Cold black holes in scalar-tensor theories
K. A. Bronnikov, C. P. Constantinidis, R. L. Evangelista, J. C., Fabris

TL;DR
This paper investigates the existence and properties of black holes in scalar-tensor theories of gravity, revealing unique features such as zero temperature and infinite horizon area in certain anomalous cases, with detailed analysis of Brans-Dicke theory.
Contribution
It demonstrates the existence of black holes with unusual characteristics in scalar-tensor theories, especially in anomalous cases with negative kinetic terms, and analyzes their thermodynamic and geometric properties.
Findings
Black holes with zero Hawking temperature in scalar-tensor theories.
Infinite horizon area occurs in certain anomalous theories.
In Brans-Dicke theory, two types of infinite-area black holes are identified.
Abstract
We study the possible existence of black holes in scalar-tensor theories of gravity in four dimensions. Their existence is verified for anomalous versions of these theories, with a negative kinetic term in the Lagrangian. The Hawking temperature T_H of these holes is zero, while the horizon area is (in most cases) infinite. It is shown that an infinite value of T_H can occur only at a curvature singularity rather than a horizon. As a special case, the Brans-Dicke theory is studied in more detail, and two kinds of infinite-area black holes are revealed, with finite and infinite proper time needed for an infalling particle to reach 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.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
