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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.
[Conley:2006tw]
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. [Astier:2005qq]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications,
A. Clocchiatti et al.(High Z SN Search),
Astrophys. J. 642 (2006) 1-21,arXiv:astro-ph/0510155.
[Clocchiatti:2005vy]
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.
[Nobili:2005tr]
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.
[Lidman:2004en]
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.
[Garavini:2004fa]
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 $P(\Omega_{\Lambda}>0)>0.99$. [Knop:2003iy]
Cosmological Results from High-z Supernovae,
John L. Tonry et al.(Supernova Search Team),
Astrophys. J. 594 (2003) 1,arXiv:astro-ph/0305008. From the abstract:The High-$ z$ Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval $ z=0.3-1.2$. These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to $ z\approx 1$, where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is $ w=-1$, then $ H_0\,t_0 = 0.96\pm0.04$, and $ \Omega_\Lambda-1.4\Omega_M=0.35\pm0.14$. Including the constraint of a flat Universe, we find $ \Omega_M=0.28\pm0.05$, independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on $ \Omega_M$ and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range $ -1.48-1$, we obtain $ w<-0.73$ at 95% confidence. [Tonry:2003zg]
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 Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration,
Adam G. Riess et al.(Supernova Search Team),
Astrophys. J. 560 (2001) 49-71,arXiv:astro-ph/0104455.
[Riess:2001gk]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae,
S. Perlmutter et al.(Supernova Cosmology Project),
Astrophys. J. 517 (1999) 565-586,arXiv:astro-ph/9812133. From the abstract:The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation $0.8 \,\Omega_{\rm M}- 0.6\,\Omega_\Lambda \approx -0.2 \pm 0.1$ in the region of interest ($\Omega_{\rm M} \lesssim 1.5$). For a flat ($\Omega_{\rm M}+\Omega_\Lambda = 1$) cosmology we find $\Omega_{\rm M}^{\rm flat} = 0.28^{+0.09}_{-0.08}$ (1$\sigma$ statistical) $^{+0.05}_{-0.04}$ (identified systematics). The data are strongly inconsistent with a $\Lambda = 0$ flat cosmology, the simplest inflationary universe model. An open, $\Lambda = 0$ cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of $P(\Lambda > 0) = 99$\%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is $t_0^{\rm flat}=14.9^{+1.4}_{-1.1}\,(0.63/h)$ Gyr for a flat cosmology. [Perlmutter:1998np]
Supernova Limits on the Cosmic Equation of State,
Peter M. Garnavich et al.(Supernova Search Team),
Astrophys. J. 509 (1998) 74-79,arXiv:astro-ph/9806396.
[Garnavich:1998th]
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,
Adam G. Riess et al.(Supernova Search Team),
Astron. J. 116 (1998) 1009-1038,arXiv:astro-ph/9805201.
[Riess:1998cb]
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]
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,
M. Aglietta et al.,
Nuovo Cim. C14 (1991) 171-193. [Aglietta:1991im]
Correlations of the low-energy pulses and muons recorded at the Mont Blanc LSD apparatus between 10 February and 1 July 1987,
V. L. Dadykin et al.,
Bull. Russ. Acad. Sci. Phys. 55 (1991) 4129. [Dadykin:1991sq]
Correlation between the Maryland and Rome gravitational wave detectors and the Mont Blanc, Kamioka and IMB particle detectors during SN1987A,
M. Aglietta et al.,
Nuovo Cim. B106 (1991) 1257-1269. [Aglietta:1991xa]
ANALYSIS OF THE DATA RECORDED BY THE MONT BLANC NEUTRINO DETECTOR AND BY THE MARYLAND AND ROME GRAVITATIONAL WAVE DETECTORS DURING SN1987A,
M. Aglietta et al.,
Nuovo Cim. C12 (1989) 75-103. [Aglietta:1989tw]
DETECTION OF A RARE EVENT ON 23 FEBRUARY 1987 BY THE NEUTRINO RADIATION DETECTOR UNDER MONT BLANC,
V. L. Dadykin et al.,
JETP Lett. 45 (1987) 593-595. [Dadykin:1987ek]
Resonance production of keV sterile neutrinos in core-collapse supernovae and lepton number diffusion,
Vsevolod Syvolap, Oleg Ruchayskiy, Alexey Boyarsky,
