Matter Accretion Versus Semiclassical Bounce in Schwarzschild Interior
We discuss the properties of the previously constructed model of a Schwarzschild black hole interior where the singularity is replaced by a regular bounce, ultimately leading to a white hole. We assume that the black hole is young enough so that the Hawking radiation may be neglected. The model is s...
Tallennettuna:
| Päätekijät: | , , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
MDPI AG
2020-10-01
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| Sarja: | Universe |
| Aiheet: | |
| Linkit: | https://www.mdpi.com/2218-1997/6/10/178 |
| Tagit: |
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