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August 15, 2026Journal of Physics A Mathematical and TheoreticalOpen Access

Thermodynamic remnants in black-hole evaporation

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Authors

IAIvan ArrautUniversity of Saint JosephAMAbhishek MehtaUniversity of Seoul

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Implication

Theoretical analysis demonstrates black-hole remnants emerge naturally from Hawking's original evaporation computations, indicating extra assumptions are unnecessary.

Key Points

  • To determine whether black-hole remnants arise directly from Hawking's original evaporation framework without requiring additional theoretical assumptions.
  • Re-evaluated the foundational mathematical computations of black-hole evaporation established by Hawking.
  • Analyzed the emergence of remnant states strictly within baseline thermodynamic and quantum mechanical formulations.
  • Showed that the black-hole remnant scenario arises naturally from standard Hawking evaporation calculations.
  • Established that remnant formation requires no supplementary conjectures or modifications to the initial computational framework.

Cite This Study

Arraut et al. (2026) studied this question.

synapsesocial.com/papers/6a80194675c2e31742c85553https://doi.org/10.1088/1751-8121/ae999e
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Also Consider

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  1. 1Topological Remnants of Black Hole Evaporation: From 2D Toy Models to 4D Axionic Wormholes and Dark Matter2026
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