UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox
Fuente:
arXiv
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Format: | Preprint |
| Veröffentlicht: |
2024
|
| Schlagworte: | |
| Online-Zugang: | |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| _version_ | 1866908952944443392 |
|---|---|
| author | Ho, Pei-Ming Kawai, Hikaru Shao, Wei-Hsiang |
| author_facet | Ho, Pei-Ming Kawai, Hikaru Shao, Wei-Hsiang |
| contents | This chapter suggests an alternative solution to the black-hole information paradox by proposing that Hawking radiation ceases around the scrambling time due to trans-Planckian effects inherent in string theory. We consider two toy models in the literature that incorporate stringy effects. The first model utilizes the generalized uncertainty principle, which introduces a minimal length. The second model is inspired by string field theory, where interactions are exponentially suppressed in the UV limit. Both models indicate an early termination of Hawking radiation around the scrambling time, resulting in negligible evaporated energy and a predominantly classical black hole. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2411_01105 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox Ho, Pei-Ming Kawai, Hikaru Shao, Wei-Hsiang High Energy Physics - Theory This chapter suggests an alternative solution to the black-hole information paradox by proposing that Hawking radiation ceases around the scrambling time due to trans-Planckian effects inherent in string theory. We consider two toy models in the literature that incorporate stringy effects. The first model utilizes the generalized uncertainty principle, which introduces a minimal length. The second model is inspired by string field theory, where interactions are exponentially suppressed in the UV limit. Both models indicate an early termination of Hawking radiation around the scrambling time, resulting in negligible evaporated energy and a predominantly classical black hole. |
| title | UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox |
| topic | High Energy Physics - Theory |
| url | https://arxiv.org/abs/2411.01105 |