arXiv:1909.06320, 2019. [Syvolap:2019dat]
Triangulation Pointing to Core-Collapse Supernovae with Next-Generation Neutrino Detectors,
N. B. Linzer, K. Scholberg,
arXiv:1909.03151, 2019. [Linzer:2019swe]
Sensitivity of Super-Kamiokande with Gadolinium to Low Energy Anti-neutrinos from Pre-supernova Emission,
C. Simpson et al.,
arXiv:1908.07551, 2019. [Simpson:2019xwo]
Constraints for stellar electron-capture rates on $^{86}$Kr via the $^{86}$Kr($t$,$^{3}$He$+\gamma$)$^{86}$Br reaction and the implications for core-collapse supernovae,
R. Titus et al.,
arXiv:1908.03985, 2019. [Titus:2019pcw]
New Insights into Uncertainties in the Relic Neutrino Background and Effects from the Nuclear Equation of State,
Grant J. Mathews, Luca Boccioli, Jun Hidaka, Toshitaka Kajino,
arXiv:1907.10088, 2019. [Mathews:2019rjr]
The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics?,
Oscar Straniero, Inma Dominguez, Luciano Piersanti, Maurizio Giannotti, Alessandro Mirizzi,
arXiv:1907.06367, 2019. [Straniero:2019dtm]
Possible early linear acceleration of proto-neutron stars via asymmetric neutrino emission in core-collapse supernovae,
Hiroki Nagakura, Kohsuke Sumiyoshi, Shoichi Yamada,
Astrophys.J. 880 (2019) L28,arXiv:1907.04863.
[Nagakura:2019evv]
Multimessenger Asteroseismology of Core-Collapse Supernovae,
John Ryan Westernacher-Schneider, Evan O'Connor, Erin O'Sullivan, Irene Tamborra, Meng-Ru Wu, Sean M. Couch, Felix Malmenbeck,
arXiv:1907.01138, 2019. [Westernacher-Schneider:2019utn]
Probing Non-Standard Neutrino Interactions with Supernova Neutrinos at Hyper-K,
Minjie Lei, Noah Steinberg, James D. Wells,
arXiv:1907.01059, 2019. [Lei:2019nma]
The impact of asymmetric neutrino emissions on nucleosynthesis in core-collapse supernovae,
Shin-ichiro Fujimoto, Hiroki Nagakura,
Mon.Not.Roy.Astron.Soc. 488 (2019) L114-L118,arXiv:1906.09553.
[Fujimoto:2019kod]
Constraining the Fraction of Core-Collapse Supernovae Harboring Choked Jets with High-energy Neutrinos,
Dafne Guetta, Roi Rahin, Imre Bartos, Massimo Della Valle,
arXiv:1906.07399, 2019. [Guetta:2019wpb]
Presupernova neutrino signals as potential probes of neutrino mass hierarchy,
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Paleo-Detectors for Galactic Supernova Neutrinos,
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JCAP 1809 (2018) 029,arXiv:1808.01677.
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JCAP 1805 (2018) 066,arXiv:1804.03157.
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JCAP 1806 (2018) 019,arXiv:1803.04541.
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Phys.Rev. D97 (2018) 103018,arXiv:1803.04504.
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JCAP 1809 (2018) 002,arXiv:1712.03836.
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Confronting Models of Massive Star Evolution and Explosions with Remnant Mass Measurements,
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A physical model of mass ejection in failed supernovae,
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Pre-supernova neutrino emissions from ONe cores in the progenitors of core-collapse supernovae: are they distinguishable from those of Fe cores?,
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Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos,
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Study of Gamow-Teller transitions in isotopes of titanium within the quasi particle random phase approximation,
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How many nucleosynthesis processes exist at low metallicity?,
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Resolving neutrino mass hierarchy from supernova (anti)neutrino-nucleus reactions,
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Supernova Relic Neutrinos and the Supernova Rate Problem: Analysis of Uncertainties and Detectability of ONeMg and Failed Supernovae,
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Observing the Next Galactic Supernova,
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RAA 13 (2013) 1063-1074,arXiv:1305.1755.
