| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5494549 | Nuclear Physics B | 2016 | 9 Pages |
Abstract
We study the influence of black-hole evaporation on light propagation. The framework employed is based on the non-linear QED effective action at one-loop level. We show that the light-cone condition is modified for low-energy radiation due to black-hole evaporation. We discuss conditions under which the phase velocity of this low-energy radiation is greater than c. We also compute the modified light-deflection angle, which turns out to be significantly different from the standard GR value for black-hole masses in the range MPlâªMâ²1019MPl.
Related Topics
Physical Sciences and Engineering
Mathematics
Mathematical Physics
Authors
Slava Emelyanov,