dc.contributorUniversidade Estadual Paulista (UNESP)
dc.contributorUniversity of Wisconsin-Madison
dc.date.accessioned2022-04-29T08:28:22Z
dc.date.accessioned2022-12-20T02:42:24Z
dc.date.available2022-04-29T08:28:22Z
dc.date.available2022-12-20T02:42:24Z
dc.date.created2022-04-29T08:28:22Z
dc.date.issued2019-09-01
dc.identifierJournal of High Energy Physics, v. 2019, n. 9, 2019.
dc.identifier1029-8479
dc.identifier1126-6708
dc.identifierhttp://hdl.handle.net/11449/228715
dc.identifier10.1007/s13130-019-11194-5
dc.identifier2-s2.0-85071950944
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5408850
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.
dc.languageeng
dc.relationJournal of High Energy Physics
dc.sourceScopus
dc.subjectBeyond Standard Model
dc.subjectCosmology of Theories beyond the SM
dc.titleElectroweak symmetric dark matter balls
dc.typeArtículos de revistas


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