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Publicação:
Electroweak symmetric dark matter balls

dc.contributor.authorPonton, Eduardo [UNESP]
dc.contributor.authorBai, Yang [UNESP]
dc.contributor.authorJain, Bithika [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionUniv Wisconsin
dc.date.accessioned2020-12-10T19:37:55Z
dc.date.available2020-12-10T19:37:55Z
dc.date.issued2019-09-02
dc.description.abstractIn 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.en
dc.description.affiliationUniv Estadual Paulista, ICTP South Amer Inst Fundamental Res, Sao Paulo, Brazil
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, Sao Paulo, Brazil
dc.description.affiliationUniv Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA
dc.description.affiliationUnespUniv Estadual Paulista, ICTP South Amer Inst Fundamental Res, Sao Paulo, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, Sao Paulo, Brazil
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipU. S. Department of Energy
dc.description.sponsorshipNational Science Foundation
dc.description.sponsorshipMunich Institute for Astro-and Particle Physics (MIAPP) of the DFG cluster of excellence Origin and Structure of the Universe
dc.description.sponsorshipIdFAPESP: 2016/01343-7
dc.description.sponsorshipIdFAPESP: 2017/05770-0
dc.description.sponsorshipIdU. S. Department of Energy: DE-SC0017647
dc.description.sponsorshipIdNational Science Foundation: PHY-1066293
dc.format.extent47
dc.identifierhttp://dx.doi.org/10.1007/JHEP09(2019)011
dc.identifier.citationJournal Of High Energy Physics. New York: Springer, n. 9, 47 p., 2019.
dc.identifier.doi10.1007/JHEP09(2019)011
dc.identifier.issn1029-8479
dc.identifier.urihttp://hdl.handle.net/11449/196230
dc.identifier.wosWOS:000489138800001
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofJournal Of High Energy Physics
dc.sourceWeb of Science
dc.subjectBeyond Standard Model
dc.subjectCosmology of Theories beyond the SM
dc.titleElectroweak symmetric dark matter ballsen
dc.typeArtigo
dcterms.licensehttp://www.springer.com/open+access/authors+rights?SGWID=0-176704-12-683201-0
dcterms.rightsHolderSpringer
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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