The Entropy of the Complex Scalar Field in a Charged Kerr Black Hole
msra(1996)
摘要
By using the brick wall method we calculate the thermodynamic potential of
the complex scalar field in a charged Kerr black hole. Using it we show that in
the Hartle-Hawking state the leading term of the entropy is proportional to
$\frac{ A _H}{\epsilon^2}$, which becomes divergent as the system approaches
the black hole horizon. The origin of the divergence is that the density of
states diverges at the horizon.
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关键词
scalar field,density of state,thermodynamics,black hole
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