Hawking radiation in a Rotating Kaluza-Klein Black Hole with Squashed Horizons
Songbai Chen, Bin Wang, Ru-Keng Su

TL;DR
This paper investigates how extra dimensions influence Hawking radiation in rotating Kaluza-Klein black holes with squashed horizons, revealing that rotation and extra dimensions can enhance radiation, potentially aiding detection.
Contribution
It demonstrates the impact of rotation and extra dimensions on Hawking radiation, providing insights into detecting extra dimensions through black hole emissions.
Findings
Rotation enriches the physics of Hawking radiation.
Extra dimensions can significantly enhance Hawking radiation.
The size of extra dimensions affects radiation detectability.
Abstract
We explore the signature of the extra dimension in the Hawking radiation in a rotating Kaluza-Klein black hole with squashed horizons. Comparing with the spherical case, we find that the rotating parameter brings richer physics. We obtain the appropriate size of the extra dimension which can enhance the Hawking radiation and may open a window to detect the extra dimensions.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
