Black hole shadow and chaos bound violation in f(T) teleparallel gravity
Mar 3, 2023
5 pages
Published in:
- Phys.Lett.B 839 (2023) 137828
- Published: Apr 10, 2023
e-Print:
- 2303.01956 [gr-qc]
DOI:
- 10.1016/j.physletb.2023.137828 (publication)
View in:
Citations per year
Abstract: (Elsevier B.V.)
We show that the so-called chaos bound, proposed by Maldacena, Shenker & Stanford, can be violated in teleparallel gravity. In particular, it is possible to select a new gravitational Lyapunov parameter, controlling chaotization of circular trajectories, in black hole photo-sphere, that can exceed the Maldacena, Shenker & Stanford thermal bound. This feature alters the standard quasi-normal modes and ringdown phase after black hole merging with intriguing implications for future gravitational wave detections and black hole shadow measurements. It is a general characteristic for several gravitational theories beyond standard General Relativity.Note:
- 5 pages, 1 figure, accepted for publication in Physics Letters B
- gravitation: teleparallel
- black hole
- chaos
- trajectory
- general relativity
- thermal
- gravitational radiation
- shadowing
- gravitation: f(T)
- Lyapunov exponent
References(38)
Figures(1)
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