Electroweak symmetric dark matter balls

Detalhes bibliográficos
Autor(a) principal: Ponton, Eduardo [UNESP]
Data de Publicação: 2019
Outros Autores: Bai, Yang [UNESP], Jain, Bithika [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1007/JHEP09(2019)011
http://hdl.handle.net/11449/196230
Resumo: In the simple Higgs-portal dark matter model with a conserved dark matter number, we show that there exists a non-topological soliton state of dark matter. This state has smaller energy per dark matter number than a free particle state and has its interior in the electroweak symmetric vacuum. It could be produced in the early universe from first-order electroweak phase transition and contribute most of dark matter. This electroweak symmetric dark matter ball is a novel macroscopic dark matter candidate with an energy density of the electroweak scale and a mass of 1 gram or above. Because of its electroweak-symmetric interior, the dark matter ball has a large geometric scattering cross section off a nucleon or a nucleus. Dark matter and neutrino experiments with a large-size detector like Xenon1T, BOREXINO and JUNO have great potential to discover electroweak symmetric dark matter balls. We also discuss the formation of bound states of a dark matter ball and ordinary matter.
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spelling Electroweak symmetric dark matter ballsBeyond Standard ModelCosmology of Theories beyond the SMIn the simple Higgs-portal dark matter model with a conserved dark matter number, we show that there exists a non-topological soliton state of dark matter. This state has smaller energy per dark matter number than a free particle state and has its interior in the electroweak symmetric vacuum. It could be produced in the early universe from first-order electroweak phase transition and contribute most of dark matter. This electroweak symmetric dark matter ball is a novel macroscopic dark matter candidate with an energy density of the electroweak scale and a mass of 1 gram or above. Because of its electroweak-symmetric interior, the dark matter ball has a large geometric scattering cross section off a nucleon or a nucleus. Dark matter and neutrino experiments with a large-size detector like Xenon1T, BOREXINO and JUNO have great potential to discover electroweak symmetric dark matter balls. We also discuss the formation of bound states of a dark matter ball and ordinary matter.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)U. S. Department of EnergyNational Science FoundationMunich Institute for Astro-and Particle Physics (MIAPP) of the DFG cluster of excellence Origin and Structure of the UniverseUniv Estadual Paulista, ICTP South Amer Inst Fundamental Res, Sao Paulo, BrazilUniv Estadual Paulista, Inst Fis Teor, Sao Paulo, BrazilUniv Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USAUniv Estadual Paulista, ICTP South Amer Inst Fundamental Res, Sao Paulo, BrazilUniv Estadual Paulista, Inst Fis Teor, Sao Paulo, BrazilFAPESP: 2016/01343-7FAPESP: 2017/05770-0U. S. Department of Energy: DE-SC0017647National Science Foundation: PHY-1066293SpringerUniversidade Estadual Paulista (Unesp)Univ WisconsinPonton, Eduardo [UNESP]Bai, Yang [UNESP]Jain, Bithika [UNESP]2020-12-10T19:37:55Z2020-12-10T19:37:55Z2019-09-02info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article47http://dx.doi.org/10.1007/JHEP09(2019)011Journal Of High Energy Physics. New York: Springer, n. 9, 47 p., 2019.1029-8479http://hdl.handle.net/11449/19623010.1007/JHEP09(2019)011WOS:000489138800001Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal Of High Energy Physicsinfo:eu-repo/semantics/openAccess2021-10-23T05:17:29Zoai:repositorio.unesp.br:11449/196230Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:09:59.473284Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Electroweak symmetric dark matter balls
title Electroweak symmetric dark matter balls
spellingShingle Electroweak symmetric dark matter balls
Ponton, Eduardo [UNESP]
Beyond Standard Model
Cosmology of Theories beyond the SM
title_short Electroweak symmetric dark matter balls
title_full Electroweak symmetric dark matter balls
title_fullStr Electroweak symmetric dark matter balls
title_full_unstemmed Electroweak symmetric dark matter balls
title_sort Electroweak symmetric dark matter balls
author Ponton, Eduardo [UNESP]
author_facet Ponton, Eduardo [UNESP]
Bai, Yang [UNESP]
Jain, Bithika [UNESP]
author_role author
author2 Bai, Yang [UNESP]
Jain, Bithika [UNESP]
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
Univ Wisconsin
dc.contributor.author.fl_str_mv Ponton, Eduardo [UNESP]
Bai, Yang [UNESP]
Jain, Bithika [UNESP]
dc.subject.por.fl_str_mv Beyond Standard Model
Cosmology of Theories beyond the SM
topic Beyond Standard Model
Cosmology of Theories beyond the SM
description In the simple Higgs-portal dark matter model with a conserved dark matter number, we show that there exists a non-topological soliton state of dark matter. This state has smaller energy per dark matter number than a free particle state and has its interior in the electroweak symmetric vacuum. It could be produced in the early universe from first-order electroweak phase transition and contribute most of dark matter. This electroweak symmetric dark matter ball is a novel macroscopic dark matter candidate with an energy density of the electroweak scale and a mass of 1 gram or above. Because of its electroweak-symmetric interior, the dark matter ball has a large geometric scattering cross section off a nucleon or a nucleus. Dark matter and neutrino experiments with a large-size detector like Xenon1T, BOREXINO and JUNO have great potential to discover electroweak symmetric dark matter balls. We also discuss the formation of bound states of a dark matter ball and ordinary matter.
publishDate 2019
dc.date.none.fl_str_mv 2019-09-02
2020-12-10T19:37:55Z
2020-12-10T19:37:55Z
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/JHEP09(2019)011
Journal Of High Energy Physics. New York: Springer, n. 9, 47 p., 2019.
1029-8479
http://hdl.handle.net/11449/196230
10.1007/JHEP09(2019)011
WOS:000489138800001
url http://dx.doi.org/10.1007/JHEP09(2019)011
http://hdl.handle.net/11449/196230
identifier_str_mv Journal Of High Energy Physics. New York: Springer, n. 9, 47 p., 2019.
1029-8479
10.1007/JHEP09(2019)011
WOS:000489138800001
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.format.none.fl_str_mv 47
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
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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