We gratefully acknowledge support from
the Simons Foundation and member institutions.
Full-text links:

Download:

Current browse context:

astro-ph.HE

Change to browse by:

References & Citations

Bookmark

(what is this?)
CiteULike logo BibSonomy logo Mendeley logo del.icio.us logo Digg logo Reddit logo

Astrophysics > High Energy Astrophysical Phenomena

Title: Confronting Dark Matter Capture Rate with Continuous Gravitational Wave Probe of Local Neutron Stars

Abstract: 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.
Comments: 13 pages, 5 figures
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); Cosmology and Nongalactic Astrophysics (astro-ph.CO); Astrophysics of Galaxies (astro-ph.GA); Solar and Stellar Astrophysics (astro-ph.SR); High Energy Physics - Phenomenology (hep-ph)
Cite as: arXiv:2404.15038 [astro-ph.HE]
  (or arXiv:2404.15038v1 [astro-ph.HE] for this version)

Submission history

From: Pooja Bhattacharjee [view email]
[v1] Tue, 23 Apr 2024 13:42:41 GMT (444kb,D)

Link back to: arXiv, form interface, contact.