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Revisiting the Triangulation Method for Pointing to Supernova and Failed Supernova with Neutrinos,
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Could a reported 2007 analysis of Super-Kamiokande data have missed a detectable supernova signal from Andromeda?,
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The First Supernova Explosions in the Universe,
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Light curves and $\mathrm{H}\alpha$ luminosities as indicators of $^{56}\mathrm{Ni}$ mass in type IIP supernovae,
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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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SN1999E: Another piece in the SN-GRB connection puzzle,
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Mirror model for sterile neutrinos,
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The high energy gamma-ray emission expected from Tycho's supernova remnant,
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Peculiar, Low Luminosity Type II Supernovae: Low Energy Explosions in Massive Progenitors?,
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What Can Be Learned with a Lead-Based Supernova-Neutrino Detector?,
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Bulk neutrinos and core collapse supernovae,
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Sterile neutrinos: from cosmology to experiments,
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IAU Colloquium 192 'Supernovae (10 years of SN 1993J)', April 2003, Valencia, Spain. [Ray:2003nu]
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Type Ia Supernovae: Spectroscopic Surprises,
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Neutrinos in Extra Dimensions and Supernovae,
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Neutrinos and Nucleosynthesis in Supernova,
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Mexican School of Astrophysics (EMA), Guanajuato, Mexico, July 31 - August 7, 2002. [Solis:2003ak]
Supernova Explosions from Accretion Disk Winds,
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IAU 215 'Stellar Rotation'. [Heger:2003nh]
Supernovae, Gamma-Ray Bursts, and Stellar Rotation,
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Magnetic Field in Supernovae,
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Synchronised neutrino oscillations from self interaction and associated applications,
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3rd Topical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology, San Juan, Puerto Rico, 19-24 Aug 2002. [Wong:2002sc]
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Supernovae and Neutrinos,
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Neutron Stars, Pulsars and Supernova Remnants: concluding remarks,
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Supernova neutrinos, LSND and MiniBooNE,
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Can a bright and energetic X-ray pulsar be hiding amid the debris of SN 1987A?,
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JHEP 1809 (2018) 051,arXiv:1803.00993.
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Updated Constraints on Self-Interacting Dark Matter from Supernova 1987A,
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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.
[Barger:2002px]
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.
[Lunardini:2000sw]
SN1987A: A testing ground for the KARMEN anomaly,
I. Goldman, R. Mohapatra, S. Nussinov,
Phys. Lett. B481 (2000) 151-159,arXiv:hep-ph/9912465.
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Contact interactions involving right-handed neutrinos and SN 1987A,
J. A. Grifols, E. Masso, R. Toldra,
Phys. Rev. D57 (1998) 2005-2008,arXiv:hep-ph/9707531.
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Gamma rays from SN1987A due to pseudoscalar conversion,
J. A. Grifols, E. Masso, R. Toldra,
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[Grifols:1996id]
Gamma-rays and the decay of neutrinos from SN1987A,
Andrew H. Jaffe, Michael S. Turner,
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Constraints to the decays of Dirac neutrinos from SN1987A,
Scott Dodelson, Joshua A. Frieman, Michael S. Turner,
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Limits to the Radiative Decays of Neutrinos and Axions from Gamma-Ray Observations of SN 1987a,
Edward W. Kolb, Michael S. Turner,
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Constraints on decaying right-handed majorana neutrinos from SN1987A observations,
R. N. Mohapatra, S. Nussinov,
Phys. Rev. D39 (1989) 1378-1385. [Mohapatra:1989su]
comment on 'constraints on the majoron interactions from the supernova SN1987A.',
Y. Aharonov, F. T. Avignone, S. Nussinov,
Phys. Rev. D39 (1989) 985. [Aharonov:1989ik]
Neutrino helicity flips via electroweak interactions and SN1987A,
K. J. F. Gaemers, R. Gandhi, J. m. Lattimer,
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Limit on the magnetic moment of the neutrino from supernova SN1987A observations,
Riccardo Barbieri, Rabindra N. Mohapatra,
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implications of the triplet - majoron model for the supernova SN1987A,
Y. Aharonov, F. T. Avignone, S. Nussinov,
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Implications of the supernova SN1987A neutrino signals,
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The magnetic moment of the neutrino and its implications for neutrino signal from SN1987A,
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Correlation mass method for analysis of neutrinos from supernova 1987A,
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The mass of the electron-neutrino: monte carlo studies of SN1987A observations,
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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]
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]
A simple model for neutrino cooling of the LMC supernova,
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Science 237 (1987) 1471. [Spergel:1987ch]
Neutrino temperatures and fluxes from the LMC supernova,
J. N. Bahcall, T. Piran, W. H. Press, D. N. Spergel,
Nature 327 (1987) 682-685. [Bahcall:1987ua]
Neutrino mass speculation on the neutrino events from the supernova LMC 1987 A,
H. Huzita,
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Constraint on the mass and lifetime of heavy neutrinos from the supernova SN1987A in the Large Magellanic Cloud,
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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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Total energy of neutrino burst from the supernova SN1987A and the mass of neutron star just born,
Katsuhiko Sato, Hideyuki Suzuki,
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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]
Neutrino events from SN1987A revisited,
B. Bekman, J. Holeczek, J. Kisiel,
Acta Phys. Polon. B37 (2006) 269,arXiv:hep-ph/0511271.
