Sharing but not caring: dark matter and the baryon asymmetry of the universe

Detalhes bibliográficos
Autor(a) principal: Bernal, Nicolas [UNESP]
Data de Publicação: 2016
Outros Autores: Fong, Chee Sheng, Fonseca, Nayara
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1475-7516/2016/09/005
http://hdl.handle.net/11449/162243
Resumo: We consider scenarios where Dark Matter (DM) particles carry baryon and/or lepton numbers, which can be defined if there exist operators connecting the dark to the visible sector. As a result, the DM fields become intimately linked to the Standard Model (SM) ones and can be maximally asymmetric just like the ordinary matter. In particular, we discuss minimal scenarios where the DM is a complex scalar or a Dirac fermion coupled to operators with nonzero baryon and/or lepton numbers, and that consist of only SM fields. We consider an initial asymmetry stored in either the SM or the DM sector; the main role of these operators is to properly share the asymmetry between the two sectors, in accordance with observations. After the chemical decoupling, the DM and SM sectors do not care about each other as there is only an ineffective communication between them. Once the DM mass is specified, the Wilson coefficients of these operators are fixed by the requirement of the correct transfer of the asymmetry. We study the phenomenology of this framework at colliders, direct detection and indirect detection experiments. In particular, the LHC phenomenology is very rich and can be tested in different channels such as the two same-sign leptons with two jets, monojet and monojet with a monolepton.
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spelling Sharing but not caring: dark matter and the baryon asymmetry of the universebaryon asymmetrydark matter theoryparticle physics - cosmology connectionWe consider scenarios where Dark Matter (DM) particles carry baryon and/or lepton numbers, which can be defined if there exist operators connecting the dark to the visible sector. As a result, the DM fields become intimately linked to the Standard Model (SM) ones and can be maximally asymmetric just like the ordinary matter. In particular, we discuss minimal scenarios where the DM is a complex scalar or a Dirac fermion coupled to operators with nonzero baryon and/or lepton numbers, and that consist of only SM fields. We consider an initial asymmetry stored in either the SM or the DM sector; the main role of these operators is to properly share the asymmetry between the two sectors, in accordance with observations. After the chemical decoupling, the DM and SM sectors do not care about each other as there is only an ineffective communication between them. Once the DM mass is specified, the Wilson coefficients of these operators are fixed by the requirement of the correct transfer of the asymmetry. We study the phenomenology of this framework at colliders, direct detection and indirect detection experiments. In particular, the LHC phenomenology is very rich and can be tested in different channels such as the two same-sign leptons with two jets, monojet and monojet with a monolepton.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Spanish MINECO'Joint Excellence in Science and Humanities' (JESH) program of the Austrian Academy of SciencesUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, R Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, BrazilAustrian Acad Sci, Inst High Energy Phys, Nikolsdorfer Gasse 18, A-1050 Vienna, AustriaUniv Sao Paulo, Inst Fis, Rua Matao 1371, BR-05508090 Sao Paulo, BrazilDESY, Notkestr 85, D-22607 Hamburg, GermanyUniv Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, R Dr Bento Teobaldo Ferraz 271, BR-01140070 Sao Paulo, BrazilFAPESP: 2011/11973-4FAPESP: 2013/01792-8FAPESP: 2012/10995-7FAPESP: 2013/13689-7FAPESP: 2015/15361-4Spanish MINECO: FPA2014-54459-PIop Publishing LtdUniversidade Estadual Paulista (Unesp)Austrian Acad SciUniversidade de São Paulo (USP)DESYBernal, Nicolas [UNESP]Fong, Chee ShengFonseca, Nayara2018-11-26T17:13:50Z2018-11-26T17:13:50Z2016-09-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article29application/pdfhttp://dx.doi.org/10.1088/1475-7516/2016/09/005Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 9, 29 p., 2016.1475-7516http://hdl.handle.net/11449/16224310.1088/1475-7516/2016/09/005WOS:000389772300008WOS000389772300008.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal Of Cosmology And Astroparticle Physics1,089info:eu-repo/semantics/openAccess2023-10-15T06:05:20Zoai:repositorio.unesp.br:11449/162243Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:58:50.832675Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Sharing but not caring: dark matter and the baryon asymmetry of the universe
title Sharing but not caring: dark matter and the baryon asymmetry of the universe
spellingShingle Sharing but not caring: dark matter and the baryon asymmetry of the universe
Bernal, Nicolas [UNESP]
baryon asymmetry
dark matter theory
particle physics - cosmology connection
title_short Sharing but not caring: dark matter and the baryon asymmetry of the universe
title_full Sharing but not caring: dark matter and the baryon asymmetry of the universe
title_fullStr Sharing but not caring: dark matter and the baryon asymmetry of the universe
title_full_unstemmed Sharing but not caring: dark matter and the baryon asymmetry of the universe
title_sort Sharing but not caring: dark matter and the baryon asymmetry of the universe
author Bernal, Nicolas [UNESP]
author_facet Bernal, Nicolas [UNESP]
Fong, Chee Sheng
Fonseca, Nayara
author_role author
author2 Fong, Chee Sheng
Fonseca, Nayara
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Austrian Acad Sci
Universidade de São Paulo (USP)
DESY
dc.contributor.author.fl_str_mv Bernal, Nicolas [UNESP]
Fong, Chee Sheng
Fonseca, Nayara
dc.subject.por.fl_str_mv baryon asymmetry
dark matter theory
particle physics - cosmology connection
topic baryon asymmetry
dark matter theory
particle physics - cosmology connection
description We consider scenarios where Dark Matter (DM) particles carry baryon and/or lepton numbers, which can be defined if there exist operators connecting the dark to the visible sector. As a result, the DM fields become intimately linked to the Standard Model (SM) ones and can be maximally asymmetric just like the ordinary matter. In particular, we discuss minimal scenarios where the DM is a complex scalar or a Dirac fermion coupled to operators with nonzero baryon and/or lepton numbers, and that consist of only SM fields. We consider an initial asymmetry stored in either the SM or the DM sector; the main role of these operators is to properly share the asymmetry between the two sectors, in accordance with observations. After the chemical decoupling, the DM and SM sectors do not care about each other as there is only an ineffective communication between them. Once the DM mass is specified, the Wilson coefficients of these operators are fixed by the requirement of the correct transfer of the asymmetry. We study the phenomenology of this framework at colliders, direct detection and indirect detection experiments. In particular, the LHC phenomenology is very rich and can be tested in different channels such as the two same-sign leptons with two jets, monojet and monojet with a monolepton.
publishDate 2016
dc.date.none.fl_str_mv 2016-09-01
2018-11-26T17:13:50Z
2018-11-26T17:13:50Z
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/10.1088/1475-7516/2016/09/005
Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 9, 29 p., 2016.
1475-7516
http://hdl.handle.net/11449/162243
10.1088/1475-7516/2016/09/005
WOS:000389772300008
WOS000389772300008.pdf
url http://dx.doi.org/10.1088/1475-7516/2016/09/005
http://hdl.handle.net/11449/162243
identifier_str_mv Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 9, 29 p., 2016.
1475-7516
10.1088/1475-7516/2016/09/005
WOS:000389772300008
WOS000389772300008.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal Of Cosmology And Astroparticle Physics
1,089
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 29
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing Ltd
publisher.none.fl_str_mv Iop Publishing Ltd
dc.source.none.fl_str_mv Web of Science
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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