Stringy forces in the black hole interior
Abstract Effective field theories break down inside large black holes on macroscopic scales when tidal forces are string-sized. If r 0 is the horizon radius and α′ is the square of the string scale, the 4D Schwarzschild interior is strongly curved at (r 0 α ′)1/3. Infalling massless probes that reac...
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| Auteur principal: | |
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| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
SpringerOpen
2024-11-01
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| Collection: | Journal of High Energy Physics |
| Sujets: | |
| Accès en ligne: | https://doi.org/10.1007/JHEP11(2024)063 |
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