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Is instability near a black hole key for ”thermalization” of its horizon?
We put forward an attempt towards building a possible theoretical model to understand the observer dependent thermalization of black hole horizon. The near horizon Hamiltonian for a massless, chargeless particle is xp type. This is unstable in nature and so the horizon can induce instability in a sy...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Springer US
2022
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9395861/ https://www.ncbi.nlm.nih.gov/pubmed/36035890 http://dx.doi.org/10.1007/s10714-022-02975-8 |