Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry

Detalhes bibliográficos
Autor(a) principal: Alves, Alexandre [UNIFESP]
Data de Publicação: 2016
Outros Autores: Camargo, Daniel A., Dias, Alex G., Longas, Robinson, Nishi, Celso C., Queiroz, Farinaldo S.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNIFESP
Texto Completo: https://repositorio.unifesp.br/handle/11600/56913
http://dx.doi.org/10.1007/JHEP10(2016)015
Resumo: Weakly Interacting Massive Particles (WIMPs) and axions are arguably the most compelling dark matter candidates in the literature. Could they coexist as dark matter particles? More importantly, can they be incorporated in a well motivated framework in agreement with experimental data? In this work, we show that this two component dark matter can be realized in the Inert Doublet Model in an elegant and natural manner by virtue of the spontaneous breaking of a Peccei-Quinn U(1)(PQ) symmetry into a residual Z(2) symmetry. The WIMP stability is guaranteed by the Z(2) symmetry and a new dark matter component, the axion, arises. There are two interesting outcomes: (i) vector-like quarks needed to implement the Peccei-Quinn symmetry in the model may act as a portal between the dark sector and the SM fields with a supersymmetry-type phenomenology at colliders
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spelling Alves, Alexandre [UNIFESP]Camargo, Daniel A.Dias, Alex G.Longas, RobinsonNishi, Celso C.Queiroz, Farinaldo S.2020-07-31T12:47:35Z2020-07-31T12:47:35Z2016Journal Of High Energy Physics. New York, v. , n. 10, p. -, 2016.1029-8479https://repositorio.unifesp.br/handle/11600/56913http://dx.doi.org/10.1007/JHEP10(2016)015WOS000386379600001.pdf10.1007/JHEP10(2016)015WOS:000386379600001Weakly Interacting Massive Particles (WIMPs) and axions are arguably the most compelling dark matter candidates in the literature. Could they coexist as dark matter particles? More importantly, can they be incorporated in a well motivated framework in agreement with experimental data? In this work, we show that this two component dark matter can be realized in the Inert Doublet Model in an elegant and natural manner by virtue of the spontaneous breaking of a Peccei-Quinn U(1)(PQ) symmetry into a residual Z(2) symmetry. The WIMP stability is guaranteed by the Z(2) symmetry and a new dark matter component, the axion, arises. There are two interesting outcomes: (i) vector-like quarks needed to implement the Peccei-Quinn symmetry in the model may act as a portal between the dark sector and the SM fields with a supersymmetry-type phenomenology at colliders(ii) two-component Inert Doublet Model re-opens the phenomenologically interesting 100{500 GeV mass region. We show that the model can successfully realize a two component dark matter framework and at the same time avoid low and high energy physics constraints such as monojet and dijet plus missing energy, as well as indirect and direct dark matter detection bounds.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)COLCIENCIASMainz Institute for Theoretical Physics (MITP)Univ Fed Sao Paulo, Dept Ciencias Exatas & Terra, BR-09972270 Diadema, SP, BrazilUniv Fed ABC, Ctr Ciencias Nat & Humanas, BR-09210580 Santo Andre, SP, BrazilUniv Antioquia, Inst Fis, Calle 70 52-21, Medellin, ColombiaUniv Fed ABC, Ctr Matemat Comp & Cognicao Nat, BR-09210580 Santo Andre, SP, BrazilMax Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, GermanyDepartamento de Ciências Exatas e da Terra, Universidade Federal de São Paulo, Diadema, BrasilCNPq: 307098/2014-1CNPq: 303094/2013-3CNPq: 311792/2012-0FAPESP: 2013/22079-8Web of Science-engSpringerJournal Of High Energy PhysicsBeyond Standard ModelCosmology of Theories beyond the SMDiscrete SymmetriesCollider and dark matter searches in the inert doublet model from Peccei-Quinn symmetryinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleNew York10info:eu-repo/semantics/openAccessreponame:Repositório Institucional da UNIFESPinstname:Universidade Federal de São Paulo (UNIFESP)instacron:UNIFESPORIGINALWOS000386379600001.pdfapplication/pdf919930${dspace.ui.url}/bitstream/11600/56913/1/WOS000386379600001.pdf97ddfdc77a2ef140baea36b4b2b6263cMD51open accessTEXTWOS000386379600001.pdf.txtWOS000386379600001.pdf.txtExtracted texttext/plain80366${dspace.ui.url}/bitstream/11600/56913/8/WOS000386379600001.pdf.txte0a3f75fa2721bffeef913aeaa796bdbMD58open accessTHUMBNAILWOS000386379600001.pdf.jpgWOS000386379600001.pdf.jpgIM Thumbnailimage/jpeg5856${dspace.ui.url}/bitstream/11600/56913/10/WOS000386379600001.pdf.jpge27b23f501da5808c60fa30f73a75a8eMD510open access11600/569132023-06-05 19:34:52.432open accessoai:repositorio.unifesp.br:11600/56913Repositório InstitucionalPUBhttp://www.repositorio.unifesp.br/oai/requestopendoar:34652023-06-05T22:34:52Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP)false
dc.title.en.fl_str_mv Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
title Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
spellingShingle Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
Alves, Alexandre [UNIFESP]
Beyond Standard Model
Cosmology of Theories beyond the SM
Discrete Symmetries
title_short Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
title_full Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
title_fullStr Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
title_full_unstemmed Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
title_sort Collider and dark matter searches in the inert doublet model from Peccei-Quinn symmetry
author Alves, Alexandre [UNIFESP]
author_facet Alves, Alexandre [UNIFESP]
Camargo, Daniel A.
Dias, Alex G.
Longas, Robinson
Nishi, Celso C.
Queiroz, Farinaldo S.
author_role author
author2 Camargo, Daniel A.
Dias, Alex G.
Longas, Robinson
Nishi, Celso C.
Queiroz, Farinaldo S.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Alves, Alexandre [UNIFESP]
Camargo, Daniel A.
Dias, Alex G.
Longas, Robinson
Nishi, Celso C.
Queiroz, Farinaldo S.
dc.subject.eng.fl_str_mv Beyond Standard Model
Cosmology of Theories beyond the SM
Discrete Symmetries
topic Beyond Standard Model
Cosmology of Theories beyond the SM
Discrete Symmetries
description Weakly Interacting Massive Particles (WIMPs) and axions are arguably the most compelling dark matter candidates in the literature. Could they coexist as dark matter particles? More importantly, can they be incorporated in a well motivated framework in agreement with experimental data? In this work, we show that this two component dark matter can be realized in the Inert Doublet Model in an elegant and natural manner by virtue of the spontaneous breaking of a Peccei-Quinn U(1)(PQ) symmetry into a residual Z(2) symmetry. The WIMP stability is guaranteed by the Z(2) symmetry and a new dark matter component, the axion, arises. There are two interesting outcomes: (i) vector-like quarks needed to implement the Peccei-Quinn symmetry in the model may act as a portal between the dark sector and the SM fields with a supersymmetry-type phenomenology at colliders
publishDate 2016
dc.date.issued.fl_str_mv 2016
dc.date.accessioned.fl_str_mv 2020-07-31T12:47:35Z
dc.date.available.fl_str_mv 2020-07-31T12:47:35Z
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dc.identifier.citation.fl_str_mv Journal Of High Energy Physics. New York, v. , n. 10, p. -, 2016.
dc.identifier.uri.fl_str_mv https://repositorio.unifesp.br/handle/11600/56913
http://dx.doi.org/10.1007/JHEP10(2016)015
dc.identifier.issn.none.fl_str_mv 1029-8479
dc.identifier.file.none.fl_str_mv WOS000386379600001.pdf
dc.identifier.doi.none.fl_str_mv 10.1007/JHEP10(2016)015
dc.identifier.wos.none.fl_str_mv WOS:000386379600001
identifier_str_mv Journal Of High Energy Physics. New York, v. , n. 10, p. -, 2016.
1029-8479
WOS000386379600001.pdf
10.1007/JHEP10(2016)015
WOS:000386379600001
url https://repositorio.unifesp.br/handle/11600/56913
http://dx.doi.org/10.1007/JHEP10(2016)015
dc.language.iso.fl_str_mv eng
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dc.publisher.none.fl_str_mv Springer
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