Highlight: The Physics of Supernovae, ESO Astrophysics Symposia. [Sorokina:2002gr]
The Mechanism of Core-Collapse Supernovae and the Ejection of Heavy Elements,
H.-Th. Janka, R. Buras, M. Rampp,
Nucl. Phys. A718 (2003) 269,arXiv:astro-ph/0212317.
NIC7, Fuji-Yoshida, Japan, July 8-12, 2002. [Janka:2002ej]
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,
Adv.Space Res. 33 (2004) 392-397,arXiv:astro-ph/0212188.
34th COSPAR Sci. Assembly, Houston, 10-19 october 2002. [Kosenko:2002yc]
Energy exchange inside SN ejecta and light curves of SNe Ia,
E.I.Sorokina, S.I.Blinnikov,
arXiv:astro-ph/0212187, 2002.11th Workshop on 'Nuclear Astrophysics', Ringberg Castle, Tegernsee, Germany, February 11-16, 2002. [Sorokina:2002yb]
Magnetic Field in Supernovae,
Shizuka Akiyama, J. Craig Wheeler,
arXiv:astro-ph/0211458, 2002.conference 'Core Collapse of Massive Stars'. [Akiyama:2002ur]
The Neutrino Signal in Stellar Core Collapse and Postbounce Evolution,
M. Liebendoerfer et al.,
Nucl. Phys. A719 (2003) 144,arXiv:astro-ph/0211329.
Nuclear Physics in Astrophysics Conference, Debrecen, Hungary, 2002. [Liebendoerfer:2002ny]
Variety in Supernovae,
Massimo Turatto, Stefano Benetti, Enrico Cappellaro,
arXiv:astro-ph/0211219, 2002.ESO / MPA / MPE Workshop: From Twilight to Highlight: The Physics of Supernovae, Garching, Germany, 29-31 June 2002. [Turatto:2002nx]
Synchronised neutrino oscillations from self interaction and associated applications,
Yvonne Y. Y. W.,
Aip Conf. Proc. 655 (2003) 240,arXiv:hep-ph/0211045.
3rd Topical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology, San Juan, Puerto Rico, 19-24 Aug 2002. [Wong:2002sc]
Nucleosynthesis as a result of multiple delayed detonations in Type Ia Supernovae,
Domingo Garcia-Senz, Eduardo Bravo,
Nucl. Phys. A718 (2003) 563,arXiv:astro-ph/0210339.
'Nuclei in the Cosmos VII' 2002. [Garcia-Senz:2002fvw]
Supernovae and Neutrinos,
John F. Beacom,
Nucl. Phys. Proc. Suppl. 118 (2003) 307,arXiv:astro-ph/0209136.
XXth International Conference on Neutrino Physics and Astrophysics (Neutrino 2002), Munich, Germany, May 25-30, 2002. [Beacom:2002th]
Neutron Stars, Pulsars and Supernova Remnants: concluding remarks,
F. Pacini,
arXiv:astro-ph/0208563, 2002.Proceedings of the 270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Jan. 21-25, 2002, Physikzentrum Bad Honnef. [Pacini:2002iv]
Supernova neutrinos, LSND and MiniBooNE,
Michel Sorel,
arXiv:hep-ph/0205207, 2002.37th Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, France, 9-16 Mar 2002. [Sorel:2002hd]
Core-collapse supernova simulations: Variations of the input physics,
M. Rampp, R. Buras, H.-Th. Janka, G. Raffelt,
arXiv:astro-ph/0203493, 2002.Proceedings of the 11th Workshop on 'Nuclear Astrophysics' held at Ringberg Castle, February 11-16, 2002. [Rampp:2002kn]
Supernova constraints on neutrino mass and mixing,
Srubabati Goswami,
Pramana 54 (2000) 173-184,arXiv:hep-ph/0104094.
Meeting on Recent Developments in Neutrino Physics, Ahmedabad, India, 2-4 Feb 1999. [Goswami:2000bv]
Supernova neutrinos and the neutrino masses,
J. F. Beacom,
Rev.Mex.Fis. 45 (1999) 36,arXiv:hep-ph/9901300.
