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- W4220844089 abstract "In this paper, we consider an axially symmetric $(2+1)-$dimensional rotating Banados-Teitelboim-Zanelli (BTZ) black hole to investigate its interior textbf{information}. First, we choose a largest space-like hyper-surface at $r_v=0.45$ and calculate the maximal interior volume bound by it. We found the interior volume to increase with advance time $v$. Similarly, the textbf{scalar} quantum mode entropy textbf{is} also found to increase with advance time. Nexttextbf{,} considering two important assumptions, an evolution relation is obtained between textbf{the variation of scalar} quantum mode entropy and Bekenstein Hawking entropy textbf{for an} infinitesimal interval of time. In contrast to the evolution relation of higher dimensional black holes, the characteristic feature of this relation is its increase with extremely large increase in black hole mass. Moreover, this work extends the notion of black hole evaporation idea to lower space-time dimensions." @default.
- W4220844089 created "2022-04-03" @default.
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- W4220844089 date "2022-03-15" @default.
- W4220844089 modified "2023-09-24" @default.
- W4220844089 title "Entropy variation of rotating BTZ black hole under Hawking radiation" @default.
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- W4220844089 doi "https://doi.org/10.1088/1402-4896/ac5af3" @default.
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