Cosmography of KNdS Black Holes and Isentropic Phase Transitions
James McInerney, Gautam Satishchandran, Jennie Traschen

TL;DR
This paper analyzes Kerr-Newman-deSitter black holes using observable thermodynamic quantities, revealing phase transitions, degeneracies, and a critical point where high and low density phases merge, enhancing understanding of black hole thermodynamics.
Contribution
It introduces a new parameterization using the area product X, simplifies thermodynamic functions, and uncovers isentropic pairs and phase transition phenomena in KNdS black holes.
Findings
Identification of a physical parameter space with unique and degenerate regions.
Discovery of isentropic pairs of black holes with different X values.
Divergence of compressibility at the maximal entropy point indicating a phase transition.
Abstract
We present a new analysis of Kerr-Newman-deSitter black holes in terms of thermodynamic quantities that are defined in the observable portion of the universe; between the black hole and cosmological horizons. In particular, we replace the mass with a new 'area product' parameter . The physical region of parameter space is found analytically and thermodynamic quantities are given by simple algebraic functions of these parameters. We find that different geometrical properties of the black holes are usefully distinguished by the sum of the black hole and cosmological entropies. The physical parameter space breaks into a region in which the total entropy, together with , and uniquely specifies the black hole, and a region in which there is a two-fold degeneracy. In this latter region, there are isentropic pairs of black holes, having the same , , and ,…
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