XXIX Mazurian Lakes Conference on Physics, August 30 - September 6, 2005, Piaski, Poland. [Bekman:2005rp]
SN 1987A: The Unusual Explosion of a Normal Type II Supernova,
Nino Panagia,
ASP Conf.Ser. (2004),arXiv:astro-ph/0410275.
International Conference '1604-2004 Supernovae as Cosmological Lighthouses' (Padova, Italy, June 16-19, 2004). [Panagia:2004ii]
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,
Phys. Atom. Nucl. 63 (2000) 979-983.2nd International Conference on Nonaccelerator New Physics (NANP 99), Dubna, Moscow Region, Russia, 28 June - 3 Jul 1999. [Huzita:2000vd]
Analysis of Neutrinos from Supernova 1987A,
H. Y. Chiu, K. L. Chan, Y. Kondo,
IAU Colloq. 108: Atmospheric Diagnostics of Stellar Evolution 422 (1988). [Chiu-Chan-Kondo-1988adse-conf-422C]
A Look at the Supernova SN 1987a,
David N. Schramm,
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Neutrino masses from SN1987a,
Jerrold Franklin, 1987.IN 'FAIRFAX 1987, PROCEEDINGS, SUPERNOVA 1987A IN THE LARGE MAGELLANIC CLOUD' 197-199. [Franklin:1987nz]
Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations,
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arXiv:1908.02928, 2019. [Sumiyoshi:2019qgs]
Three-Dimensional Boltzmann-Hydro Code for core-collapse in massive stars III. A New method for momentum feedback from neutrino to matter,
Hiroki Nagakura, Kohsuke Sumiyoshi, Shoichi Yamada,
Astrophys.J. 878 (2019) 160,arXiv:1906.10143.
[Nagakura:2019rdf]
Temporal and Angular Variations of 3D Core-Collapse Supernova Emissions and their Physical Correlations,
David Vartanyan, Adam Burrows, David Radice,
arXiv:1906.08787, 2019. [Vartanyan:2019ssu]
Fallback accretion powered supernova light curves based on a neutrino-driven explosion simulation of a 40 Msun star,
Takashi J. Moriya, Bernhard Muller, Conrad Chan, Alexander Heger, Sergei I. Blinnikov,
Astrophys.J. 880 (2019) 21,arXiv:1906.00153.
[Moriya:2019jon]
Towards an Understanding of the Resolution Dependence of Core-Collapse Supernova Simulations,
Hiroki Nagakura, Adam Burrows, David Radice, David Vartanyan,
arXiv:1905.03786, 2019. [Nagakura:2019gmh]
Long-term Simulations of Multi-Dimensional Core-collapse Supernovae: Implications for Neutron Star Kicks,
Ko Nakamura, Tomoya Takiwaki, Kei Kotake,
arXiv:1904.08088, 2019. [Nakamura:2019snn]
Resolution Study for Three-dimensional Supernova Simulations with the Prometheus-Vertex Code,
Tobias Melson, H.-Thomas Janka,
arXiv:1904.01699, 2019. [1904.01699]
One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars,
Takashi Yoshida, Tomoya Takiwaki, Kei Kotake, Koh Takahashi, Ko Nakamura, Hideyuki Umeda,
arXiv:1903.07811, 2019. [Yoshida:2019loj]
The $\nu$-process with fully time-dependent supernova neutrino emission spectra,
Andre Sieverding, Gabriel Martinez-Pinedo, Karlheinz Langanke, Robert Bollig, Hans-Thomas Janka, Alexander Heger,
Astrophys.J. 876 (2019) 151,arXiv:1902.06643.
