Abstract
AbstractThe 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 is used in the thermo field dynamics 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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