|
| | | | |
| | | |
| Stat |
Members: 3525
Articles: 2'347'340
Articles rated: 2602
01 June 2023 |
|
| | | | |
|
Article overview
| |
|
|
Self-Interaction Correction to Black Hole Radiance | | Per Kraus
; Frank Wilczek
; | | Date: |
2 Aug 1994 | | Journal: | Nucl.Phys. B433 (1995) 403-420 | | Subject: | gr-qc hep-th | | Abstract: | We consider the modification of the formulas for black hole radiation, due to the self-gravitation of the radiation. This is done by truncating the coupled particle-hole system to a small set of modes, that are plausibly the most significant ones, and quantizing the reduced system. In this way we find that the particles no longer move along geodesics, nor is the action along the rays zero for a massless particle. The radiation is no longer thermal, but is corrected in a definite way that we calculate. Our methods can be extended in a straightforward manner to discuss correlations in the radiation, or between incoming particles and the radiation. | | Source: | arXiv, gr-qc/9408003 | | Services: | Forum | Review | PDF | Favorites | |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser CCBot/2.0 (https://commoncrawl.org/faq/)
|
| |
|
|
|
|
News, job offers and information for researchers and scientists:
| |
REGISTER