[Sieverding:2019qet]
Simulating Turbulence-aided Neutrino-driven Core-collapse Supernova Explosions in One Dimension,
Sean M. Couch, MacKenzie L. Warren, Evan P. O'Connor,
arXiv:1902.01340, 2019. [Couch:2019mrd]
Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M$_{\odot}$ Stars,
Adam Burrows, David Radice, David Vartanyan,
Mon.Not.Roy.Astron.Soc. 485 (2019) 3153-3168,arXiv:1902.00547.
[Burrows:2019rtd]
Convection-Aided Explosions in One-Dimensional Core-Collapse Supernova Simulations I: Technique and Validation,
Quintin A. Mabanta, Jeremiah W. Murphy, Joshua C. Dolence,
arXiv:1901.11234, 2019. [Mabanta:2019mmm]
Features of Accretion Phase Gravitational Wave Emission from Two-dimensional Rotating Core-Collapse Supernovae,
Michael A. Pajkos, Sean M. Couch, Kuo-Chuan Pan, Evan P. O'Connor,
Astrophys.J. 878 (2019) 13,arXiv:1901.09055.
[Pajkos:2019nef]
Effects of SASI and LESA in the neutrino emission of rotating supernovae,
Laurie Walk, Irene Tamborra, Hans-Thomas Janka, Alexander Summa,
arXiv:1901.06235, 2019. [Walk:2019ier]
The Evolution towards Electron-capture Supernovae: the Flame Propagation and the Pre-bounce Electron-neutrino Radiation,
K. Takahashi, K. Sumiyoshi, S. Yamada, H. Umeda, T. Yoshida,
Astrophys.J. 871 (2019) 153,arXiv:1812.07175.
[Takahashi:2018lgj]
Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies,
Jade Powell, Bernhard Muller,
Mon.Not.Roy.Astron.Soc. 487 (2019) 1178-1190,arXiv:1812.05738.
[Powell:2018isq]
Three-Dimensional Simulations of Neutrino-Driven Core-Collapse Supernovae from Low-Mass Single and Binary Star Progenitors,
B. Muller, T.M. Tauris, A. Heger, P. Banerjee, Y.-Z. Qian, J. Powell, C. Chan, D.W. Gay, N. Langer,
Mon.Not.Roy.Astron.Soc. 484 (2019) 3307,arXiv:1811.05483.
[Muller:2018utr]
On the Neutrino Distributions in Phase Space for the Rotating Core-Collapse Supernova Simulated with a Boltzmann-Neutrino-Radiation-Hydrodynamics Code,
Akira Harada, Hiroki Nagakura, Wakana Iwakami, Hirotada Okawa, Shun Furusawa, Hideo Matsufuru, Kohsuke Sumiyoshi, Shoichi Yamada,
Astrophys.J. 872 (2019) 181,arXiv:1810.12316.
[Harada:2018ubo]
Gravitational waves and core-collapse supernovae,
G. S. Bisnovatyi-Kogan, S. G. Moiseenko,
Phys. Usp. 60 (2017) 843-850,arXiv:1810.12198.
[Bisnovatyi-Kogan:2017vpn]
Gravitational waves from three-dimensional core-collapse supernova models: The impact of moderate progenitor rotation,
H. Andresen, E. Muller, H.-Th. Janka, A. Summa, K. Gill, M. Zanolin,
Mon.Not.Roy.Astron.Soc. 486 (2019) 2238-2253,arXiv:1810.07638.
[Andresen:2018aom]
Effects of LESA in Three-Dimensional Supernova Simulations with Multi-Dimensional and Ray-by-Ray-plus Neutrino Transport,
Robert Glas, H.-Thomas Janka, Tobias Melson, Georg Stockinger, Oliver Just,
arXiv:1809.10150, 2018. [Glas:2018vcs]
Three-Dimensional Core-Collapse Supernova Simulations with Multi-Dimensional Neutrino Transport Compared to the Ray-by-Ray-plus Approximation,
Robert Glas, Oliver Just, H.-Thomas Janka, Martin Obergaulinger,
Astrophys.J. 873 (2019) 45,arXiv:1809.10146.
[Glas:2018oyz]
A Successful 3D Core-Collapse Supernova Explosion Model,
David Vartanyan, Adam Burrows, David Radice, Aaron Skinner, Joshua Dolence,
Mon.Not.Roy.Astron.Soc. 482 (2019) 351,arXiv:1809.05106.
