The effect of Rényi entropy on Hawking radiation
نویسندگان
چکیده
Abstract It is widely believed that Hawking radiation originates from excitations near the horizons of black holes (Hawking in Commun Math Phys 43:199, 1975, Giddings Lett B 754:39, 2016, Mathur Class Quantum Gravity 26:224001, 2009). However, (Phys 2016) proposed spectrum characterizes evaporating semi-classical a quantum “atmosphere”, which extends beyond horizon hole. Although several research projects have been conducted this field, they not yet taken into account effect Rényi entropy. In present article, we will therefore consider entropy on power. We assume if very small, suggest should originate “atmosphere” hole’s for finite dimensions. That is, Giddings’ suggestion more likely above possibilities. infinite dimensions, both suggestions are equally credible. briefly large power as well. find and $$\omega /T_{BH}$$ ω / T BH then spectral density $$S_R$$ S R proportional to $$S_{BH}$$ .
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ژورنال
عنوان ژورنال: General Relativity and Gravitation
سال: 2022
ISSN: ['0001-7701', '1572-9532']
DOI: https://doi.org/10.1007/s10714-021-02896-y