Hybrid and quark star matter based on a nonperturbative equation of state-Reference-Cited by-同舟云学术

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Hybrid and quark star matter based on a nonperturbative equation of state

Published:2020-05-15 Issue:10 Volume:101 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Otto Konstantin^ORCID,Oertel Micaela^ORCID,Schaefer Bernd-Jochen^ORCID

Funder

Deutsche Forschungsgemeinschaft

Bundesministerium für Bildung und Forschung

Helmholtz International Center

German Academic Scholarship Foundation

Helmholtz Graduate School for Hadron and Ion Research

Physique fondamentale et ondes gravitationnelles

Observatoire de Paris

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.101.103021/fulltext

Reference121 articles.

1. The NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars

2. A two-solar-mass neutron star measured using Shapiro delay

3. A Massive Pulsar in a Compact Relativistic Binary

4. Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar

5. The equation of state of hot, dense matter and neutron stars

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1. Nucleon-quark mixed matter and neutron-star equation of state;Physical Review C;2024-08-26

2. Exploring pathways to forming twin stars;Physical Review D;2024-08-19

3. Impact of nonzero strangeness and momentum anisotropy on thermodynamics of finite volume quark matter;Physical Review D;2024-07-19

4. Central speed of sound, the trace anomaly, and observables of neutron stars from a perturbative analysis of scaled Tolman-Oppenheimer-Volkoff equations;Physical Review D;2023-11-27

5. Quark phases in neutron stars consistent with implications from NICER observations;Physical Review C;2023-09-26

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