[Vartanyan:2018iah]
Effects of rotation and magnetic field on the revival of a stalled shock in supernova explosions,
Kotaro Fujisawa, Hirotada Okawa, Yu Yamamoto, Shoichi Yamada,
Astrophys.J. 872 (2019) 155,arXiv:1809.04358.
[Fujisawa:2018dnh]
The Impact of Different Neutrino Transport Methods on Multidimensional Core-collapse Supernova Simulations,
Kuo-Chuan Pan et al.,
J.Phys. G46 (2019) 014001,arXiv:1806.10030.
[Pan:2018vkx]
Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project,
Ruben M. Cabezon et al.,
Astron.Astrophys. 619 (2018) A118,arXiv:1806.09184.
[Cabezon:2018lpr]
Fornax: a Flexible Code for Multiphysics Astrophysical Simulations,
M. Aaron Skinner, Joshua C. Dolence, Adam Burrows, David Radice, David Vartanyan,
Astrophys.J.Suppl. 241 (2019) 7,arXiv:1806.07390.
[Skinner:2018iti]
Global Comparison of Core-Collapse Supernova Simulations in Spherical Symmetry,
Evan O'Connor et al.,
J.Phys. G45 (2018) 104001,arXiv:1806.04175.
[OConnor:2018sti]
Core collapse with magnetic fields and rotation,
M. Obergaulinger, O. Just, M.A. Aloy,
J.Phys. G45 (2018) 084001,arXiv:1806.00393.
[Obergaulinger:2018udn]
Core-collapse supernova simulations in one and two dimensions: comparison of codes and approximations,
Oliver Just et al.,
Mon.Not.Roy.Astron.Soc. 481 (2018) 4786-4814,arXiv:1805.03953.
[Just:2018djz]
The non-linear onset of neutrino-driven convection in two and three-dimensional core-collapse supernovae,
Remi. Kazeroni, Brendan. K. Krueger, Jerome Guilet, Thierry Foglizzo, Daniel Pomarede,
Mon.Not.Roy.Astron.Soc. 480 (2018) 261-280,arXiv:1802.08125.
[Kazeroni:2018blm]
Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova,
Alexandra Gessner, Hans-Thomas Janka,
Astrophys.J. 865 (2018) 61,arXiv:1802.05274.
[Gessner:2018ekd]
$r$-Process Nucleosynthesis from Three-dimensional Jet-driven Core-Collapse Supernovae with Magnetic Misalignments,
Goni Halevi, Philipp Mosta,
Mon.Not.Roy.Astron.Soc. 477 (2018) 2366,arXiv:1801.08943.
[Halevi:2018vgp]
Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M$_{\odot}$,
David Vartanyan, Adam Burrows, David Radice, M. Aaron Skinner, Joshua Dolence,
Mon.Not.Roy.Astron.Soc. 477 (2018) 3091,arXiv:1801.08148.
[Vartanyan:2018xcd]
A full general relativistic neutrino radiation-hydrodynamics simulation of a collapsing very massive star and the formation of a black hole,
Takami Kuroda, Kei Kotake, Tomoya Takiwaki, Friedrich-Karl Thielemann,
Mon.Not.Roy.Astron.Soc. 477 (2018) L80-L84,arXiv:1801.01293.
[Kuroda:2018gqq]
Emission line models for the lowest-mass core collapse supernovae. I: Case study of a 9 $M_\odot$ one-dimensional neutrino-driven explosion,
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Mon.Not.Roy.Astron.Soc. 475 (2018) 277,arXiv:1710.04508.
[Jerkstrand:2017hbi]
Mass Ejection in Failed Supernovae: Variation with Stellar Progenitor,
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Mon.Not.Roy.Astron.Soc. 476 (2018) 2366-2383,arXiv:1710.01735.
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Black hole formation and fallback during the supernova explosion of a $40 \,\mathrm{M}_\odot$ star,
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Astrophys.J. 852 (2018) L19,arXiv:1710.00838.
[Chan:2017tdg]
Properties of Convective Oxygen and Silicon Burning Shells in Supernova Progenitors,
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Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition,
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A Detailed Comparison of Multi-Dimensional Boltzmann Neutrino Transport Methods in Core-Collapse Supernovae,
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Astrophys.J. 847 (2017) 133,arXiv:1706.06187.
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Supernova Simulations from a 3D Progenitor Model - Impact of Perturbations and Evolution of Explosion Properties,
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Mon.Not.Roy.Astron.Soc. 472 (2017) 491,arXiv:1705.00620.
