Quantum-gravitational trans-Planckian energy of a time-dependent black hole
A. J. Nurmagambetov (Kharkov, KIPT), I. Y. Park (Philander Smith, Coll.)
TL;DR
This paper investigates the quantum-gravitational energy behavior near the horizon of a time-dependent rotating black hole, revealing trans-Planckian energy scaling similar to non-rotating cases, thus advancing understanding of quantum effects in dynamic black holes.
Contribution
It extends previous work on quantum-corrected black holes to include rotation, demonstrating consistent trans-Planckian energy phenomena in more complex, realistic black hole models.
Findings
Trans-Planckian energy scaling near the horizon
Similar behavior in rotating and non-rotating black holes
Quantum effects persist in dynamic, rotating black hole solutions
Abstract
We continue our recent endeavor in which a time-dependent black hole solution of a one-loop quantum-corrected Einstein-scalar system was obtained and its near-horizon behavior was analyzed. The energy analysis led to a trans-Planckian scaling behavior near the event horizon. In the present work the analysis is extended to a rotating black hole solution of an Einstein-Maxwell-scalar system with a Higgs potential. Although the analysis becomes much more complex compared to that of the previous, we observe the same basic features, including the quantum-gravitational trans-Planckian energy near the horizon.
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.