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Search for continuous gravitational waves from unknown neutron stars in binary systems with long orbital periods in O3 data

Title: Search for continuous gravitational waves from unknown neutron stars in binary systems with long orbital periods in O3 data
Authors: Covas, P.; Papa, M.; Prix, R.
Source: The Astrophysical Journal
Publication Year: 2025
Collection: Max Planck Society: MPG.PuRe
Description: Gravitational waves emitted by asymmetric rotating neutron stars are the primary targets of continuous gravitational-wave searches. Neutron stars in binary systems are particularly interesting due to the potential for non-axisymmetric deformations induced by a companion star. However, all-sky searches for unknown neutron stars in binary systems are very computationally expensive and this limits their sensitivity and/or breadth. In this paper we present results of a search for signals with gravitational-wave frequencies between $50$ and $150$~Hz, from systems with orbital periods between $100$ and $1\,000$ days and projected semi-major axes between $40$ and $200$~light-seconds. This parameter-space region has never been directly searched before. We do not detect any signal, and our results exclude gravitational-wave amplitudes above $1.25 \times 10^{-25}$ at $144.32$~Hz with $95\%$ confidence. Our improved search pipeline is more sensitive than any previous all-sky binary search by about $75\%$.
Document Type: article in journal/newspaper
File Description: application/pdf
Language: unknown
Relation: info:eu-repo/semantics/altIdentifier/arxiv/2409.16196
Availability: https://hdl.handle.net/21.11116/0000-000F-E139-3; https://hdl.handle.net/21.11116/0000-000F-E13B-1; https://hdl.handle.net/21.11116/0000-0011-53BC-C
Rights: info:eu-repo/semantics/openAccess ; http://creativecommons.org/licenses/by/4.0/
Accession Number: edsbas.AD53AF52
Database: BASE