Quantum thermodynamics in the interior of a Schwarzschild black-hole
نویسندگان
چکیده
We study the interior of a Schwarzschild Black-Hole (B-H) using Relativistic Quantum Geometry described in \cite{rb} and \cite{rb1}. found discrete energy levels for scalar field from polynomial condition Heun Confluent functions expanded around radius. From solutions it is obtained that uncertainty principle valid each level space-time, form: $E_n\, r_{sh,n}=\hbar/2$. Temperature, entropy B-H mass are dependent on number states B-H, such Bekenstein-Hawking (BH) results limit case.
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ژورنال
عنوان ژورنال: Physica Scripta
سال: 2021
ISSN: ['1402-4896', '0031-8949']
DOI: https://doi.org/10.1088/1402-4896/abd203