Ultralight vector dark matter search using data from the KAGRA O3GK run

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

Detalles Bibliográficos
Autores: Abac, A.G., LIGO Scientific Collaboration, Virgo Collaboration, KAGRA Collaboration, Braglia, M., Jaraba, S., Kuroyanagi, S., Morras, G., Nuño Siles, J.F., Ruiz Morales, E., García-Bellido Capdevila, Juan
Tipo de recurso: artículo
Fecha de publicación:2024
País:España
Institución:Universidad Autónoma de Madrid
Repositorio:Biblos-e Archivo. Repositorio Institucional de la UAM
Idioma:inglés
OAI Identifier:oai:repositorio.uam.es:10486/716887
Acceso en línea:http://hdl.handle.net/10486/716887
https://dx.doi.org/10.1103/PhysRevD.110.042001
Access Level:acceso abierto
Palabra clave:Gravitational wave
neutron stars
Hidden Markov model
Física
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spelling Ultralight vector dark matter search using data from the KAGRA O3GK runAbac, A.G.LIGO Scientific CollaborationVirgo CollaborationKAGRA CollaborationBraglia, M.Jaraba, S.Kuroyanagi, S.Morras, G.Nuño Siles, J.F.Ruiz Morales, E.García-Bellido Capdevila, JuanGravitational waveneutron starsHidden Markov modelFísicaArtículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAMAmong the various candidates for dark matter (DM), ultralight vector DM can be probed by laser interferometric gravitational wave detectors through the measurement of oscillating length changes in the arm cavities. In this context, KAGRA has a unique feature due to differing compositions of its mirrors, enhancing the signal of vector DM in the length change in the auxiliary channels. Here we present the result of a search for Formula Presented gauge boson DM using the KAGRA data from auxiliary length channels during the first joint observation run together with GEO600. By applying our search pipeline, which takes into account the stochastic nature of ultralight DM, upper bounds on the coupling strength between the Formula Presented gauge boson and ordinary matter are obtained for a range of DM masses. While our constraints are less stringent than those derived from previous experiments, this study demonstrates the applicability of our method to the lower-mass vector DM search, which is made difficult in this measurement by the short observation time compared to the auto-correlation timescale of DMAmerican Physical SocietyDepartamento de Física TeóricaFacultad de Ciencias20242024-08-15research articlehttp://purl.org/coar/resource_type/c_2df8fbb1AMhttp://purl.org/coar/version/c_ab4af688f83e57aainfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10486/716887https://dx.doi.org/10.1103/PhysRevD.110.042001reponame:Biblos-e Archivo. Repositorio Institucional de la UAMinstname:Universidad Autónoma de MadridInglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttp://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:repositorio.uam.es:10486/7168872026-06-23T12:46:27Z
dc.title.none.fl_str_mv Ultralight vector dark matter search using data from the KAGRA O3GK run
title Ultralight vector dark matter search using data from the KAGRA O3GK run
spellingShingle Ultralight vector dark matter search using data from the KAGRA O3GK run
Abac, A.G.
Gravitational wave
neutron stars
Hidden Markov model
Física
title_short Ultralight vector dark matter search using data from the KAGRA O3GK run
title_full Ultralight vector dark matter search using data from the KAGRA O3GK run
title_fullStr Ultralight vector dark matter search using data from the KAGRA O3GK run
title_full_unstemmed Ultralight vector dark matter search using data from the KAGRA O3GK run
title_sort Ultralight vector dark matter search using data from the KAGRA O3GK run
dc.creator.none.fl_str_mv Abac, A.G.
LIGO Scientific Collaboration
Virgo Collaboration
KAGRA Collaboration
Braglia, M.
Jaraba, S.
Kuroyanagi, S.
Morras, G.
Nuño Siles, J.F.
Ruiz Morales, E.
García-Bellido Capdevila, Juan
author Abac, A.G.
author_facet Abac, A.G.
LIGO Scientific Collaboration
Virgo Collaboration
KAGRA Collaboration
Braglia, M.
Jaraba, S.
Kuroyanagi, S.
Morras, G.
Nuño Siles, J.F.
Ruiz Morales, E.
García-Bellido Capdevila, Juan
author_role author
author2 LIGO Scientific Collaboration
Virgo Collaboration
KAGRA Collaboration
Braglia, M.
Jaraba, S.
Kuroyanagi, S.
Morras, G.
Nuño Siles, J.F.
Ruiz Morales, E.
García-Bellido Capdevila, Juan
author2_role author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Departamento de Física Teórica
Facultad de Ciencias
dc.subject.none.fl_str_mv Gravitational wave
neutron stars
Hidden Markov model
Física
topic Gravitational wave
neutron stars
Hidden Markov model
Física
description Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
publishDate 2024
dc.date.none.fl_str_mv 2024
2024-08-15
dc.type.none.fl_str_mv research article
http://purl.org/coar/resource_type/c_2df8fbb1
AM
http://purl.org/coar/version/c_ab4af688f83e57aa
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv http://hdl.handle.net/10486/716887
https://dx.doi.org/10.1103/PhysRevD.110.042001
url http://hdl.handle.net/10486/716887
https://dx.doi.org/10.1103/PhysRevD.110.042001
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
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
Attribution 4.0 International
http://creativecommons.org/licenses/by/4.0/
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:Biblos-e Archivo. Repositorio Institucional de la UAM
instname:Universidad Autónoma de Madrid
instname_str Universidad Autónoma de Madrid
reponame_str Biblos-e Archivo. Repositorio Institucional de la UAM
collection Biblos-e Archivo. Repositorio Institucional de la UAM
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,812455

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