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Thermodynamics of a class of regular black holes with a generalized uncertainty principle

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arxiv 1801.02661 v2 pith:D3EON3SF submitted 2018-01-08 gr-qc hep-th

Thermodynamics of a class of regular black holes with a generalized uncertainty principle

classification gr-qc hep-th
keywords blackholesclassregularthermodynamicsentropygeneralizedobtained
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In this article, we present a study on thermodynamics of a class of regular black holes. Such a class includes Bardeen and Hayward regular black holes. We obtained thermodynamic quantities like the Hawking temperature, entropy, and heat capacity for the entire class. As part of an effort to indicate some physical observable to distinguish regular black holes from singular black holes, we suggest that regular black holes are colder than singular black holes. Besides, contrary to the Schwarzschild black hole, that class of regular black holes may be thermodynamically stable. From a generalized uncertainty principle, we also obtained the quantum-corrected thermodynamics for the studied class. Such quantum corrections provide a logarithmic term for the quantum-corrected entropy.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraints and Consistency of Rotating Regular Black Hole Thermodynamics

    gr-qc 2026-01 reject novelty 6.0

    For rotating regular black holes, the thermodynamic Hawking temperature is order-dependent under the regularity constraint; only computing in the full phase space before imposing the constraint reproduces the geometri...

  2. Improved unimodular black holes with self-consistent renormalization scale identification

    gr-qc 2026-06 unverdicted novelty 5.0

    Renormalization group improved unimodular black holes with self-consistent radial scale identification yield non-singular metrics and associated mass gaps.

  3. Thermodynamic Phase Transitions and Quantum Entropy Corrections in the Simpson-Visser Regular Black Hole

    gr-qc 2025-12 reject novelty 4.0

    For the Simpson-Visser regular black hole, the heat capacity diverges at a = √2 m, but the claimed quantum entropy corrections are internally inconsistent: the 1/a² term has the wrong sign and the remnant-entropy form...

  4. De Sitter Cores from Nonlocal Quantum Field Theories

    physics.gen-ph 2026-07 conditional novelty 2.0

    An exponential nonlocal regulator maps a point mass to a Gaussian density whose Einstein solution has a de Sitter core, reproducing (with new labeling) the known Gaussian-sourced regular black hole.