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Title: Signatures for quark matter from multi-messenger observations

Abstract

In this article we review the prospects for detecting quark matter in neutron star cores. We survey the proposed signatures and emphasize the importance of data from neutron star mergers, which provide access to dynamical properties that operate on short timescales that are not probed by most other neutron star observables.

Authors:
ORCiD logo [1]; ORCiD logo [2];  [3]
  1. Washington Univ., St. Louis, MO (United States)
  2. Ohio Univ., Athens, OH (United States); Univ. of California, Berkeley, CA (United States)
  3. Istanbul Univ., Istanbul (Turkey)
Publication Date:
Research Org.:
Washington Univ., St. Louis, MO (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Nuclear Physics (NP) (SC-26)
OSTI Identifier:
1595000
Grant/Contract Number:  
FG02-05ER41375
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Physics. G, Nuclear and Particle Physics
Additional Journal Information:
Journal Volume: 46; Journal Issue: 11; Journal ID: ISSN 0954-3899
Publisher:
IOP Publishing
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Alford, Mark G., Han, Sophia, and Schwenzer, Kai. Signatures for quark matter from multi-messenger observations. United States: N. p., 2019. Web. doi:10.1088/1361-6471/ab337a.
Alford, Mark G., Han, Sophia, & Schwenzer, Kai. Signatures for quark matter from multi-messenger observations. United States. doi:10.1088/1361-6471/ab337a.
Alford, Mark G., Han, Sophia, and Schwenzer, Kai. Fri . "Signatures for quark matter from multi-messenger observations". United States. doi:10.1088/1361-6471/ab337a.
@article{osti_1595000,
title = {Signatures for quark matter from multi-messenger observations},
author = {Alford, Mark G. and Han, Sophia and Schwenzer, Kai},
abstractNote = {In this article we review the prospects for detecting quark matter in neutron star cores. We survey the proposed signatures and emphasize the importance of data from neutron star mergers, which provide access to dynamical properties that operate on short timescales that are not probed by most other neutron star observables.},
doi = {10.1088/1361-6471/ab337a},
journal = {Journal of Physics. G, Nuclear and Particle Physics},
number = 11,
volume = 46,
place = {United States},
year = {2019},
month = {10}
}

Journal Article:
Free Publicly Available Full Text
This content will become publicly available on October 11, 2020
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