Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars

Fuente: arXiv
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Autores principales: Bhattacharjee, Pooja, Banik, Amit Dutta
Formato: Preprint
Publicado: 2024
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author Bhattacharjee, Pooja
Banik, Amit Dutta
author_facet Bhattacharjee, Pooja
Banik, Amit Dutta
contents Continuous gravitational waves (CGWs) from various astrophysical sources are one of the many future probes of upcoming gravitational wave (GW) search missions. Neutron stars (NSs) with deformity are one of the leading sources of CGW emissions. In this work, for the first time, a novel attempt to estimate the dark matter (DM) capture rate is performed using CGW as the probe to the local NS population. Competitive bounds on DM capture from the local NS population are reported when compared with DM direct search experiments and other astrophysical observations.
format Preprint
id arxiv_https___arxiv_org_abs_2404_15038
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
Bhattacharjee, Pooja
Banik, Amit Dutta
High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Solar and Stellar Astrophysics
High Energy Physics - Phenomenology
Continuous gravitational waves (CGWs) from various astrophysical sources are one of the many future probes of upcoming gravitational wave (GW) search missions. Neutron stars (NSs) with deformity are one of the leading sources of CGW emissions. In this work, for the first time, a novel attempt to estimate the dark matter (DM) capture rate is performed using CGW as the probe to the local NS population. Competitive bounds on DM capture from the local NS population are reported when compared with DM direct search experiments and other astrophysical observations.
title Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
topic High Energy Astrophysical Phenomena
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Solar and Stellar Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2404.15038