Detecting dark matter oscillations with gravitational waveforms

We consider the phase shift in the gravitational wave signal induced by fast oscillations of scalar dark matter surrounding binary systems, which could be probed by the future experiments LISA and DECIGO. This effect depends on the local matter density and the mass of the dark matter particle. We co...

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Detalles Bibliográficos
Autores: Brax, Philippe, Valageas, Patrick, Burrage, Clare, Ruiz Cembranos, José Alberto
Tipo de recurso: artículo
Fecha de publicación:2024
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/110433
Acceso en línea:https://hdl.handle.net/20.500.14352/110433
Access Level:acceso abierto
Palabra clave:52-33
530.12
Binary population
Astrofísica
2212 Física Teórica
2212.14 Teoría de la Relatividad
2101 Cosmología y Cosmogonía
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spelling Detecting dark matter oscillations with gravitational waveformsBrax, PhilippeValageas, PatrickBurrage, ClareRuiz Cembranos, José Alberto52-33530.12Binary populationAstrofísica2212 Física Teórica2212.14 Teoría de la Relatividad2101 Cosmología y CosmogoníaWe consider the phase shift in the gravitational wave signal induced by fast oscillations of scalar dark matter surrounding binary systems, which could be probed by the future experiments LISA and DECIGO. This effect depends on the local matter density and the mass of the dark matter particle. We compare it to the phase shift due to a standard dynamical friction term, which should generically be present. We find that the effect associated with the oscillations only dominates over the dynamical friction for dark matter masses below 10-21 eV, with masses below 10-23 eV implying cloud sizes that are too large to be realistic. Moreover, for masses of the order of 10-21 eV, LISA and DECIGO would only detect this effect for dark matter densities greater than that in the solar system by a factor 105 or 104 respectively. We conclude that this signal can be ignored for most dark matter scenarios unless very dense clouds of very light dark matter are created early in the Universe at a redshift z similar to 104.American Physical SocietyUniversidad Complutense de Madrid20242024-01-0120242024-01-01journal articlehttp://purl.org/coar/resource_type/c_6501AOhttp://purl.org/coar/version/c_b1a7d7d4d402bcceinfo:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/110433reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)InglésengMinisterio de Ciencia e Innovación http://dx.doi.org/10.13039/501100004837 Not available PID2019–107394GB-I00Ministerio de Ciencia e Innovación http://dx.doi.org/10.13039/501100004837 Not available PID2022139841NB-I00open accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/1104332026-06-02T12:44:21Z
dc.title.none.fl_str_mv Detecting dark matter oscillations with gravitational waveforms
title Detecting dark matter oscillations with gravitational waveforms
spellingShingle Detecting dark matter oscillations with gravitational waveforms
Brax, Philippe
52-33
530.12
Binary population
Astrofísica
2212 Física Teórica
2212.14 Teoría de la Relatividad
2101 Cosmología y Cosmogonía
title_short Detecting dark matter oscillations with gravitational waveforms
title_full Detecting dark matter oscillations with gravitational waveforms
title_fullStr Detecting dark matter oscillations with gravitational waveforms
title_full_unstemmed Detecting dark matter oscillations with gravitational waveforms
title_sort Detecting dark matter oscillations with gravitational waveforms
dc.creator.none.fl_str_mv Brax, Philippe
Valageas, Patrick
Burrage, Clare
Ruiz Cembranos, José Alberto
author Brax, Philippe
author_facet Brax, Philippe
Valageas, Patrick
Burrage, Clare
Ruiz Cembranos, José Alberto
author_role author
author2 Valageas, Patrick
Burrage, Clare
Ruiz Cembranos, José Alberto
author2_role author
author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 52-33
530.12
Binary population
Astrofísica
2212 Física Teórica
2212.14 Teoría de la Relatividad
2101 Cosmología y Cosmogonía
topic 52-33
530.12
Binary population
Astrofísica
2212 Física Teórica
2212.14 Teoría de la Relatividad
2101 Cosmología y Cosmogonía
description We consider the phase shift in the gravitational wave signal induced by fast oscillations of scalar dark matter surrounding binary systems, which could be probed by the future experiments LISA and DECIGO. This effect depends on the local matter density and the mass of the dark matter particle. We compare it to the phase shift due to a standard dynamical friction term, which should generically be present. We find that the effect associated with the oscillations only dominates over the dynamical friction for dark matter masses below 10-21 eV, with masses below 10-23 eV implying cloud sizes that are too large to be realistic. Moreover, for masses of the order of 10-21 eV, LISA and DECIGO would only detect this effect for dark matter densities greater than that in the solar system by a factor 105 or 104 respectively. We conclude that this signal can be ignored for most dark matter scenarios unless very dense clouds of very light dark matter are created early in the Universe at a redshift z similar to 104.
publishDate 2024
dc.date.none.fl_str_mv 2024
2024-01-01
2024
2024-01-01
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
AO
http://purl.org/coar/version/c_b1a7d7d4d402bcce
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/110433
url https://hdl.handle.net/20.500.14352/110433
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.relation.none.fl_str_mv Ministerio de Ciencia e Innovación http://dx.doi.org/10.13039/501100004837 Not available PID2019–107394GB-I00
Ministerio de Ciencia e Innovación http://dx.doi.org/10.13039/501100004837 Not available PID2022139841NB-I00
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,811543

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