Stress tensor for extreme 2D dilatonic Reissner-Nordstrom black holes
arXiv:hep-th/0503090 · doi:10.1103/PhysRevD.72.024015
Abstract
We calculate the expectation value of the stress energy tensor for a massless dilaton-coupled 2D scalar field propagating on an extremal Reissner-Nordstrom black hole formed by the collapse of a timelike shell, showing its regularity on the horizon.
4 pages, latex
References in corpus (1)
Cited by in corpus (5)
- Hawking radiation from extremal and non-extremal black holes
- Reissner-Nordström geometry counterpart in semiclassical gravity
- Some general properties of the renormalized stress-energy tensor for static quantum states on (n+1)-dimensional spherically symmetric black holes
- The Unruh vacuum and the in-vacuum in the Reissner-Nordström spacetime
- Regularity of the stress-energy tensor for extremal Reissner-Nordstrom black holes