2019
DOI: 10.1088/0253-6102/71/3/307
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Entropy Quantization of Schwarzschild Black Hole

Abstract: The surface gravity of Schwarzschild black hole can be quantized from the test particle moving around different energy states analog to the Bohr’s atomic model. We have quantized the Hawking temperature and entropy of Schwarzschild black hole from quantization of surface gravity. We also have shown that the change of entropy reduces to zero when the boundary shrinks to very small size.

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Cited by 3 publications
(1 citation statement)
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“…Instead, Kothawala et al [125], Skákala [126,127], Maggiore [128], Liu et al [129], Ren et al [130], Yu and Qi [131] and Bakshi et al [132] argued for a horizon entropy quantum of 2πk. Corishi et al [133,134] proposed 2γ 0 k ln 3, where the Barbero-Immirzi parameter γ 0 is unspecified, Sakalli et al [135] and Rahman [136][137][138] deduced more complex expressions. Liao and Shou-Yong [139] deduced 2πk/3, and Jiang [140] and Aldrovandi and Pereira [141] deduced the value k. The list is not exhaustive but gives an impression of the situation.…”
Section: Black Hole Horizonsmentioning
confidence: 99%
“…Instead, Kothawala et al [125], Skákala [126,127], Maggiore [128], Liu et al [129], Ren et al [130], Yu and Qi [131] and Bakshi et al [132] argued for a horizon entropy quantum of 2πk. Corishi et al [133,134] proposed 2γ 0 k ln 3, where the Barbero-Immirzi parameter γ 0 is unspecified, Sakalli et al [135] and Rahman [136][137][138] deduced more complex expressions. Liao and Shou-Yong [139] deduced 2πk/3, and Jiang [140] and Aldrovandi and Pereira [141] deduced the value k. The list is not exhaustive but gives an impression of the situation.…”
Section: Black Hole Horizonsmentioning
confidence: 99%