Results 41 to 50 of about 622,543 (345)

Diffuse Supernova Neutrino Background from extensive core-collapse simulations of $8$-$100 {\rm M}_\odot$ progenitors

open access: yes, 2017
We revisit the diffuse supernova neutrino background in light of recent systematic studies of stellar core collapse that reveal the quantitative impacts of the progenitor conditions on the collapse process. In general, the dependence of the progenitor on
Fischer, Tobias   +7 more
core   +1 more source

Multiwavelength View of Circumstellar Interaction in Supernovae

open access: yesUniverse
The interaction of post-explosion supernova ejecta with the surrounding circumstellar medium creates emissions across the electromagnetic spectrum. Since the circumstellar medium is created by the mass lost from the progenitor star, it carries tell-tale ...
Poonam Chandra
doaj   +1 more source

Models of Millimeter and Radio Emission from Interacting Supernovae

open access: yesThe Astrophysical Journal, 2022
This work utilizes established models of synchrotron-powered light curves for core-collapse supernovae in dense circumstellar environments, namely, type IIn and Ibn, to demonstrate the potential for detecting millimeter emission from these events.
Nitika Yadlapalli Yurk   +2 more
doaj   +1 more source

The consequences of nuclear electron capture in core collapse supernovae

open access: yes, 2003
The most important weak nuclear interaction to the dynamics of stellar core collapse is electron capture, primarily on nuclei with masses larger than 60. In prior simulations of core collapse, electron capture on these nuclei has been treated in a highly
A. Burrows   +21 more
core   +1 more source

Nucleosynthesis in Core Collapse Supernovae

open access: yesAIP Conference Proceedings, 2006
PDF Document, 6 pages, 2 figures. . Proceedings of "Origin of Matter and Evolution of Galaxies (OMEG05): New Horizon of Nuclear Astrophysics and Cosmology".
Limongi, M., Chieffi, A.
openaire   +2 more sources

Testing Magnetic Field Models for the Class 0 Protostar L1527

open access: yes, 2014
For the Class 0 protostar, L1527, we compare 131 polarization vectors from SCUPOL/JCMT, SHARP/CSO and TADPOL/CARMA observations with the corresponding model polarization vectors of four ideal-MHD, non-turbulent, cloud core collapse models.
Chapman, N. L.   +12 more
core   +1 more source

Core-Collapse Supernovae at the Threshold [PDF]

open access: yesInternational Astronomical Union Colloquium, 2005
SummaryRecent progress in modeling core-collapse supernovae is summarized and set in perspective. Two-dimensional simulations with state-of-the-art treatment of neutrino transport still fail to produce powerful explosions, but evidence is presented that they are very close to a success.
Janka, H.   +4 more
openaire   +4 more sources

Computational models of stellar collapse and core-collapse supernovae

open access: yesJournal of Physics: Conference Series, 2009
Core-collapse supernovae are among Nature's most energetic events. They mark the end of massive star evolution and pollute the interstellar medium with the life-enabling ashes of thermonuclear burning. Despite their importance for the evolution of galaxies and life in the universe, the details of the core-collapse supernova explosion mechanism remain ...
Ott, Christian D.   +5 more
openaire   +3 more sources

Gravitational waves from core collapse supernovae [PDF]

open access: yesClassical and Quantum Gravity, 2010
10 pages, 5 ...
Yakunin, Konstantin N   +10 more
openaire   +2 more sources

Progenitors of Core-Collapse Supernovae

open access: yes, 2017
Massive stars have a strong impact on their surroundings, in particular when they produce a core-collapse supernova at the end of their evolution. In these proceedings, we review the general evolution of massive stars and their properties at collapse as ...
Arnett, David   +5 more
core   +1 more source

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