activity
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 2013 · astro-ph.HEShow all

5 papers · 2 filters

astro-ph.HE2013★ 213 cited

Revival of The Stalled Core-Collapse Supernova Shock Triggered by Precollapse Asphericity in the Progenitor Star

Sean M. Couch, Christian D. Ott

Multi-dimensional simulations of advanced nuclear burning stages of massive stars suggest that the Si/O layers of presupernova stars harbor large deviations from the spherical symm…

astro-ph.HE2013★ 132 cited

High-Resolution Three-Dimensional Simulations of Core-Collapse Supernovae in Multiple Progenitors

Sean M. Couch, Evan P. O'Connor

Three-dimensional simulations of core-collapse supernovae are granting new insight into the as-yet uncertain mechanism that drives successful explosions. While there is still debat…

astro-ph.HE2013★ 65 cited

Multidimensional Simulations of Rotating Pair Instability Supernovae

E. Chatzopoulos, J. C. Wheeler, S. M. Couch

We study the effects of rotation on the dynamics, energetics and Ni-56 production of Pair Instability Supernova explosions by performing rotating two-dimensional ("2.5-D") hydrodyn…

astro-ph.HE2013★ 79 cited

An Improved Multipole Approximation for Self-Gravity and Its Importance for Core-Collapse Supernova Simulations

Sean M. Couch, Carlo Graziani, Norbert Flocke

Self-gravity computation by multipole expansion is a common approach in problems such as core-collapse and Type Ia supernovae, where single large condensations of mass must be trea…

astro-ph.HE2013★ 72 cited

Radiation Transport for Explosive Outflows: A Multigroup Hybrid Monte Carlo Method

Ryan T. Wollaeger, Daniel R. van Rossum, Carlo Graziani +4

We explore Implicit Monte Carlo (IMC) and Discrete Diffusion Monte Carlo (DDMC) for radiation transport in high-velocity outflows with structured opacity. The IMC method is a stoch…