Continuum-mediated self-interacting dark matter

Detalhes bibliográficos
Autor(a) principal: Chaffey, Ian
Data de Publicação: 2021
Outros Autores: Fichet, Sylvain [UNESP], Tanedo, Philip
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1007/JHEP06(2021)008
http://hdl.handle.net/11449/207820
Resumo: Dark matter may self-interact through a continuum of low-mass states. This happens if dark matter couples to a strongly-coupled nearly-conformal hidden sector. This type of theory is holographically described by brane-localized dark matter interacting with bulk fields in a slice of 5D anti-de Sitter space. The long-range potential in this scenario depends on a non-integer power of the spatial separation, in contrast to the Yukawa potential generated by the exchange of a single 4D mediator. The resulting self-interaction cross section scales like a non-integer power of velocity. We identify the Born, classical and resonant regimes and investigate them using state-of-the-art numerical methods. We demonstrate the viability of our continuum-mediated framework to address the astrophysical small-scale structure anomalies. Investigating the continuum-mediated Sommerfeld enhancement, we demonstrate that a pattern of resonances can occur depending on the non-integer power. We conclude that continuum mediators introduce novel power-law scalings which open new possibilities for dark matter self-interaction phenomenology.
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spelling Continuum-mediated self-interacting dark matterPhenomenology of Field Theories in Higher DimensionsStrings and branes phenomenologyDark matter may self-interact through a continuum of low-mass states. This happens if dark matter couples to a strongly-coupled nearly-conformal hidden sector. This type of theory is holographically described by brane-localized dark matter interacting with bulk fields in a slice of 5D anti-de Sitter space. The long-range potential in this scenario depends on a non-integer power of the spatial separation, in contrast to the Yukawa potential generated by the exchange of a single 4D mediator. The resulting self-interaction cross section scales like a non-integer power of velocity. We identify the Born, classical and resonant regimes and investigate them using state-of-the-art numerical methods. We demonstrate the viability of our continuum-mediated framework to address the astrophysical small-scale structure anomalies. Investigating the continuum-mediated Sommerfeld enhancement, we demonstrate that a pattern of resonances can occur depending on the non-integer power. We conclude that continuum mediators introduce novel power-law scalings which open new possibilities for dark matter self-interaction phenomenology.Department of Physics & Astronomy University of California, 900 University AvenueICTP SAIFR & IFT-UNESP, R. Dr. Bento Teobaldo FerrazICTP SAIFR & IFT-UNESP, R. Dr. Bento Teobaldo FerrazUniversity of CaliforniaUniversidade Estadual Paulista (Unesp)Chaffey, IanFichet, Sylvain [UNESP]Tanedo, Philip2021-06-25T11:01:36Z2021-06-25T11:01:36Z2021-06-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1007/JHEP06(2021)008Journal of High Energy Physics, v. 2021, n. 6, 2021.1029-8479http://hdl.handle.net/11449/20782010.1007/JHEP06(2021)0082-s2.0-85107134038Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of High Energy Physicsinfo:eu-repo/semantics/openAccess2021-10-23T17:46:00Zoai:repositorio.unesp.br:11449/207820Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462021-10-23T17:46Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Continuum-mediated self-interacting dark matter
title Continuum-mediated self-interacting dark matter
spellingShingle Continuum-mediated self-interacting dark matter
Chaffey, Ian
Phenomenology of Field Theories in Higher Dimensions
Strings and branes phenomenology
title_short Continuum-mediated self-interacting dark matter
title_full Continuum-mediated self-interacting dark matter
title_fullStr Continuum-mediated self-interacting dark matter
title_full_unstemmed Continuum-mediated self-interacting dark matter
title_sort Continuum-mediated self-interacting dark matter
author Chaffey, Ian
author_facet Chaffey, Ian
Fichet, Sylvain [UNESP]
Tanedo, Philip
author_role author
author2 Fichet, Sylvain [UNESP]
Tanedo, Philip
author2_role author
author
dc.contributor.none.fl_str_mv University of California
Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Chaffey, Ian
Fichet, Sylvain [UNESP]
Tanedo, Philip
dc.subject.por.fl_str_mv Phenomenology of Field Theories in Higher Dimensions
Strings and branes phenomenology
topic Phenomenology of Field Theories in Higher Dimensions
Strings and branes phenomenology
description Dark matter may self-interact through a continuum of low-mass states. This happens if dark matter couples to a strongly-coupled nearly-conformal hidden sector. This type of theory is holographically described by brane-localized dark matter interacting with bulk fields in a slice of 5D anti-de Sitter space. The long-range potential in this scenario depends on a non-integer power of the spatial separation, in contrast to the Yukawa potential generated by the exchange of a single 4D mediator. The resulting self-interaction cross section scales like a non-integer power of velocity. We identify the Born, classical and resonant regimes and investigate them using state-of-the-art numerical methods. We demonstrate the viability of our continuum-mediated framework to address the astrophysical small-scale structure anomalies. Investigating the continuum-mediated Sommerfeld enhancement, we demonstrate that a pattern of resonances can occur depending on the non-integer power. We conclude that continuum mediators introduce novel power-law scalings which open new possibilities for dark matter self-interaction phenomenology.
publishDate 2021
dc.date.none.fl_str_mv 2021-06-25T11:01:36Z
2021-06-25T11:01:36Z
2021-06-01
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1007/JHEP06(2021)008
Journal of High Energy Physics, v. 2021, n. 6, 2021.
1029-8479
http://hdl.handle.net/11449/207820
10.1007/JHEP06(2021)008
2-s2.0-85107134038
url http://dx.doi.org/10.1007/JHEP06(2021)008
http://hdl.handle.net/11449/207820
identifier_str_mv Journal of High Energy Physics, v. 2021, n. 6, 2021.
1029-8479
10.1007/JHEP06(2021)008
2-s2.0-85107134038
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of High Energy Physics
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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