Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
Abstract
The accumulation of certain types of dark matter particles in neutron star cores due to accretion over long timescales can lead to the formation of a mini black hole. In this scenario, the neutron star is destabilized and implodes to form a black hole without significantly increasing its mass. When this process occurs in neutron stars in coalescing binaries, one or both stars might be converted to a black hole before they merge. Thus, in the mass range of ~1–2M⊙, the Universe might contain three distinct populations of compact binaries: one containing only neutron stars, the second population of only black holes, and a third, mixed population consisting of a neutron star and a black hole. However, it is unlikely to have a mixed population as the various timescales allow for both neutron stars to remain or collapse within a short timescale. In this paper, we explore the capability of future gravitational-wave detector networks, including upgrades of Advanced LIGO and Virgo, and new facilities such as the Cosmic Explorer and Einstein Telescope (XG network), to discriminate between different populations by measuring the effective tidal deformability of the binary, which is zero for binary black holes but nonzero for binary neutronmore »
- Authors:
-
- Pennsylvania State University, University Park, PA (United States)
- University of Mississippi, Oxford, MS (United States)
- Johns Hopkins University, Baltimore, MD (United States)
- University of Washington, Seattle, WA (United States)
- Pennsylvania State University, University Park, PA (United States); Cardiff University (United Kingdom)
- Publication Date:
- Research Org.:
- Univ. of Washington, Seattle, WA (United States)
- Sponsoring Org.:
- USDOE; National Science Foundation (NSF); National Aeronautics and Space Administration (NASA)
- OSTI Identifier:
- 2229762
- Grant/Contract Number:
- FG02-00ER41132; 19-ATP19-0051; 20-LPS20-0011; 21- ATP21-0010; PHY-1836779; PHY-2012083; AST-2006384; PHY-2207638; AST-2205920; AST-2006538; PHY-2207502; PHY-090003; PHY20043; NSF PHY-1748958
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Volume: 107; Journal Issue: 8; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; Dark matter; Gravitational wave detection; Gravitational wave sources; Gravitational waves; Particle dark matter; Astronomical black holes; Neutron stars & pulsars; Weakly interacting massive particles
Citation Formats
Singh, Divya, Gupta, Anuradha, Berti, Emanuele, Reddy, Sanjay, and Sathyaprakash, B. S. Constraining properties of asymmetric dark matter candidates from gravitational-wave observations. United States: N. p., 2023.
Web. doi:10.1103/physrevd.107.083037.
Singh, Divya, Gupta, Anuradha, Berti, Emanuele, Reddy, Sanjay, & Sathyaprakash, B. S. Constraining properties of asymmetric dark matter candidates from gravitational-wave observations. United States. https://doi.org/10.1103/physrevd.107.083037
Singh, Divya, Gupta, Anuradha, Berti, Emanuele, Reddy, Sanjay, and Sathyaprakash, B. S. Fri .
"Constraining properties of asymmetric dark matter candidates from gravitational-wave observations". United States. https://doi.org/10.1103/physrevd.107.083037.
@article{osti_2229762,
title = {Constraining properties of asymmetric dark matter candidates from gravitational-wave observations},
author = {Singh, Divya and Gupta, Anuradha and Berti, Emanuele and Reddy, Sanjay and Sathyaprakash, B. S.},
abstractNote = {The accumulation of certain types of dark matter particles in neutron star cores due to accretion over long timescales can lead to the formation of a mini black hole. In this scenario, the neutron star is destabilized and implodes to form a black hole without significantly increasing its mass. When this process occurs in neutron stars in coalescing binaries, one or both stars might be converted to a black hole before they merge. Thus, in the mass range of ~1–2M⊙, the Universe might contain three distinct populations of compact binaries: one containing only neutron stars, the second population of only black holes, and a third, mixed population consisting of a neutron star and a black hole. However, it is unlikely to have a mixed population as the various timescales allow for both neutron stars to remain or collapse within a short timescale. In this paper, we explore the capability of future gravitational-wave detector networks, including upgrades of Advanced LIGO and Virgo, and new facilities such as the Cosmic Explorer and Einstein Telescope (XG network), to discriminate between different populations by measuring the effective tidal deformability of the binary, which is zero for binary black holes but nonzero for binary neutron stars. Furthermore, we show that observing the relative abundances of the different populations can be used to infer the timescale for neutron stars to implode into black holes, and in turn, provide constraints on the particle nature of dark matter. Furthermore, the XG network will infer the implosion timescale to within an accuracy of 0.01 Gyr at 90% credible interval and determine the dark matter mass and interaction cross section to within a factor of 2 GeV and 10 cm–2, respectively.},
doi = {10.1103/physrevd.107.083037},
journal = {Physical Review. D.},
number = 8,
volume = 107,
place = {United States},
year = {Fri Apr 28 00:00:00 EDT 2023},
month = {Fri Apr 28 00:00:00 EDT 2023}
}
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