Entropy of Dirac field in a rectilinearly nonuniformly accelerating Kinnersley black hole

Yang Bo

doi:10.7498/aps.56.6772

Abstract
Using the Tortoise coordinate transformation and the Dirac field equation near the event horizon, the Hawking temperature of Kinnersley black hole is obtained. Meanwhile, adopting thin film brick-wall model, the entropy of Kinnersley black hole is calculated. The entropy near the event horizon is shown to be the entropy of black hole by regulating the cut-off parameter and the thin film's thickness properly. The results show that the entropy of the black hole is proportional to the area of the event horizon.

Keywords:
Kinnersley black hole /

Hawking temperature /

thin film brick-wall model /

entropy
Authors and contacts
Yang Bo

1.
重庆三峡学院物理与电子工程学院,万州 404000
References

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Vol. 56, Issue 11 - 2007-06-05

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Entropy of Dirac field in a rectilinearly nonuniformly accelerating Kinnersley black hole

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Entropy of Dirac field in a rectilinearly nonuniformly accelerating Kinnersley black hole

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