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Use este identificador para citar ou linkar para este item: http://repositorio.ufla.br/jspui/handle/1/50172
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Campo DCValorIdioma
dc.creatorSantos, Luis C. N.-
dc.creatorMota, Clésio E.-
dc.creatorSilva, Franciele M. da-
dc.creatorGrams, Guilherme-
dc.creatorLobo, Iarley P.-
dc.date.accessioned2022-06-09T22:14:08Z-
dc.date.available2022-06-09T22:14:08Z-
dc.date.issued2021-11-
dc.identifier.citationSANTOS, L. C. N. et al. Effects of modified dispersion relations on free Fermi gas: Equations of state and applications in astrophysics. Physics Letters B, [S.I.], v. 822, 136684, Nov. 2021. DOI: https://doi.org/10.1016/j.physletb.2021.136684.pt_BR
dc.identifier.urihttp://repositorio.ufla.br/jspui/handle/1/50172-
dc.description.abstractDeformed dispersion relations are considered in the study of equations of state of Fermi gas with applications to compact objects. Different choices of deformed energy relations are used in the formulation of our model. As a first test, we consider a relativistic star with a simple internal structure. The mass-radius diagrams obtained suggest a positive influence of deformed Fermi gas, depending of the functions employed. In addition, we comment on how realistic equations of state, in which interactions between nucleons are taken into account, can be addressed.pt_BR
dc.languageenpt_BR
dc.publisherElsevierpt_BR
dc.rightsacesso abertopt_BR
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.sourcePhysics Letters Bpt_BR
dc.subjectFermi gaspt_BR
dc.subjectRelationspt_BR
dc.subjectRelativistic starspt_BR
dc.subjectGás de Fermipt_BR
dc.subjectAstrofísicapt_BR
dc.subjectEstrelas relativísticaspt_BR
dc.titleEffects of modified dispersion relations on free Fermi gas: Equations of state and applications in astrophysicspt_BR
dc.typeArtigopt_BR
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