activity
20062025
most citedThe neutrino signal from protoneutron star accretion and black hole formation

198 citations · 1.3k across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.HE2025★ 1 cited

Turbulence in Core-Collapse Supernovae

David Calvert, Michael Redle, Bibek Gautam +4

It is understood in a general sense that turbulent fluid motion below the shock front in a core-collapse supernova stiffens the effective equation of state of the fluid and aids in…

astro-ph.HE2020★ 58 cited

Stellar Mass Black Hole Formation and Multi-messenger Signals from Three Dimensional Rotating Core-Collapse Supernova Simulations

Kuo-Chuan Pan, Matthias Liebendörfer, Sean Couch +1

We present self-consistent, 3D core-collapse supernova simulations of a 40 Msun progenitor model using the isotropic diffusion source approximation for neutrino transport and an ef…

astro-ph.SR2019★ 62 cited

PUSHing core-collapse supernovae to explosions in spherical symmetry IV: Explodability, remnant properties and nucleosynthesis yields of low metallicity stars

Kevin Ebinger, Sanjana Curtis, Somdutta Ghosh +5

In this fourth paper of the series, we use the parametrized, spherically symmetric explosion method PUSH to perform a systematic study of two sets of non-rotating stellar progenito…

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★ 44 cited

Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project

Rubén M. Cabezón, Kuo-Chuan Pan, Matthias Liebendörfer +5

Modeling core-collapse supernovae (CCSNe) with neutrino transport in three dimensions (3D) requires tremendous computing resources and some level of approximation. We present a fir…

astro-ph.SR2018★ 117 cited

PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields

Sanjana Curtis, Kevin Ebinger, Carla Fröhlich +4

In a previously presented proof-of-principle study, we established a parametrized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse su…