dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade Federal de São Paulo (UNIFESP)
dc.date.accessioned2018-12-11T17:18:12Z
dc.date.available2018-12-11T17:18:12Z
dc.date.created2018-12-11T17:18:12Z
dc.date.issued2018-02-01
dc.identifierJournal of High Energy Physics, v. 2018, n. 2, 2018.
dc.identifier1029-8479
dc.identifier1126-6708
dc.identifierhttp://hdl.handle.net/11449/175932
dc.identifier10.1007/JHEP02(2018)145
dc.identifier2-s2.0-85042489833
dc.identifier2-s2.0-85042489833.pdf
dc.description.abstractIn this work we use momentum-space techniques to evaluate the propagator G(x, x′) for a spin 1/2 mass dimension one spinor field on a curved Friedmann-Robertson-Walker spacetime. As a consequence, we built the one-loop correction to the effective lagrangian in the coincidence limit. Going further we compute the effective lagrangian in the finite temperature regime. We arrive at interesting cosmological consequences, as time-dependent cosmological ‘constant’, fully explaining the functional form of previous cosmological models.
dc.languageeng
dc.relationJournal of High Energy Physics
dc.relation1,227
dc.relation1,227
dc.rightsAcesso aberto
dc.sourceScopus
dc.subjectCosmology of Theories beyond the SM
dc.subjectEffective Field Theories
dc.subjectThermal Field Theory
dc.titleEffective lagrangian for a mass dimension one fermionic field in curved spacetime
dc.typeArtículos de revistas


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