Renormalized Vacuum Polarization and Stress Tensor on the Horizon of a Schwarzschild Black Hole Threaded by a Cosmic String
arXiv:1010.3943 · doi:10.1088/0264-9381/28/1/015007
Abstract
We calculate the renormalized vacuum polarization and stress tensor for a massless, arbitrarily coupled scalar field in the Hartle-Hawking vacuum state on the horizon of a Schwarzschild black hole threaded by an infinte straight cosmic string. This calculation relies on a generalized Heine identity for non-integer Legendre functions which we derive without using specific properties of the Legendre functions themselves.
This is an expanded version of a previous submission, we have added the calculation of the stress tensor. 28 pages, 7 figures
References in corpus (2)
Cited by in corpus (4)
- Versatile method for renormalized stress-energy computation in black-hole spacetimes
- Fermionic vacuum polarization by a flat boundary in cosmic string spacetime
- Induced fermionic currents in de Sitter spacetime in the presence of a compactified cosmic string
- Vacuum Polarization of STU Black Holes and their Subtracted Geometry Limit