Calculating the Hawking Temperatures of Conventional Black Holes in the f(R) Gravity Models with the RVB Method

Abstract

This paper attempted to apply the RVB method for calculating the Hawking temperatures of black holes under f(R) gravity. In calculating the Hawking temperature, we found a difference in the integration constant between the RVB and general methods.

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Cited by in corpus (2)

• Extended uncertainty principle and Van der Waals black holes
• Thermodynamic geometric analysis of RN black holes under f(R) gravity