Degeneracy pressure of mass dimension one fermionic fields and the dark matter halo of galaxies

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dc.contributor.authorPereira, S. H. [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2023-03-01T20:41:46Z
dc.date.available2023-03-01T20:41:46Z
dc.date.issued2022-05-01
dc.description.abstractIn this paper, the recently proposed mass dimension one fermionic field is supposed to be responsible for the dark matter (DM) halo around galactic nuclei, through the quantum degeneracy pressure effect of the field. It will be shown that the mass-ratio relation for dwarf galaxies can be well explained for a particle DM mass of about 100-200eV. For a large galaxy, as Milky Way, the observational data for rotation curve can be well reproduced for a particle mass of about 23eV, with the addition of other substructures.en
dc.description.affiliationDepartamento de Física Faculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista (UNESP), Av. Dr. Ariberto Pereira da Cunha 333
dc.description.affiliationUnespDepartamento de Física Faculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista (UNESP), Av. Dr. Ariberto Pereira da Cunha 333
dc.identifierhttp://dx.doi.org/10.1142/S0218271822500560
dc.identifier.citationInternational Journal of Modern Physics D, v. 31, n. 7, 2022.
dc.identifier.doi10.1142/S0218271822500560
dc.identifier.issn0218-2718
dc.identifier.scopus2-s2.0-85129966131
dc.identifier.urihttp://hdl.handle.net/11449/240982
dc.language.isoeng
dc.relation.ispartofInternational Journal of Modern Physics D
dc.sourceScopus
dc.subjectDark matter
dc.subjectdegeneracy pressure
dc.subjectmass dimension one fermionic field
dc.titleDegeneracy pressure of mass dimension one fermionic fields and the dark matter halo of galaxiesen
dc.typeArtigo
unesp.author.orcid0000-0001-9471-583X[1]

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