Rotating black holes in semiclassical gravity
arXiv:2305.10382 · doi:10.1103/PhysRevD.108.L061502
Abstract
We present analytic stationary and axially-symmetric black hole solutions to the semiclassical Einstein equations that are sourced by the trace anomaly. We also find that the same spacetime geometry satisfies the field equations of a subset of Horndeski theories featuring a conformally coupled scalar field. We explore various properties of these solutions, and determine the domain of existence of black holes. These black holes display distinctive features, such as non-circularity, a non-spherically symmetric event horizon and violations of the Kerr bound.
5 pages, 2 figures. v2: references added, expanded discussion
References in corpus (16)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- Spontaneously scalarised Kerr black holes
- On Taking the limit of Gauss-Bonnet Gravity: Theory and Solutions
- The 4D Einstein-Gauss-Bonnet Theory of Gravity: A Review
- Kerr Black Holes are Not Unique to General Relativity
- Macroscopic Effects of the Quantum Trace Anomaly
- Thermodynamics of Conformal Anomaly Corrected Black Holes in AdS Space
- Gravity with a generalized conformal scalar field: Theory and solutions
- Stress Tensor from the Trace Anomaly in Reissner-Nordstrom Spacetimes
- Disformal transformation of stationary and axisymmetric solutions in modified gravity
- Exploring the Small Mass Limit of Stationary Black Holes in Theories with Gauss-Bonnet Terms
- Newman-Janis algorithm's application to regular black hole models
- Selecting Horndeski theories without apparent symmetries and their black hole solutions
- Conformally coupled scalar in Lovelock theory
- Black holes in a new gravitational theory with trace anomalies
Cited by in corpus (7)
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- Kerr-Vaidya type radiating black holes in semi-classical gravity with conformal anomaly
- Properties of general stationary axisymmetric spacetimes: circularity and beyond
- Lensing Stability and Scattering Phenomena in Anisotropic Black Hole Spacetimes in Plasma
- Analytical calculation of Kerr and Kerr-Ads black holes in theory
- Trace anomaly contributions to semi-classical wormhole geometries