## Massive Dirac quasinormal modes in Schwarzschild-de Sitter black holes: Anomalous decay rate and fine structure

 dc.contributor.author Aragon, Almendra dc.contributor.author Becar, Ramon dc.contributor.author Gonzalez, P. A. dc.contributor.author Vasquez, Yerko dc.date 2021 dc.date.accessioned 2021-04-30T16:47:00Z dc.date.available 2021-04-30T16:47:00Z dc.description.abstract Recently, the anomalous decay rate of quasinormal modes has been studied for some geometries under scalar field perturbations, which occurs when the longest-lived modes are the ones with higher angular number, as well as the existence of a critical scalar field mass, i.e., the value of scalar field mass such that the decay rate does not depend appreciably on the angular number, and beyond which the behavior of the decay rate is inverted. Here, we consider the propagation of fermionic fields in the background of Schwarzschild-de Sitter black holes, and we show that the anomalous decay rate behavior and the fine structure, related to the coupling between the chirality and the mass of the field, can be observed in the fermionic spectrum. dc.identifier.citation PHYSICAL REVIEW D,Vol.103,,2021 dc.identifier.doi 10.1103/PhysRevD.103.064006 dc.identifier.uri http://repositoriodigital.uct.cl/handle/10925/3485 dc.language.iso en dc.publisher AMER PHYSICAL SOC dc.source PHYSICAL REVIEW D dc.title Massive Dirac quasinormal modes in Schwarzschild-de Sitter black holes: Anomalous decay rate and fine structure dc.type Article uct.catalogador WOS uct.indizacion SCI