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arXiv · 0902.0230

Hawking temperature and higher order calculations

Bhramar Chatterjee·P. Mitra
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Abstract

Hawking radiation has recently been explained by using solutions of wave equations across black hole horizons in a WKB approximation. Higher order calculations using both usual and non-singular coordinates are found to change the solution for zero spin, but this change is not an alteration of the Hawking temperature. For spin 1/2, there is no correction to the simplest form of the solution.

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Bhramar Chatterjee, P. Mitra. 2009-04-09. Hawking temperature and higher order calculations. https://doi.org/10.1016/j.physletb.2009.04.009

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