Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817-Reference-Cited by-同舟云学术

Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817

Published:2022-05-20 Issue:10 Volume:105 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Kashyap Rahul^ORCID,Das Abhishek^ORCID,Radice David^ORCID,Padamata Surendra^ORCID,Prakash Aviral^ORCID,Logoteta Domenico^ORCID,Perego Albino^ORCID,Godzieba Daniel A.^ORCID,Bernuzzi Sebastiano^ORCID,Bombaci Ignazio^ORCID,Fattoyev Farrukh J.^ORCID,Reed Brendan T.^ORCID,Schneider André da Silva^ORCID

Funder

U.S. Department of Energy

National Science Foundation

H2020 European Research Council

National Energy Research Scientific Computing Center

Partnership for Advanced Computing in Europe AISBL

High Performance Computing Center Stuttgart

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.105.103022/fulltext

Reference72 articles.