Results 71 to 80 of about 59,386 (288)
The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae [PDF]
Fallback in core-collapse supernovae plays a crucial role in determining the properties of the compact remnants and of the ejecta composition. We perform three-dimensional simulations of mixing and fallback for selected non-rotating supernova models to ...
Conrad Chan, B. Mueller, A. Heger
semanticscholar +1 more source
Essential ingredients in core-collapse supernovae
Carrying 1044 joules of kinetic energy and a rich mix of newly synthesized atomic nuclei, core-collapse supernovae are the preeminent foundries of the nuclear species which make up our solar system and ourselves.
W. Raphael Hix +9 more
doaj +1 more source
Spectropolarimetry of Supernovae
Overwhelming evidence has accumulated in recent years that supernova explosions are intrinsically 3-dimensional phenomena with significant departures from spherical symmetry.
Chandrasekhar S +18 more
core +1 more source
Non-spherical core collapse supernovae and nucleosynthesis [PDF]
Motivated by observations of supernova SN 1987A, various authors have simulated Rayleigh-Taylor (RT) instabilities in the envelopes of core collapse supernovae (for a review, see Mueller 1998).
Kifonidis, K., Mueller, E., Plewa, T.
core +3 more sources
Young Core‐Collapse Supernova Remnants and Their Supernovae [PDF]
43 pages, ApJ, revised, discussion of 3C58 changed, in press for Feb.
openaire +2 more sources
SN 2020bio: A Double-peaked, H-poor Type IIb Supernova with Evidence of Circumstellar Interaction
We present photometric and spectroscopic observations of SN 2020bio, a double-peaked Type IIb supernova (SN) discovered within a day of explosion, primarily obtained by Las Cumbres Observatory and Swift.
C. Pellegrino +14 more
doaj +1 more source
Core-collapse supernovae missed by optical surveys [PDF]
We estimate the fraction of core-collapse supernovae (CCSNe) that remain undetected by optical SN searches due to obscuration by large amounts of dust in their host galaxies.
A. Alonso-Herrero +81 more
core +2 more sources
Exciting prospects for detecting late-time neutrinos from core-collapse supernovae [PDF]
In this theoretical study of successful core-collapse supernovae, the authors provide a detailed model of neutrino emission from the different phases of the transition - explosion to proto-neutron star cooling to late-time formation of either neutron ...
S. Li, L. Roberts, J. Beacom
semanticscholar +1 more source
Critical Conditions for Core-Collapse Supernovae [PDF]
The explosion of a core-collapse supernova can be approximated by the breakdown of steady-state solutions for accretion onto a proto-neutron star (PNS). We analytically show that as the neutrino luminosity exceeds a critical value L_c, the neutrinosphere pressure exceeds the hydrostatic limit even for an optimal shock radius R.
Keshet, Uri, Balberg, Shmuel
openaire +3 more sources
A New Monte Carlo Method for Time-Dependent Neutrino Radiation Transport [PDF]
Monte Carlo approaches to radiation transport have several attractive properties compared to deterministic methods. These include simplicity of implementation, high accuracy, and good parallel scaling.
Adam Burrows +51 more
core +2 more sources

