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- W2914095041 abstract "With the help of the Bohr--Sommerfeld quantization rule, the area spectrum of a charged, spherically symmetric spacetime is obtained by studying an adiabatic invariant action variable. The period of the Einstein-Maxwell system, which is related to the surface gravity of a given spacetime, is determined by the Kruskal--like coordinates. It is shown that the area spectrum of the Reissner-Nordstr{o}m black hole is evenly spaced and the spacing is the same as that of a Schwarzschild black hole, which indicates that the area spectrum of a black hole is independent of its parameters. In contrast to the quasi-normal mode analysis, we do not impose the small charge limit as the general area gap $8pi $ is obtained." @default.
- W2914095041 created "2019-02-21" @default.
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- W2914095041 date "2012-04-08" @default.
- W2914095041 modified "2023-09-27" @default.
- W2914095041 title "Spectroscopy of a Reissner-Nordstr" @default.
- W2914095041 hasPublicationYear "2012" @default.
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