Surface Area Products for Kerr-Taub-NUT Space-time
Parthapratim Pradhan

TL;DR
This paper investigates the thermodynamic properties of Kerr-Taub-NUT black holes, revealing non-universal area and entropy products due to NUT charge and topological singularities, and explores their implications for black hole entropy understanding.
Contribution
It provides new insights into the thermodynamics of Kerr-Taub-NUT black holes, highlighting deviations from standard laws caused by NUT charge and topological features.
Findings
Area and entropy products are mass-dependent and non-universal.
First law and Smarr relations do not hold for Lorentzian TN and KTN black holes.
Mass formulas are derived for TN and KTN black holes.
Abstract
We examine properties of the inner and outer horizon thermodynamics of Taub-NUT (Newman-Unti-Tamburino) and Kerr-Taub-NUT (KTN) black hole (BH) in four dimensional \emph{Lorentzian geometry}. We compare and contrasted these properties with the properties of Reissner Nordstr{\o}m (RN) BH and Kerr BH. We focus on "area product", "entropy product", "irreducible mass product" of the event horizon and Cauchy horizons. Due to mass-dependence, we speculate that these products have no beautiful quantization feature. Nor does it has any universal property. We further observe that the \emph{First law} of BH thermodynamics and \emph {Smarr-Gibbs-Duhem} relations do not hold for Taub-NUT (TN) and KTN BH in Lorentzian regime. The failure of these aforementioned features are due to presence of the non-trivial NUT charge which makes the space-time to be asymptotically non-flat, in contrast with RN BH…
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