Extended Tsallis-Cirto entropy for black and white holes
G.E. Volovik

TL;DR
This paper extends the non-extensive Tsallis-Cirto entropy framework to white holes, revealing their negative entropy and symmetry with black holes, and applies this to Reissner-Nordström black holes and Planck-scale black hole models.
Contribution
It introduces a novel extension of Tsallis-Cirto entropy to white holes, incorporating negative entropy and preserving the composition rule, thus broadening the thermodynamic understanding of black and white holes.
Findings
White hole entropy is negative and antisymmetric to black hole entropy.
The non-extensive composition rule applies to white holes with an entropy modulus.
Reissner-Nordström black hole entropy includes positive outer and negative inner horizon contributions.
Abstract
In reference [1] we considered the black hole thermodynamics with the non-extensive entropy. This entropy obeys the composition rule which coincides with the composition rule in the non-extensive Tsallis-Cirto statistics. Here we extend this approach to the thermodynamics of white holes. The entropy of the white hole is negative as follows from the rate of macroscopic quantum tunneling from black hole to white hole. The white hole entropy is with the minus sign the entropy of the black hole with the same mass, . This reflects the anti-symmetry with respect to time reversal, at which the shift vector in the Arnowitt-Deser-Misner formalism changes sign. This symmetry allows one to extend the Tsallis-Chirto entropy by adding a minus sign to the Tsallis-Chirto formula applied to white hole. As a result, the composition rule remains the same, with the…
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