Authors: Shihong Tong
Publish Date: 2015/07/02
Volume: 55, Issue: 2, Pages: 854-860
Abstract
By using dimensional reduction and consistent anomaly method we calculate the Hawking flux of the spin 3/2 field in the Kerr black hole background The results confirm that the Hawking radiation doesn’t depends on the detail of the fields living near the horizon at least at the semiclassical level The Hawking temperature is an universality character of black hole which only depends on the information of the horizon Our calculation agrees with earlier results obtained by the WKB/tunneling method Yale and Mann Phys Lett B 6732 168–172 2009
Keywords: