What kinds of coordinate can keep the Hawking temperature invariant for the static spherically symmetric black hole?

Abstract

By studying the Hawking radiation of the most general static spherically symmetric black hole arising from scalar and Dirac particles tunnelling, we find the Hawking temperature is invariant in the general coordinate representation (\ref{arbitrary1}), which satisfies two conditions: a) its radial coordinate transformation is regular at the event horizon; and b) there is a time-like Killing vector.

10 pages

References in corpus (4)

• Fermions Tunnelling from Black Holes
• Tunnelling, Temperature and Taub-NUT Black Holes
• Hawking temperature from tunnelling formalism
• Entropy of the Schwarzschild-de Sitter Black Hole due to arbitrary spin fields in different Coordinates

Cited by in corpus (5)

• Fermions tunnelling from the charged dilatonic black holes
• Einstein-Gauss-Bonnet gravity coupled to bumblebee field in four dimensional spacetime
• Quantum corrections and black hole spectroscopy
• Back reaction, emission spectrum and entropy spectroscopy
• High dimensional AdS-like black hole and Phase transition in Einstein-bumblebee gravity