The renormalized charged scalar current in the Reissner-Nordström-de Sitter spacetime
arXiv:2104.06005 · doi:10.1103/PhysRevD.104.025009
Abstract
We perform a Hadamard point-split renormalization of the current density of a charged scalar field in a Reissner-Nordström-de Sitter spacetime. We compute numerically the expectation values of the components and in the Unruh state in the exterior region and study their dependence on the field parameters and the position.
12 pages, 5 figures, version as accepted for PRD
References in corpus (7)
- Quasinormal modes and Strong Cosmic Censorship
- Stability of Reissner-Nordström black hole in de Sitter background under charged scalar perturbation
- Charged scalar field instability between the event and cosmological horizons
- Mode-sum regularization of in the angular-splitting method
- Two-point function of a quantum scalar field in the interior region of a Reissner-Nordstrom black hole
- Quantum superradiance on static black hole space-times
- The current density in quantum electrodynamics in external potentials
Cited by in corpus (7)
- Quantum (dis)charge of black hole interiors
- Quantization of a charged scalar field on a charged black hole background
- Infinite quantum twisting at the Cauchy horizon of rotating black holes
- Strong Cosmic Censorship and Eigenvalue Repulsions for rotating de Sitter black holes in higher-dimensions
- Immortality through the dark forces: Dark-charge primordial black holes as dark matter candidates
- Computation of and quantum fluxes at the polar interior of a spinning black hole
- Quantum kicks near a Cauchy horizon