22nd Symposium on Nuclear Physics, Oaxtepec, Morelos, Mexico, 5-8 Jan 1999. [Beacom:1999bn]
Supernova Remnants - Part One - Historical Events,
R. G. Strom, 1990.NATO Advanced Study Institute on Neutron Stars: Their Birth, Evolution, Radiation and Winds, Erice, Sicily, Italy, September 5-17, 1988, p. 253. [Strom-253-1990]
Supernova statistics and related problems,
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Understanding and visualizing the statistical analysis of SN1987A neutrino data,
Marcos V. dos Santos, Pedro Cunha de Holanda,
arXiv:2108.06448, 2021. [dosSantos:2021egl]
Relationships among detector signals recorded during events SN1987A and GW170817,
N. Agafonova, A. Malgin, E. Fischbach,
arXiv:2107.00265, 2021. [Agafonova:2021tgr]
SN1987A still shining: A Quest for Pseudo-Dirac Neutrinos,
Ivan Martinez-Soler, Yuber F. Perez-Gonzalez, Manibrata Sen,
arXiv:2105.12736, 2021. [Martinez-Soler:2021unz]
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,
Astrophys.J. 914 (2021) 4,arXiv:2102.09686.
[Utrobin:2021nhm]
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,
Astrophys.J.Lett. 908 (2021) L45,arXiv:2101.09029.
[Greco:2021sfi]
Supernova Constraints on Dark Flavored Sectors,
Jorge Martin Camalich, Jorge Terol-Calvo, Laura Tolos, Robert Ziegler,
Phys.Rev. D103 (2021) L121301,arXiv:2012.11632.
[Camalich:2020wac]
Supernova Muons: New Constraints on Z' Bosons, Axions, and ALPs,
Djuna Croon, Gilly Elor, Rebecca K. Leane, Samuel D. McDermott,
JHEP 2101 (2021) 107,arXiv:2006.13942.
[Croon:2020lrf]
NS 1987A in SN 1987A,
Dany Page, Mikhail V. Beznogov, Ivan Garibay, James M. Lattimer, Madappa Prakash, Hans-Thomas Janka,
Astrophys.J. 898 (2020) 125,arXiv:2004.06078.
[Page:2020gsx]
Properties of gamma-ray decay lines in 3D core-collapse supernova models, with application to SN 1987A and Cas A,
A. Jerkstrand et al.,
Mon.Not.Roy.Astron.Soc. 494 (2020) 2471-2497,arXiv:2003.05156.
[Jerkstrand:2020hlf]
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,
J.Exp.Theor.Phys. 128 (2019) 599-606,arXiv:1906.06088.
[Eroshenko:2019qiv]
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,
Astron.Astrophys. 624 (2019) A116,arXiv:1812.11083.
[Utrobin:2018mjr]
Can a bright and energetic X-ray pulsar be hiding amid the debris of SN 1987A?,
P. Esposito et al.,
Astrophys.J. 857 (2018) 58,arXiv:1803.04692.
[Esposito:2018nib]
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,
JHEP 1809 (2018) 051,arXiv:1803.00993.
[Chang:2018rso]
Updated Constraints on Self-Interacting Dark Matter from Supernova 1987A,
Cameron Mahoney, Adam K. Leibovich, Andrew R. Zentner,
Phys.Rev. D96 (2017) 043018,arXiv:1706.08871.
[Mahoney:2017jqk]
Evidence for two neutrinos bursts from SN1987A,
R. Valentim, J. E. Horvath, E. M. Rangel,
Int.J.Mod.Phys.Conf.Ser. 45 (2017) 1760040,arXiv:1706.07824.
[Valentim:2017ihe]
Revisiting Supernova 1987A Constraints on Dark Photons,
Jae Hyeok Chang, Rouven Essig, Samuel D. McDermott,
JHEP 1701 (2017) 107,arXiv:1611.03864.
[Chang:2016ntp]
New analysis for the correlation between gravitational waves and neutrino detectors during SN1987A,
P. Galeotti, G. Pizzella,
Eur.Phys.J. C76 (2016) 426,arXiv:1603.05076.
