Detectability of finite-temperature effects from neutron star mergers with next-generation gravitational wave detectors-Reference-Cited by-同舟云学术

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Detectability of finite-temperature effects from neutron star mergers with next-generation gravitational wave detectors

Published:2024-08-02 Issue:4 Volume:110 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Raithel Carolyn A.¹²^ORCID,Paschalidis Vasileios³³^ORCID

Affiliation:

1. Institute for Advanced Study

2. Princeton University

3. University of Arizona

Funder

National Science Foundation

University of Arizona

San Diego Supercomputer Center

Princeton University

XSEDE

Princeton Institute for Computational Science and Engineering

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.110.043002/fulltext

Reference81 articles.

1. Binary neutron star mergers: a review of Einstein’s richest laboratory

2. Rotating stars in relativity

3. Neutron star merger remnants

4. Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections

5. The Dynamics of Binary Neutron Star Mergers and GW170817

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