[Muller:2017hht]
Light curve analysis of ordinary type IIP supernovae based on neutrino-driven explosion simulations in three dimensions,
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Astrophys.J. 846 (2017) 37,arXiv:1704.03800.
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A Parametric Study of the Acoustic Mechanism for Core-Collapse Supernovae,
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Astrophys.J. 839 (2017) 28,arXiv:1704.02984.
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The effect upon neutrinos of core-collapse supernova accretion phase turbulence,
James P. Kneller, Mithi de los Reyes,
J.Phys. G44 (2017) 084008,arXiv:1702.06951.
[Kneller:2017lqg]
Electron-Capture and Low-Mass Iron-Core-Collapse Supernovae: New Neutrino-Radiation-Hydrodynamics Simulations,
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Six-Dimensional Simulations of Core-Collapse Supernovae with Full Boltzmann Neutrino Transport,
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Astrophys.J. 854 (2018) 136,arXiv:1702.01752.
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The Gravitational Wave Signal of a Core Collapse Supernova Explosion of a 15M$_\odot$ Star,
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Nucleosynthesis in the Innermost Ejecta of Neutrino-Drive Supernova Explosions in Two Dimensions,
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Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism,
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Production and Distribution of 44Ti and 56Ni in a Three-dimensional Supernova Model Resembling Cassiopeia A,
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A new gravitational-wave signature of SASI activities in non-rotating supernova cores,
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Astrophys.J. 829 (2016) L14,arXiv:1605.09215.
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Astrophys.J. 831 (2016) 98,arXiv:1604.07848.
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Astrophys.J. 825 (2016) 6,arXiv:1511.07871.
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Astrophys.J. 854 (2018) 63,arXiv:1511.07443.
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Astrophys.J. 821 (2016) 38,arXiv:1510.04643.
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Quantum Simulations of Nuclei and Nuclear Pasta with the Multi-resolution Adaptive Numerical Environment for Scientific Simulations,
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Phys. Rev. C93 (2016) 055801,arXiv:1509.06671.
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Astrophys. J. 813 (2015) L6,arXiv:1509.02494.
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A Comparative study of hyperon equations of state in supernova simulations,
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Astrophys. J. 809 (2015) 116,arXiv:1508.01854.
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The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D,
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Mon. Not. Roy. Astron. Soc. 453 (2015) 287,arXiv:1506.05139.
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Astrophys. J. 808 (2015) L42,arXiv:1504.07631.
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The Three Dimensional Evolution to Core Collapse of a Massive Star,
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Astrophys. J. 808 (2015) L21,arXiv:1503.02199.
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A New Multi-Energy Neutrino Radiation-Hydrodynamics Code in Full General Relativity and Its Application to Gravitational Collapse of Massive Stars,
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Astrophys. J. Suppl. 222 (2016) 20,arXiv:1501.06330.
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A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics,
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Recent Progress on Ascertaining the Core Collapse Supernova Explosion Mechanism,
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Astrophys. J. 811 (2015) 97,arXiv:1412.1096.
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Neutrino-driven Turbulent Convection and Standing Accretion Shock Instability in Three-Dimensional Core-Collapse Supernovae,
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Astrophys. J. 808 (2015) 70,arXiv:1409.7078.
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Astrophys. J. 818 (2016) 123,arXiv:1409.5779.
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The Role of Turbulence in Neutrino-Driven Core-Collapse Supernova Explosions,
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Astrophys.J. 799 (2015) 5,arXiv:1408.1399.
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The criterion of supernova explosion revisited: the mass accretion history,
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Astrophys. J. 816 (2016) 43,arXiv:1406.6414.
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Astrophys.J.Suppl. 216 (2015) 5,arXiv:1403.4476.
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MODA: a new algorithm to compute optical depths in multi-dimensional hydrodynamic simulations,
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A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal,
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Astrophys.J. 788 (2014) 82,arXiv:1402.3415.
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PTEP 2014 (2014) 023D05,arXiv:1401.5579.
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Astrophys.J. 779 (2013) L18,arXiv:1310.8290.
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Porting Large HPC Applications to GPU Clusters: The Codes GENE and VERTEX,
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Irene Tamborra, Florian Hanke, Bernhard Mueller, Hans-Thomas Janka, Georg Raffelt,
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