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20072026
most citedExploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae

228 citations · 3.5k across the 65 of their papers we have counts for

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Showing 2018 · astro-ph.HEShow all

5 papers · 2 filters

astro-ph.HE2018★ 1 cited

FRIB and the GW170817 Kilonova

A. Aprahamian, R. Surman, A. Frebel +45

In July 2018 an FRIB Theory Alliance program was held on the implications of GW170817 and its associated kilonova for r-process nucleosynthesis. Topics of discussion included the a…

astro-ph.HE2018★ 228 cited

Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae

Evan O'Connor, Sean Couch

The details of the physical mechanism that drives core-collapse supernovae (CCSNe) remain uncertain. While there is an emerging consensus on the qualitative outcome of detailed CCS…

astro-ph.HE2018★ 154 cited

Global Comparison of Core-Collapse Supernova Simulations in Spherical Symmetry

Evan O'Connor, Robert Bollig, Adam Burrows +10

We present a comparison between several simulation codes designed to study the core-collapse supernova mechanism. We pay close attention to controlling the initial conditions and i…

astro-ph.HE2018★ 36 cited

The Impact of Different Neutrino Transport Methods on Multidimensional Core-collapse Supernova Simulations

Kuo-Chuan Pan, Carlos Mattes, Evan P. O'Connor +3

Neutrinos play a crucial role in the core-collapse supernova (CCSN) explosion mechanism. The requirement of accurately calculating the transport of neutrinos makes simulations of t…

astro-ph.HE2018★ 12 cited

The Antesonic Condition for the Explosion of Core-Collapse Supernovae I: Spherically Symmetric Polytropic Models: Stability & Wind Emergence

Matthias J. Raives, Sean M. Couch, Johnny P. Greco +2

Shock revival in core-collapse supernovae (CCSNe) may be due to the neutrino mechanism. While it is known that in a neutrino-powered CCSN, explosion begins when the neutrino lumino…