Spinors in (anti-) de Sitter Space
V Schaub - Journal of High Energy Physics, 2023 - Springer
A bstract We explore analytical aspects of correlators involving Dirac spinors in d+ 1-
dimensional de Sitter space. Adapting the formalism of Sleight and Taronna, we show how …
dimensional de Sitter space. Adapting the formalism of Sleight and Taronna, we show how …
Analytic formula for quasinormal modes in the near-extreme Kerr-Newman–de Sitter spacetime governed by a non-Pöschl-Teller potential
MS Churilova, RA Konoplya, A Zhidenko - Physical Review D, 2022 - APS
Quasinormal modes of scalar, electromagnetic, and gravitational fields in the extreme
Schwarzschild–de Sitter background are known to be expressed in analytic form as …
Schwarzschild–de Sitter background are known to be expressed in analytic form as …
Quasinormal modes of D-dimensional de Sitter spacetime
A López-Ortega - General Relativity and Gravitation, 2006 - Springer
We calculate the exact values of the quasinormal frequencies for an electromagnetic field
and a gravitational perturbation moving in D-dimensional de Sitter spacetime (D≥ 4). We …
and a gravitational perturbation moving in D-dimensional de Sitter spacetime (D≥ 4). We …
Absorption and quasinormal modes of classical fields propagating on 3D and 4D de Sitter spacetime
A Lopez-Ortega - General Relativity and Gravitation, 2006 - Springer
We extensively study the exact solutions of the massless Dirac equation in 3D de Sitter
spacetime that we published recently. Using the Newman-Penrose formalism, we find exact …
spacetime that we published recently. Using the Newman-Penrose formalism, we find exact …
The Dirac equation in D-dimensional spherically symmetric spacetimes
A Lopez-Ortega - arXiv preprint arXiv:0906.2754, 2009 - arxiv.org
We expound in detail a method frequently used to reduce the Dirac equation in D-
dimensional (D>= 4) spherically symmetric spacetimes to a pair of coupled partial differential …
dimensional (D>= 4) spherically symmetric spacetimes to a pair of coupled partial differential …
Dirac quasinormal modes of D-dimensional de Sitter spacetime
A Lopez-Ortega - General Relativity and Gravitation, 2007 - Springer
We find exact solutions to the Dirac equation in D-dimensional de Sitter spacetime. Using
these solutions we analytically calculate the de Sitter quasinormal (QN) frequencies of the …
these solutions we analytically calculate the de Sitter quasinormal (QN) frequencies of the …
Quasinormal frequencies of a two-dimensional asymptotically anti-de Sitter black hole of the dilaton gravity theory
MI Hernandez-Velazquez… - Frontiers in Astronomy …, 2021 - frontiersin.org
We numerically calculate the quasinormal frequencies of the Klein-Gordon and Dirac fields
propagating in a two-dimensional asymptotically anti-de Sitter black hole of the dilaton …
propagating in a two-dimensional asymptotically anti-de Sitter black hole of the dilaton …
Hawking radiation and Dirac quasinormal modes of 3D EMDΛ black holes
A Lopez-Ortega - General Relativity and Gravitation, 2005 - Springer
Some properties of the Hawking radiation emitted by the family of black holes of the Einstein–
Maxwell–Dilaton with cosmologicalconstant theory in three dimensions found by Chan and …
Maxwell–Dilaton with cosmologicalconstant theory in three dimensions found by Chan and …
Entropy of -dimensional de Sitter black hole to all orders in the Planck length
YW Kim, YJ Park - Physical Review D—Particles, Fields, Gravitation, and …, 2008 - APS
We calculate the statistical entropy of a scalar field on the background of (2+ 1)-dimensional
de Sitter space without an artificial cutoff considering corrections to all orders in the Planck …
de Sitter space without an artificial cutoff considering corrections to all orders in the Planck …
Decay of Dirac fields in the backgrounds of dilatonic black holes
R Becar, S Lepe, J Saavedra - International Journal of Modern …, 2010 - World Scientific
We find an exact solution to the Dirac equation in the background of the dilatonic black hole
in 1+ 1 and 4+ 1 dimensions, and for them we calculate the corresponding quasinormal …
in 1+ 1 and 4+ 1 dimensions, and for them we calculate the corresponding quasinormal …