Bertotti-Robinson Geometry and Supersymmetry
Sergio Ferrara
TL;DR
This paper explores how Bertotti-Robinson geometry influences the attractor mechanism in N=2 supersymmetric extremal black holes and discusses its implications for deriving the Bekenstein-Hawking entropy formula independently of specific models.
Contribution
It provides a model-independent derivation of black hole entropy using Bertotti-Robinson geometry within the context of N=2 supersymmetry.
Findings
Bertotti-Robinson geometry plays a crucial role in the attractor mechanism.
The paper offers a model-independent approach to derive black hole entropy.
Implications for supersymmetric black hole entropy calculations are discussed.
Abstract
The role of Bertotti-Robinson geometry in the attractor mechanism of extremal black holes is described for the case of N = 2 supersymmetry. Its implication for a model-independent derivation of the Bekenstein-Hawking entropy formula is discussed.
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.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories