| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10722884 | Physics Letters B | 2011 | 6 Pages |
Abstract
Hawking radiation is studied for arbitrary scalars, fermions and spin-1 bosons, using a tunneling approach, to every order in â but ignoring back-reaction effects. It is shown that the additional quantum terms yield no new contribution to the Hawking temperature. Indeed, it is found that the limit of small â in the standard quantum WKB approximation is replaced by the near-horizon limit in the gravitational WKB approach.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Alexandre Yale,