Publicação: Electroweak symmetric dark matter balls
dc.contributor.author | Ponton, Eduardo [UNESP] | |
dc.contributor.author | Bai, Yang [UNESP] | |
dc.contributor.author | Jain, Bithika [UNESP] | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.contributor.institution | Univ Wisconsin | |
dc.date.accessioned | 2020-12-10T19:37:55Z | |
dc.date.available | 2020-12-10T19:37:55Z | |
dc.date.issued | 2019-09-02 | |
dc.description.abstract | 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. | en |
dc.description.affiliation | Univ Estadual Paulista, ICTP South Amer Inst Fundamental Res, Sao Paulo, Brazil | |
dc.description.affiliation | Univ Estadual Paulista, Inst Fis Teor, Sao Paulo, Brazil | |
dc.description.affiliation | Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA | |
dc.description.affiliationUnesp | Univ Estadual Paulista, ICTP South Amer Inst Fundamental Res, Sao Paulo, Brazil | |
dc.description.affiliationUnesp | Univ Estadual Paulista, Inst Fis Teor, Sao Paulo, Brazil | |
dc.description.sponsorship | Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) | |
dc.description.sponsorship | U. S. Department of Energy | |
dc.description.sponsorship | National Science Foundation | |
dc.description.sponsorship | Munich Institute for Astro-and Particle Physics (MIAPP) of the DFG cluster of excellence Origin and Structure of the Universe | |
dc.description.sponsorshipId | FAPESP: 2016/01343-7 | |
dc.description.sponsorshipId | FAPESP: 2017/05770-0 | |
dc.description.sponsorshipId | U. S. Department of Energy: DE-SC0017647 | |
dc.description.sponsorshipId | National Science Foundation: PHY-1066293 | |
dc.format.extent | 47 | |
dc.identifier | http://dx.doi.org/10.1007/JHEP09(2019)011 | |
dc.identifier.citation | Journal Of High Energy Physics. New York: Springer, n. 9, 47 p., 2019. | |
dc.identifier.doi | 10.1007/JHEP09(2019)011 | |
dc.identifier.issn | 1029-8479 | |
dc.identifier.uri | http://hdl.handle.net/11449/196230 | |
dc.identifier.wos | WOS:000489138800001 | |
dc.language.iso | eng | |
dc.publisher | Springer | |
dc.relation.ispartof | Journal Of High Energy Physics | |
dc.source | Web of Science | |
dc.subject | Beyond Standard Model | |
dc.subject | Cosmology of Theories beyond the SM | |
dc.title | Electroweak symmetric dark matter balls | en |
dc.type | Artigo | |
dcterms.license | http://www.springer.com/open+access/authors+rights?SGWID=0-176704-12-683201-0 | |
dcterms.rightsHolder | Springer | |
dspace.entity.type | Publication | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |