activity
20152026
most citedCore-Collapse Supernova Explosion Theory

447 citations · 3.2k across the 49 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.HE2021

On the Origin of Pulsar and Magnetar Magnetic Fields

Christopher J. White, Adam Burrows, Matthew S. B. Coleman +1

In order to address the generation of neutron star magnetic fields, with particular focus on the dichotomy between magnetars and radio pulsars, we consider the properties of dynamo…

astro-ph.HE2021★ 21 cited

Efficient estimation method for time evolution of proto-neutron star mass and radius from supernova neutrino signal

Hiroki Nagakura, David Vartanyan

In this paper we present a novel method to estimate the time evolution of proto-neutron star (PNS) structure from the neutrino signal in core-collapse supernovae (CCSN). Employing…

astro-ph.SR2021★ 69 cited

The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis à vis One-Dimensional, Massive-star Supernova Progenitor Models

David Vartanyan, Matthew S. B. Coleman, Adam Burrows

The explosion outcome and diagnostics of core-collapse supernovae depend sensitively on the nature of the stellar progenitor, but most studies to date have focused exclusively on o…

astro-ph.SR2021★ 54 cited

Binary-Stripped Stars as Core-Collapse Supernovae Progenitors

David Vartanyan, Eva Laplace, Mathieu Renzo +3

Most massive stars experience binary interactions in their lifetimes that can alter both the surface and core structure of the stripped star with significant effects on their ultim…

astro-ph.HE2021★ 49 cited

Supernova neutrino signals based on long-term axisymmetric simulations

Hiroki Nagakura, Adam Burrows, David Vartanyan

We study theoretical neutrino signals from core-collapse supernova (CCSN) computed using axisymmetric CCSN simulations that cover the post-bounce phase up to ~s. We provide…

astro-ph.SR2021★ 160 cited

Different to the core: the pre-supernova structures of massive single and binary-stripped stars

E. Laplace, S. Justham, M. Renzo +4

The majority of massive stars live in binary or multiple systems and will interact during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae…