Mapping Hawking temperature in the spinning constant curvature black hole spaces into Unruh temperature

Abstract

We established the equivalence between the local Hawking temperature measured by the time-like Killing observer located at some positions $r$ with finite distances from the outer horizon $r_{+}$ in the 5-dimensional spinning black hole space with both negative and positive constant curvature, and the Unruh temperature measured by the Rindler observer with constant acceleration in the 6-dimensional flat space by employing the globally embedding approach.

11 pages, no figure, accepted by Modern Physics Letters A, match published version

References in corpus (3)

• A New Global Embedding Approach to Study Hawking and Unruh Effects
• Accelerating Branes and Brane Temperature
• Local free-fall temperature of a RN-AdS black hole

Cited by in corpus (4)

• Local free-fall Temperature of GMGHS Black Holes
• Local free-fall temperatures of charged BTZ black holes in massive gravity
• GEMS embeddings of Schwarzschild and RN black holes in Painlevé-Gullstrand spacetimes
• GEMS embeddings of Hayward regular black holes in massless and massive gravities