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Quantum Corrections to the Entropy of a Barriola-Vilenkin Black Hole due to Spin Fields |
LI Zhong-Heng |
Department of Physics, Zhanjiang Normal College, Zhanjiang 524048 |
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Cite this article: |
LI Zhong-Heng 2000 Chin. Phys. Lett. 17 396-397 |
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Abstract The radial parts of the gravitational, electromagnetic, neutrino, and massless scalar fields in Barriola-Vilenkin spacetime are transformed to the form of the Teukolsky-type master equation. The first quantum corrections to the entropy of the black hole due to the spin fields are calculated by using the brick wall model. It is shown that the contribution of any one of the spin fields is quadratically divergent at the event horizon and is proportional to the surface area of the event horizon.
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Keywords:
04.70.Dy
04.62.+v
97.60.Lf
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Published: 01 June 2000
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PACS: |
04.70.Dy
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(Quantum aspects of black holes, evaporation, thermodynamics)
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04.62.+v
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(Quantum fields in curved spacetime)
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97.60.Lf
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(Black holes)
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