The GEMS Approach to Stationary Motions in the Spherically Symmetric Spacetimes
arXiv:gr-qc/0409107 · doi:10.1088/1126-6708/2004/10/011
Abstract
We generalize the work of Deser and Levin on the unified description of Hawking radiation and Unruh effect to general stationary motions in spherically symmetric black holes. We have also matched the chemical potential term of the thermal spectrum of the two sides for uncharged black holes.
Latex file, 12 pages, no figure; v2: typos fixed; v3: minor corrections, final version published in JHEP