[Galeotti:2016uum]
Neutrino Signal of Collapse-Induced Thermonuclear Supernovae: The Case for Prompt Black Hole Formation in SN1987A,
Kfir Blum, Doron Kushnir,
Astrophys.J. 828 (2016) 31,arXiv:1601.03422.
[Blum:2016afe]
Signatures of Neutrino Cooling in the SN1987A Scenario,
Cristian G. Bernal, Nissim Fraija, Hidalgo-Gamez A. M,
Mon.Not.Roy.Astron.Soc. 442 (2014) 239,arXiv:1402.6292.
[Fraija:2014qup]
Evidence for two neutrino mass eigenstates from SN 1987A and the possibility of superluminal neutrinos,
Robert Ehrlich,
Astropart.Phys. 35 (2012) 625-628,arXiv:1111.0502.
[Ehrlich:2011kb]
Neutrino mass bound in the standard scenario for supernova electronic antineutrino emission,
Giulia Pagliaroli, Fernando Rossi-Torres, Francesco Vissani,
Astropart. Phys. 33 (2010) 287-291,arXiv:1002.3349.
[Pagliaroli:2010ik]
Bounds on the Parameter of Noncommutativity from Supernova SN1987A,
Mansour Haghighat,
Phys. Rev. D79 (2009) 025011,arXiv:0901.1069.
[Haghighat:2009pv]
Improved analysis of SN1987A antineutrino events,
G. Pagliaroli, F. Vissani, M.L. Costantini, A. Ianni,
Astropart.Phys. 31 (2009) 163-176,arXiv:0810.0466.
[Pagliaroli:2008ur]
How much can we learn from SN1987A events? Or: An analysis with a two-Component model for the antineutrino signal,
F. Vissani, G. Pagliaroli,
arXiv:0807.1301, 2008. [Vissani:2008ac]
Bounds on large extra dimensions from photon fusion process in SN1987A,
V. H. Satheeshkumar, P. K. Suresh,
JCAP 0806 (2008) 011,arXiv:0805.3429.
[Satheeshkumar:2008fb]
SN1987A Pulsar Velocity From Modified URCA Processes and Landau Levels,
Leonard S. Kisslinger, Sandip Pakvasa,
arXiv:0802.1689, 2008. [Kisslinger:2008rx]
Statistical analysis of neutrino events from SN1987A neutrino burst: estimation of the electron antineutrino mass,
B. I. Goryachev,
arXiv:0709.4627, 2007. [Goryachev:2007xg]
Unparticle constraints from SN1987A,
Steen Hannestad, Georg Raffelt, Yvonne Y. Y. Wong,
Phys. Rev. D76 (2007) 121701,arXiv:0708.1404.
[Hannestad:2007ys]
Supernovae as Probes of Extra Dimensions,
V. H. Satheesh Kumar, P. K. Suresh, P. K. Das,
AIP Conf. Proc. 939 (2007) 258-262,arXiv:0706.3551.
[SatheeshKumar:2007gb]
High resolution spectroscopy of the line emission from the inner circumstellar ring of SN 1987A and its hot spots,
Per Groeningsson et al.,
Astron.Astrophys. (2007),arXiv:astro-ph/0703788.
[Groeningsson:2007nh]
Neutrino Spectrum from SN 1987A and from Cosmic Supernovae,
Hasan Yuksel, John F. Beacom,
Phys. Rev. D76 (2007) 083007,arXiv:astro-ph/0702613.
[Yuksel:2007mn]
Magnetic field in supernova remnant SN 1987A,
E.G. Berezhko, L.T. Ksenofontov,
Astrophys. J. 650 (2006) L59-L62,arXiv:astro-ph/0608586.
[Berezhko:2006vv]
Is there a problem with low energy SN1987A neutrinos?,
Maria Laura Costantini, Aldo Ianni, Giulia Pagliaroli, Francesco Vissani,
JCAP 0705 (2007) 014,arXiv:astro-ph/0608399.
