Radius and equation of state constraints from massive neutron stars and GW190814-Reference-Cited by-同舟云学术

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Radius and equation of state constraints from massive neutron stars and GW190814

Published:2021-09-20 Issue:3 Volume:104 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Lim Yeunhwan,Bhattacharya Anirban,Holt Jeremy W.^ORCID,Pati Debdeep

Funder

Deutsche Forschungsgemeinschaft

Ewha Womans University

National Science Foundation

U.S. Department of Energy

National Nuclear Security Administration

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.104.L032802/fulltext

Reference74 articles.

1. GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object

2. THE BLACK HOLE MASS DISTRIBUTION IN THE GALAXY

3. Exploring the Lower Mass Gap and Unequal Mass Regime in Compact Binary Evolution

4. Could the 2.6 M⊙ object in GW190814 be a primordial black hole?

5. First direct comparison of nondisrupting neutron star-black hole and binary black hole merger simulations

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1. Constraining neutron star matter from the slope of the mass-radius curves;Physical Review D;2024-09-10

2. Visualizing the Number of Existing and Future Gravitational-wave Detections from Merging Double Compact Objects;The Astrophysical Journal;2024-07-01

3. Theoretical and experimental constraints for the equation of state of dense and hot matter;Living Reviews in Relativity;2024-06-05

4. Probing spin-induced quadrupole moments in precessing compact binaries;Physical Review D;2024-03-27

5. Symmetry energy and neutron star properties constrained by chiral effective field theory calculations;Physical Review C;2024-03-05

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