Self-Consistent Picture of the Mass Ejection from a One Second Long Binary Neutron Star Merger Leaving a Short-Lived Remnant in a General-Relativistic Neutrino-Radiation Magnetohydrodynamic Simulation-Reference-Cited by-同舟云学术

Self-Consistent Picture of the Mass Ejection from a One Second Long Binary Neutron Star Merger Leaving a Short-Lived Remnant in a General-Relativistic Neutrino-Radiation Magnetohydrodynamic Simulation

Published:2023-07-07 Issue:1 Volume:131 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Kiuchi Kenta^ORCID,Fujibayashi Sho^ORCID,Hayashi Kota^ORCID,Kyutoku Koutarou,Sekiguchi Yuichiro,Shibata Masaru

Funder

RIKEN

Japan Society for the Promotion of Science

Ministry of Education, Culture, Sports, Science and Technology

HPCI System Research Project

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.131.011401/fulltext

Reference128 articles.

1. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2. Multi-messenger Observations of a Binary Neutron Star Merger

3. GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M⊙

4. Properties of the Binary Neutron Star Merger GW170817

5. GW170817: Measurements of Neutron Star Radii and Equation of State

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