[Costantini:2006xd]
Constraints on neutrino mixing angle $\theta_{13}$ and Supernova neutrino fluxes from the LSD neutrino signal from SN1987A,
Oleg Lychkovskiy,
arXiv:hep-ph/0604113, 2006. [Lychkovskiy:2006yw]
Lower neutrino mass bound from SN1987A data and quantum geometry,
G. Lambiase, G. Papini, R. Punzi, G. Scarpetta,
Class. Quant. Grav. 23 (2006) 1347-1358,arXiv:gr-qc/0512154.
[Lambiase:2005ui]
New analysis of the SN 1987A neutrinos with a flexible spectral shape,
Alessandro Mirizzi, Georg G. Raffelt,
Phys. Rev. D72 (2005) 063001,arXiv:astro-ph/0508612.
[Mirizzi:2005tg]
The Three-Dimensional Circumstellar Environment of SN 1987A,
Ben E. K. Sugerman et al.,
Astrophys. J. Suppl. 159 (2005) 60-99,arXiv:astro-ph/0502378.
[Sugerman:2005dr]
The Light Curve of Supernova 1987A: The Structure of the Presupernova and Radioactive Nickel Mixing,
V. P. Utrobin,
Astron. Lett. 30 (2004) 293,arXiv:astro-ph/0406410.
[Utrobin:2004rt]
SN1987A and the properties of neutrino burst,
Maria Laura Costantini, Aldo Ianni, Francesco Vissani,
Phys. Rev. D70 (2004) 043006,arXiv:astro-ph/0403436.
[Costantini:2004ry]
Neutrinos from SN1987A: flavor conversion and interpretation of results,
C. Lunardini, A. Yu. Smirnov,
Astropart. Phys. 21 (2004) 703,arXiv:hep-ph/0402128.
[Lunardini:2004bj]
A Rotating Collapsar and Possible Interpretation of the LSD Neutrino Signal from SN 1987A,
V.S. Imshennik, O.G. Ryazhskaya,
Astron. Lett. 30 (2004) 14,arXiv:astro-ph/0401613.
[Imshennik:2004iya]
Supernova 1987A did not test the neutrino mass hierarchy,
V. Barger, D. Marfatia, B. P. Wood,
Phys. Lett. B532 (2002) 19-28,arXiv:hep-ph/0202158.
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SN1987A and the status of oscillation solutions to the solar neutrino problem,
M. Kachelriess, A. Strumia, R. Tomas, J. W. F. Valle,
Phys. Rev. D65 (2002) 073016,arXiv:hep-ph/0108100.
[Kachelriess:2001sg]
Bayesian analysis of neutrinos observed from supernova SN 1987A,
Thomas J. Loredo, Don Q. Lamb,
Phys. Rev. D65 (2002) 063002,arXiv:astro-ph/0107260. From the abstract:We present a Bayesian analysis of the energies and arrival times of the neutrinos from supernova SN 1987A detected by the Kamiokande II, IMB, and Baksan detectors, and find strong evidence for two components in the neutrino signal: a long time scale component from thermal Kelvin-Helmholtz cooling of the nascent neutron star, and a brief ($\sim 1$ s), softer component similar to that expected from emission by accreting material in the delayed supernova scenario. In the context of this model, we show that the data constrain the electron antineutrino rest mass to be less than 5.7~eV with 95% probability. [Loredo:2001rx]
Neutrinos from SN1987A, Earth matter effects and the LMA solution of the solar neutrino problem,
C. Lunardini, A. Yu. Smirnov,
Phys. Rev. D63 (2001) 073009,arXiv:hep-ph/0009356.
