Tortoise coordinate and Hawking effect in the Kinnersley spacetime

Details Tortoise coordinate and Hawking effect in the Kinnersley spacetime Tortoise coordinate and Hawking effect in the Kinnersley spacetime

2010-03-13

arxiv.org/abs/1003.2686v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages

Scientific paper

Hawking effect from the Kinnersley spacetime is investigated using the improved Damour-Ruffini method with a new coordinate transformation. Hawking temperature of the horizons can be obtained point by point. It is found that Hawking temperatures of different points on the horizons are different. Especially, Hawking temperature of Rindler horizon is investigated. The touch between a Kinnersley black hole and its Rindler horizon is considered, and it shows that the phenomenon is related to the third law of thermodynamics.

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