Sharing but not caring: dark matter and the baryon asymmetry of the universe
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Outros Autores: | , |
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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Repositório Institucional da UNESP |
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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 |
|
_version_ |
1808128443987001344 |