Bayesian inference of the dense-matter equation of state encapsulating a first-order hadron-quark phase transition from observables of canonical neutron stars-Reference-Cited by-同舟云学术

Bayesian inference of the dense-matter equation of state encapsulating a first-order hadron-quark phase transition from observables of canonical neutron stars

Published:2021-03-02 Issue:3 Volume:103 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Xie Wen-Jie,Li Bao-An^ORCID

Funder

U.S. Department of Energy

National Natural Science Foundation of China

Yuncheng University

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.103.035802/fulltext

Reference49 articles.

1. Gravitational waves from neutron star mergers and their relation to the nuclear equation of state

2. Towards understanding astrophysical effects of nuclear symmetry energy

3. Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory

4. Was GW170817 a Canonical Neutron Star Merger? Bayesian Analysis with a Third Family of Compact Stars

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