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SN1987A: A testing ground for the KARMEN anomaly,
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Contact interactions involving right-handed neutrinos and SN 1987A,
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Gamma-rays and the decay of neutrinos from SN1987A,
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Constraints to the decays of Dirac neutrinos from SN1987A,
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Neutrino helicity flips via electroweak interactions and SN1987A,
K. J. F. Gaemers, R. Gandhi, J. m. Lattimer,
Phys. Rev. D40 (1989) 309. [Gaemers:1989fp]
Limits to the Radiative Decays of Neutrinos and Axions from Gamma-Ray Observations of SN 1987a,
Edward W. Kolb, Michael S. Turner,
Phys. Rev. Lett. 62 (1989) 509. [Kolb:1988pe]
Constraints on decaying right-handed majorana neutrinos from SN1987A observations,
R. N. Mohapatra, S. Nussinov,
Phys. Rev. D39 (1989) 1378-1385. [Mohapatra:1989su]
constraints on the neutrino mass from the supernova data: a systematic analysis,
L. F. Abbott, A. De Rujula, T. P. Walker,
Nucl. Phys. B299 (1988) 734. [Abbott:1988bm]
implications of the triplet - majoron model for the supernova SN1987A,
Y. Aharonov, F. T. Avignone, S. Nussinov,
Phys. Rev. D37 (1988) 1360-1367. [Aharonov:1988ee]
Limit on the magnetic moment of the neutrino from supernova SN1987A observations,
Riccardo Barbieri, Rabindra N. Mohapatra,
Phys. Rev. Lett. 61 (1988) 27. [Barbieri:1988nh]
The magnetic moment of the neutrino and its implications for neutrino signal from SN1987A,
Riccardo Barbieri, R. N. Mohapatra, T. Yanagida,
Phys. Lett. B213 (1988) 69. [Barbieri:1988xw]
Correlation mass method for analysis of neutrinos from supernova 1987A,
H. Chiu, K. L. Chan, Y. Kondo,
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neutrino masses and flavors emitted in the supernova SN1987A,
R. Cowsik,
Phys. Rev. D37 (1988) 1685. 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]
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I. Goldman, Y. Aharonov, G. Alexander, S. Nussinov,
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The mass of the electron-neutrino: monte carlo studies of SN1987A observations,
David N. Spergel, J. N. Bahcall,
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J. N. Bahcall, T. Piran, W. H. Press, D. N. Spergel,
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Neutrino mass speculation on the neutrino events from the supernova LMC 1987 A,
H. Huzita,
Mod. Phys. Lett. A2 (1987) 905-911. 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]
How Reliable Are Neutrino Mass Limits Derived from SN 1987a?,
Edward W. Kolb, Albert J. Stebbins, Michael S. Turner,
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Neutrinos from supernova SN1987A,
David N. Schramm,
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Science 237 (1987) 1471. [Spergel:1987ch]
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19 - Phenomenology - Type II - SN1987A - Conference Proceedings
Neutrinos from SN 1987a. A Puzzle Revisited,
Gerd Schatz,
J. Phys. Conf. Ser. 632 (2015) 012024,arXiv:1507.07107.
24th European Cosmic Ray Symposium Kiel 2014. [Schatz:2015qxa]
Reexamination of a Bound on the Dirac Neutrino Magnetic Moment from the Supernova Neutrino Luminosity,
A.V. Kuznetsov, N.V. Mikheev, A.A. Okrugin,
arXiv:1011.2100, 2010.XVI International Seminar Quarks'2010, Kolomna, Moscow Region, June 6-12, 2010. [Kuznetsov:2010fe]
What is the issue with SN1987A neutrinos?,
F. Vissani, M.L. Costantini, W. Fulgione, A. Ianni, G. Pagliaroli,
Italian Phys.Soc.Proc. 103 (2011) 611-619,arXiv:1008.4726.
Vulcano Workshop 2010: Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, May 24-29, 2010. [Vissani:2010zi]
Analysis of Neutrino Signals from SN1987A,
G. Pagliaroli, M. L. Costantini, F. Vissani,
arXiv:0804.4598, 2008.IFAE 2007, 19th Conference on High Energy Physics: April 11-13 2007, Naples, Italy. [Pagliaroli:2008qi]
Analysis of the SN1987A two-stage explosion hypothesis with account for the MSW neutrino flavour conversion,
Oleg Lychkovskiy,
arXiv:0707.2508, 2007.Rencontres de Moriond EW 2007, 10-17 March 2007. [Lychkovskiy:2007ru]