Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars

Autores
Lucero, Gonzalo Agustin; BERNAL, Argelia; BARRANCO, Juan; Aceña, Andrés Esteban
Año de publicación
2024
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
It is shown that the data from the orbital period decay of binary pulsars give strong constraints on the dark matter-nucleons cross section. The limits are robust and competitive because this new method for testing dark matter interactions with standard model particles has a minimal number of assumptions combined with the extremely high accuracy on the measurement of the decay rate of the orbital period of binary systems. Our results exclude (with 95% confidence) spin independent interactions with cross sections greater that 3.1x10-31 cm2 for a dark matter particle with mass mc2 = 1 keV and 3.7x10-31 cm2 for mc2= 1 TeV which improves by several orders of magnitude previous constraints.
Fil: Lucero, Gonzalo Agustin. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Fil: BERNAL, Argelia. Departamento de Física, Universidad de Guanajuato; México
Fil: BARRANCO, Juan. Departamento de Física, Universidad de Guanajuato; México
Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Materia
dark matter
pulsar
cross section
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/265017
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsarsLucero, Gonzalo AgustinBERNAL, ArgeliaBARRANCO, JuanAceña, Andrés Estebandark matterpulsarcross sectionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1It is shown that the data from the orbital period decay of binary pulsars give strong constraints on the dark matter-nucleons cross section. The limits are robust and competitive because this new method for testing dark matter interactions with standard model particles has a minimal number of assumptions combined with the extremely high accuracy on the measurement of the decay rate of the orbital period of binary systems. Our results exclude (with 95% confidence) spin independent interactions with cross sections greater that 3.1x10-31 cm2 for a dark matter particle with mass mc2 = 1 keV and 3.7x10-31 cm2 for mc2= 1 TeV which improves by several orders of magnitude previous constraints.Fil: Lucero, Gonzalo Agustin. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; ArgentinaFil: BERNAL, Argelia. Departamento de Física, Universidad de Guanajuato; MéxicoFil: BARRANCO, Juan. Departamento de Física, Universidad de Guanajuato; MéxicoFil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; ArgentinaCornell University2024-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/265017Lucero, Gonzalo Agustin; BERNAL, Argelia; BARRANCO, Juan; Aceña, Andrés Esteban; Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars; Cornell University; ArXiv.org e-Print archive; 10-2024; 1-42331-8422CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2410.14559info:eu-repo/semantics/altIdentifier/doi/10.48550/arXiv.2410.14559info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:59:17Zoai:ri.conicet.gov.ar:11336/265017instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:59:17.447CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
title Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
spellingShingle Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
Lucero, Gonzalo Agustin
dark matter
pulsar
cross section
title_short Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
title_full Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
title_fullStr Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
title_full_unstemmed Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
title_sort Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars
dc.creator.none.fl_str_mv Lucero, Gonzalo Agustin
BERNAL, Argelia
BARRANCO, Juan
Aceña, Andrés Esteban
author Lucero, Gonzalo Agustin
author_facet Lucero, Gonzalo Agustin
BERNAL, Argelia
BARRANCO, Juan
Aceña, Andrés Esteban
author_role author
author2 BERNAL, Argelia
BARRANCO, Juan
Aceña, Andrés Esteban
author2_role author
author
author
dc.subject.none.fl_str_mv dark matter
pulsar
cross section
topic dark matter
pulsar
cross section
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv It is shown that the data from the orbital period decay of binary pulsars give strong constraints on the dark matter-nucleons cross section. The limits are robust and competitive because this new method for testing dark matter interactions with standard model particles has a minimal number of assumptions combined with the extremely high accuracy on the measurement of the decay rate of the orbital period of binary systems. Our results exclude (with 95% confidence) spin independent interactions with cross sections greater that 3.1x10-31 cm2 for a dark matter particle with mass mc2 = 1 keV and 3.7x10-31 cm2 for mc2= 1 TeV which improves by several orders of magnitude previous constraints.
Fil: Lucero, Gonzalo Agustin. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
Fil: BERNAL, Argelia. Departamento de Física, Universidad de Guanajuato; México
Fil: BARRANCO, Juan. Departamento de Física, Universidad de Guanajuato; México
Fil: Aceña, Andrés Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
description It is shown that the data from the orbital period decay of binary pulsars give strong constraints on the dark matter-nucleons cross section. The limits are robust and competitive because this new method for testing dark matter interactions with standard model particles has a minimal number of assumptions combined with the extremely high accuracy on the measurement of the decay rate of the orbital period of binary systems. Our results exclude (with 95% confidence) spin independent interactions with cross sections greater that 3.1x10-31 cm2 for a dark matter particle with mass mc2 = 1 keV and 3.7x10-31 cm2 for mc2= 1 TeV which improves by several orders of magnitude previous constraints.
publishDate 2024
dc.date.none.fl_str_mv 2024-10
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/265017
Lucero, Gonzalo Agustin; BERNAL, Argelia; BARRANCO, Juan; Aceña, Andrés Esteban; Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars; Cornell University; ArXiv.org e-Print archive; 10-2024; 1-4
2331-8422
CONICET Digital
CONICET
url http://hdl.handle.net/11336/265017
identifier_str_mv Lucero, Gonzalo Agustin; BERNAL, Argelia; BARRANCO, Juan; Aceña, Andrés Esteban; Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars; Cornell University; ArXiv.org e-Print archive; 10-2024; 1-4
2331-8422
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/2410.14559
info:eu-repo/semantics/altIdentifier/doi/10.48550/arXiv.2410.14559
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Cornell University
publisher.none.fl_str_mv Cornell University
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.13397

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