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• W3100807970 endingPage "30003" @default.
• W3100807970 startingPage "30003" @default.
• W3100807970 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 and Kerr BH. The another reason of the failure is that Lorentzian TN and Lorentzian KTN geometry contains emph{Dirac-Misner type singularity}, which is a manifestation of a non-trivial topological twist of the manifold. The black hole emph{mass formula} and emph{Christodoulou-Ruffini mass formula} for TN and KTN BHs are also computed. This thermodynamic product formulae gives us further understanding to the nature of BH entropy (inner and outer) at the microscopic level." @default.
• W3100807970 created "2020-11-23" @default.
• W3100807970 creator A5026583379 @default.
• W3100807970 date "2016-08-01" @default.
• W3100807970 modified "2023-09-26" @default.
• W3100807970 title "Surface area products for Kerr-Taub-NUT space-time" @default.
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• W3100807970 doi "https://doi.org/10.1209/0295-5075/115/30003" @default.
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