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Energy Extraction and Evolution of Regular Black Holes: The Case of Bardeen Spacetime

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arxiv 2508.14489 v1 pith:WJJ4OBPF submitted 2025-08-20 gr-qc

Energy Extraction and Evolution of Regular Black Holes: The Case of Bardeen Spacetime

classification gr-qc
keywords blackregularchargeevaporationholesbardeenenergyevolution
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This paper examines regular black holes, in particular the Bardeen spacetime where singularities are replaced by non-singular cores. It explores the energy extraction through the charged Penrose process and shows that magnetic charge evaporation can drive a regular black hole towards a singularity. Two evaporation models are proposed, dealing with charge loss and combined charge evaporation with mass accretion, providing insights into the evolution and stability of regular black holes.

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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. Families of regular spacetimes and energy conditions

    gr-qc 2026-05 unverdicted novelty 7.0

    A classification of admissible energy density profiles with bounded Kretschmann scalar produces families of regular static spherically symmetric spacetimes in GR, including new closed-form solutions involving hypergeo...

  2. Families of regular spacetimes and energy conditions

    gr-qc 2026-05 unverdicted novelty 7.0

    A classification of admissible energy density profiles with bounded Kretschmann scalar yields a unified framework for regular static spherically symmetric spacetimes satisfying the weak energy condition, recovering kn...

  3. Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes

    gr-qc 2026-01 unverdicted novelty 5.0

    Lorentzian-Euclidean black holes produce excess inner-shadow intensity and accumulate energy at the horizon with backreaction unlike stable light rings.

  4. Regular Black Hole Formation and Gamma-Ray Burst from Matter Conversion

    gr-qc 2026-07 conditional novelty 4.0

    The formation of a regular black hole could release gamma-ray-burst-scale energy only if its singularity-avoiding core is a weak perturbation of Schwarzschild.