Equation of state sensitivities when inferring neutron star and dense matter properties-Reference-Cited by-同舟云学术

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Equation of state sensitivities when inferring neutron star and dense matter properties

Published:2019-03-11 Issue:4 Volume:485 Page:5363-5376
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Greif S K¹²,Raaijmakers G³,Hebeler K¹²,Schwenk A¹²⁴,Watts A L³^ORCID

Affiliation:

1. Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt, Germany

2. ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, D-64291 Darmstadt, Germany

3. Anton Pannekoek Institute for Astronomy, University of Amsterdam, PO Box 94249, NL-1090GE Amsterdam, the Netherlands

4. Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany

Funder

German Research Foundation

European Research Council

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/485/4/5363/28262089/stz654.pdf

Reference54 articles.

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

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

3. Gravitational-Wave Constraints on the Neutron-Star-Matter Equation of State

4. A Massive Pulsar in a Compact Relativistic Binary

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4. Inference of neutron-star properties with unified crust-core equations of state for parameter estimation;Astronomy & Astrophysics;2024-06-25

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