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Inference of the Neutron Star Equation of State from Cosmological Distances

Haster, Carl-Johan and Chatziioannou, Katerina and Bauswein, Andreas and Clark, James Alexander (2020) Inference of the Neutron Star Equation of State from Cosmological Distances. Physical Review Letters, 125 (26). Art. No. 261101. ISSN 0031-9007. doi:10.1103/PhysRevLett.125.261101. https://resolver.caltech.edu/CaltechAUTHORS:20200731-145542176

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Abstract

Finite-size effects on the gravitational wave signal from a neutron star merger typically manifest at high frequencies where detector sensitivity decreases. Proposed sensitivity improvements can give us access both to stronger signals and to a myriad of weak signals from cosmological distances. The latter will outnumber the former and the relevant part of the signal will be redshifted towards the detector’s most sensitive band. We study the redshift dependence of information about neutron star matter and find that single-scale properties, such as the star radius or the postmerger frequency, are better measured from the distant weak sources from z∼1.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevLett.125.261101DOIArticle
https://arxiv.org/abs/2004.11334arXivDiscussion Paper
ORCID:
AuthorORCID
Haster, Carl-Johan0000-0001-8040-9807
Chatziioannou, Katerina0000-0002-5833-413X
Bauswein, Andreas0000-0001-6798-3572
Additional Information:© 2020 American Physical Society. Received 27 April 2020; revised 23 August 2020; accepted 2 November 2020; published 21 December 2020. The authors would like to thank Tom Callister and Georgios Lioutas for useful discussions. We also thank Daniel Brown for providing the NEMO/OzHF sensitivity curve, and Evan Hall for providing the CE 20 km sensitivity curve. C.-J. H. acknowledge support of the National Science Foundation, and the LIGO Laboratory. A. B. acknowledges support by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program under Grant Agreement No. 759253. A. B. and by Deutsche Forschungsgemeinschaft (DFG, German Research Foundation), Project-ID 279384907, SFB 1245, and Project-ID 138713538, SFB 881 (“The Milky Way System”, subproject A10). J. A. C. acknowledge support of the National Science Foundation Grants No. PHY-1700765, No. OAC-1841475, and No. PHY-1809572. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under cooperative agreement PHY-1764464. The Flatiron Institute is supported by the Simons Foundation. The authors are grateful for computational resources provided by the LIGO Laboratory and supported by National Science Foundation Grants No. PHY-0757058 and No. PHY-0823459. This analysis was made possible by the lalsuite [127], astropy [128,129], numpy [130], scipy [131], and matplotlib [132] software packages. This article carries LIGO Document Number LIGO-P2000143.
Group:LIGO
Funders:
Funding AgencyGrant Number
LIGO LaboratoryUNSPECIFIED
European Research Council (ERC)759253
Deutsche Forschungsgemeinschaft (DFG)279384907
Deutsche Forschungsgemeinschaft (DFG)SFB 1245
Deutsche Forschungsgemeinschaft (DFG)138713538
Deutsche Forschungsgemeinschaft (DFG)SFB 881
NSFPHY-1700765
NSFOAC-1841475
NSFPHY-1809572
NSFPHY-1764464
Simons FoundationUNSPECIFIED
NSFPHY-0757058
NSFPHY-0823459
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentP2000143
Issue or Number:26
DOI:10.1103/PhysRevLett.125.261101
Record Number:CaltechAUTHORS:20200731-145542176
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200731-145542176
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:104686
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:31 Jul 2020 22:40
Last Modified:02 Sep 2021 22:42

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