activity
20052023
most citedBlack Hole Formation in Failing Core-Collapse Supernovae

751 citations · 5.7k across the 74 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 34 cited

Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves

Michael A. Pajkos, MacKenzie L. Warren, Sean M. Couch +2

The gravitational wave (GW) signal resulting from stellar core collapse encodes a wealth of information about the physical parameters of the progenitor star and the resulting core-…

astro-ph.HE2020★ 16 cited

Impact of neutrino pair-production rates in Core-Collapse Supernovae

Aurore Betranhandy, Evan O'Connor

In this paper, we present a careful study on the impact of neutrino pair-production on core-collapse supernovae via spherically-symmetric, general-relativistic simulations of two d…

physics.ins-det2020★ 2 cited

The Hyper-Kamiokande Experiment -- Snowmass LOI

Kamiokande Collaboration, K. Abe, P. Adrich +387

Hyper-Kamiokande is the next generation underground water Cherenkov detector that builds on the highly successful Super-Kamiokande experiment. The detector which has an 8.4~times l…

astro-ph.HE2020★ 56 cited

Gravitational-wave Signature of a First-order Quantum Chromodynamics Phase Transition in Core-Collapse Supernovae

Shuai Zha, Evan P. O'Connor, Ming-chung Chu +2

A first-order quantum chromodynamics (QCD) phase transition (PT) may take place in the protocompact star (PCS) produced by a core-collapse supernova (CCSN). In this work, we study…

astro-ph.IM2020★ 3 cited

Supernova Model Discrimination with Hyper-Kamiokande

Jost Migenda

Supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants---neutron sta…

astro-ph.HE2020★ 61 cited

Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation

A. S. Schneider, E. O'Connor, E. Granqvist +2

The core collapse of a massive star results in the formation of a proto-neutron star (PNS). If enough material is accreted onto a PNS it will become gravitationally unstable and fu…