Thermodynamic phase transitions and quantum entropy corrections in the Simpson–Visser regular black hole.

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Title: Thermodynamic phase transitions and quantum entropy corrections in the Simpson–Visser regular black hole.
Authors: Joshi, Vinayak1 (AUTHOR) vinayak_j@ph.iitr.ac.in, Joshi, Ashok B.2,3 (AUTHOR) gen.rel.joshi@gmail.com
Source: European Physical Journal C -- Particles & Fields. May2026, Vol. 86 Issue 5, p1-12. 12p.
Subjects: Phase transitions, Quantum entropy, Hawking radiation, Black holes
Abstract: Regular black holes offer a compelling framework to explore the consequences of resolving the central singularity of standard black holes. Using the Simpson–Visser "black-bounce" geometry as an elegant, analytically tractable framework, we explore the intricate thermodynamic behavior in such models. We demonstrate that this regular spacetime exhibits a critical instability, marked by a phase transition where the heat capacity is discontinuous. This transition signals a fundamental change in the black hole's evaporation state, which depends on the regularization parameter. Pushing beyond the semiclassical limit, we then derive the leading-order quantum corrections to the entropy via the Hamilton–Jacobi tunneling formalism. Our analysis provides a refined statistical basis for the entropy of non-singular spacetimes and offers a quantitative analysis of the nature of the black hole end-state. These results reveal that singularity resolution is not merely a geometric modification but a profound thermodynamic event, with direct implications for the stability and ultimate fate of evaporating black holes. [ABSTRACT FROM AUTHOR]
Copyright of European Physical Journal C -- Particles & Fields is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Thermodynamic phase transitions and quantum entropy corrections in the Simpson–Visser regular black hole.
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  Data: <searchLink fieldCode="AR" term="%22Joshi%2C+Vinayak%22">Joshi, Vinayak</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> vinayak_j@ph.iitr.ac.in</i><br /><searchLink fieldCode="AR" term="%22Joshi%2C+Ashok+B%2E%22">Joshi, Ashok B.</searchLink><relatesTo>2,3</relatesTo> (AUTHOR)<i> gen.rel.joshi@gmail.com</i>
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  Data: <searchLink fieldCode="JN" term="%22European+Physical+Journal+C+--+Particles+%26+Fields%22">European Physical Journal C -- Particles & Fields</searchLink>. May2026, Vol. 86 Issue 5, p1-12. 12p.
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  Data: <searchLink fieldCode="DE" term="%22Phase+transitions%22">Phase transitions</searchLink><br /><searchLink fieldCode="DE" term="%22Quantum+entropy%22">Quantum entropy</searchLink><br /><searchLink fieldCode="DE" term="%22Hawking+radiation%22">Hawking radiation</searchLink><br /><searchLink fieldCode="DE" term="%22Black+holes%22">Black holes</searchLink>
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  Label: Abstract
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  Data: Regular black holes offer a compelling framework to explore the consequences of resolving the central singularity of standard black holes. Using the Simpson–Visser "black-bounce" geometry as an elegant, analytically tractable framework, we explore the intricate thermodynamic behavior in such models. We demonstrate that this regular spacetime exhibits a critical instability, marked by a phase transition where the heat capacity is discontinuous. This transition signals a fundamental change in the black hole's evaporation state, which depends on the regularization parameter. Pushing beyond the semiclassical limit, we then derive the leading-order quantum corrections to the entropy via the Hamilton–Jacobi tunneling formalism. Our analysis provides a refined statistical basis for the entropy of non-singular spacetimes and offers a quantitative analysis of the nature of the black hole end-state. These results reveal that singularity resolution is not merely a geometric modification but a profound thermodynamic event, with direct implications for the stability and ultimate fate of evaporating black holes. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of European Physical Journal C -- Particles & Fields is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1140/epjc/s10052-026-15763-4
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      – Code: eng
        Text: English
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      – SubjectFull: Phase transitions
        Type: general
      – SubjectFull: Quantum entropy
        Type: general
      – SubjectFull: Hawking radiation
        Type: general
      – SubjectFull: Black holes
        Type: general
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      – TitleFull: Thermodynamic phase transitions and quantum entropy corrections in the Simpson–Visser regular black hole.
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              Text: May2026
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              Y: 2026
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