Results 81 to 90 of about 59,386 (288)
Fast-pairwise Collective Neutrino Oscillations Associated with Asymmetric Neutrino Emissions in Core-collapse Supernovae [PDF]
We present a linear stability analysis of the fast-pairwise neutrino flavor conversion based on a result of our latest axisymmetric core-collapse supernova (CCSN) simulation with full Boltzmann neutrino transport.
H. Nagakura +3 more
semanticscholar +1 more source
Hydrogen-Rich Core-Collapse Supernovae [PDF]
Hydrogen-rich core collapse supernovae, known as "Type II" supernovae, are the most common type of stellar explosion realized in nature. They are defined by the presence of prominent hydrogen lines in their spectra. Type II supernovae are observed only in star-forming galaxies, and several events have been directly linked to massive star progenitors ...
openaire +2 more sources
The Innermost Ejecta of Core Collapse Supernovae [PDF]
We ensure successful explosions (of otherwise non-explosive models) by enhancing the neutrino luminosity via reducing the neutrino scattering cross sections or by increasing the heating efficiency via enhancing the neutrino absorption cross sections in ...
Beloborodov +23 more
core +2 more sources
Observational Constraints on the Progenitors of Core-Collapse Supernovae: The Case for Missing High-Mass Stars [PDF]
Over the last 15 years, the supernova community has endeavoured to directly identify progenitor stars for core-collapse supernovae discovered in nearby galaxies.
S. Smartt
semanticscholar +1 more source
Understanding Core-Collapse Supernovae
Our understanding of core-collapse supernovae continues to improve as better microphysics is included in increasingly realistic neutrino-radiationhydrodynamic simulations. Recent multi-dimensional models with spectral neutrino transport, which slowly develop successful explosions for a range of progenitors between 12 and 25 solar mass, have motivated ...
W.R. Hix +8 more
openaire +2 more sources
Topics in core-collapse supernova-theory [PDF]
10 pages, 2 color figures, to be published in the proceedings of ``3-D Signatures in Stellar Explosions: A Workshop honoring J.
Burrows, Adam +2 more
openaire +2 more sources
Long gamma-ray bursts and core-collapse supernovae have different environments [PDF]
When massive stars exhaust their fuel they collapse and often produce the extraordinarily bright explosions known as core-collapse supernovae. On occasion, this stellar collapse also powers an even more brilliant relativistic explosion known as a long ...
A Heger +80 more
core +3 more sources
Toward Realistic Models of Core Collapse Supernovae: A Brief Review [PDF]
Motivated by their role as the direct or indirect source of many of the elements in the Universe, numerical modeling of core collapse supernovae began more than five decades ago.
A. Mezzacappa
semanticscholar +1 more source
Presolar graphite grains carry the isotopic signatures of their parent stars. A significant fraction of presolar graphites show isotopic abundance anomalies relative to solar for elements such as O, Si, Mg, and Ca, which are compatible with ...
Marco Pignatari +10 more
doaj +1 more source
Fast neutrino-flavor conversion in the preshock region of core-collapse supernovae [PDF]
We make a strong case that the fast neutrino-flavor conversion, one of the collective flavor oscillation modes, commonly occurs in core-collapse supernovae (CCSNe).
Taiki Morinaga +3 more
semanticscholar +1 more source

