Kerr black hole in canonically deformed space-time
Marcin Daszkiewicz, Cezary J. Walczyk
TL;DR
This paper explores how Kerr black holes behave in a canonically deformed space-time, analyzing their event horizon, ergosphere, temperature, and entropy to understand the effects of space-time deformation.
Contribution
It provides the first detailed analysis of Kerr black holes within a canonically deformed space-time framework, including key thermodynamic and geometric properties.
Findings
Deformed event horizon and ergosphere structures identified.
Temperature and entropy of the deformed black hole calculated.
Implications for black hole thermodynamics in deformed space-time.
Abstract
We investigate the Kerr black hole defined on canonically deformed space-time. Particulary, we find the corresponding event horizon, the ergosphere, the temperature and the entropy of such deformed object.
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