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:
-
[1];
[2];
- Washington Univ., St. Louis, MO (United States)
- Ohio Univ., Athens, OH (United States); Univ. of California, Berkeley, CA (United States)
- 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)
- 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. https://doi.org/10.1088/1361-6471/ab337a
Alford, Mark G., Han, Sophia, and Schwenzer, Kai. Fri .
"Signatures for quark matter from multi-messenger observations". United States. https://doi.org/10.1088/1361-6471/ab337a. https://www.osti.gov/servlets/purl/1595000.
@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 = {Fri Oct 11 00:00:00 EDT 2019},
month = {Fri Oct 11 00:00:00 EDT 2019}
}
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Figures / Tables:
Figure 1: Conjectured diagram of phases of matter as a function of baryon chemical potential µ and temperature T . At the highest densities, we expect the color-flavor-locked (CFL) phase of quark matter.
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Are gravitational waves spinning down PSR J1023+0038?
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Tidal deformations of compact stars with crystalline quark matter
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Cooling of Accretion-Heated Neutron Stars
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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Moment of inertia, quadrupole moment, Love number of neutron star and their relations with strange matter equations of state
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Rapid neutrino cooling in the neutron star MXB 1659-29
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Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations
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Third family of compact stars within a nonlocal chiral quark model equation of state
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Constraining strangeness in dense matter with GW170817
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Tidal deformability and other global parameters of compact stars with strong phase transitions
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Constraints on the hybrid equation of state with a crossover hadron-quark phase transition in the light of GW170817
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Two-layer compact stars with crystalline quark matter: Screening effect on the tidal deformability
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Identifying a first-order phase transition in neutron star mergers through gravitational waves
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Signals in the tidal deformability for phase transitions in compact stars with constraints from GW170817
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Tidal deformability with sharp phase transitions in (binary) neutron stars
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Constraining twin stars with GW170817
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Strange stars as persistent sources of gravitational waves
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Thermal state of transiently accreting neutron stars
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The Low Quiescent X-Ray Luminosity of the Neutron Star Transient XTE J2123-058
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Gravitational Radiation Instability in Hot Young Neutron Stars
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Quasi-Normal Modes of Stars and Black Holes
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Quark deconfinement transition in hyperonic matter
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Constraining strangeness in dense matter with GW170817
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- arXiv
Tidal deformability and other global parameters of compact stars with strong phase transitions
text, January 2018
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Works referencing / citing this record:
Treating quarks within neutron stars
journal, November 2019
- Han, Sophia; Mamun, M. A. A.; Lalit, S.
- Physical Review D, Vol. 100, Issue 10
Treating quarks within neutron stars
text, January 2019
- Han, Sophia; Mamun, M. A. A.; Lalit, S.
- arXiv
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