| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1852495 | Physics Letters B | 2016 | 5 Pages |
Abstract
We present evidence for the existence of a quantum lower bound on the Bekenstein–Hawking temperature of black holes. The suggested bound is supported by a gedanken experiment in which a charged particle is dropped into a Kerr black hole. It is proved that the temperature of the final Kerr–Newman black-hole configuration is bounded from below by the relation TBH×rH>(ħ/rH)2TBH×rH>(ħ/rH)2, where rHrH is the horizon radius of the black hole.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Shahar Hod,