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Bibliographic Details
Main Authors: Jones, D. I., Riles, K.
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2403.02066
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author Jones, D. I.
Riles, K.
author_facet Jones, D. I.
Riles, K.
contents Rotating and oscillating neutron stars can give rise to long-lived Continuous Gravitational Waves (CGWs). Despite many years of searching, the detection of such a CGW signal remains elusive. In this article we describe the main astrophysical uncertainties regarding such emission, and their relation to the behaviour of matter at extremely high density. We describe the main challenges in searching for CGWs, and the prospects of detecting them using third-generation gravitational wave detectors. We end by describing some pressing issues in the field, whose resolution would help turn the detection and exploitation of CGWs into reality.
format Preprint
id arxiv_https___arxiv_org_abs_2403_02066
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Multimessenger observations and the science enabled: Continuous waves and their progenitors, equation of state of dense matter
Jones, D. I.
Riles, K.
High Energy Astrophysical Phenomena
Rotating and oscillating neutron stars can give rise to long-lived Continuous Gravitational Waves (CGWs). Despite many years of searching, the detection of such a CGW signal remains elusive. In this article we describe the main astrophysical uncertainties regarding such emission, and their relation to the behaviour of matter at extremely high density. We describe the main challenges in searching for CGWs, and the prospects of detecting them using third-generation gravitational wave detectors. We end by describing some pressing issues in the field, whose resolution would help turn the detection and exploitation of CGWs into reality.
title Multimessenger observations and the science enabled: Continuous waves and their progenitors, equation of state of dense matter
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2403.02066