On Thermodynamics of Kerr Black Hole

A. F. Santos; E. P. Spaniol; Faqir C. Khanna; S. C. Ulhoa

On Thermodynamics of Kerr Black Hole

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arxiv 2306.02950 v1 pith:O65P5F7S submitted 2023-06-05 gr-qc

S. C. Ulhoa , A. F. Santos , E. P. Spaniol , Faqir C. Khanna This is my paper · ORCID

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The gravitational Stefan-Boltzmann law is considered for the Kerr black hole in the weak-field limit. The energy-momentum tensor predicted by Teleparallelism Equivalent to General Relativity (TEGR) is used in the Thermo Field Dynamics (TFD) formalism to thermalize the field. A temperature-dependent gravitational pressure is obtained. Regions of divergent heat capacity are observed. According to Landau theory, it allows the existence of distinct phases around the Kerr black hole.

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Bhabha-like scattering in the Rarita-Schwinger model at finite temperature
hep-th 2024-12 reject novelty 4.0 of 10

For a massive Rarita-Schwinger spin-3/2 fermion coupled to photons, the tree-level Bhabha-like differential cross-section is derived at finite temperature, with a claimed T squared high-temperature growth.

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