Black holes in the TeVeS theory of gravity and their thermodynamics
Eva Sagi, Jacob D. Bekenstein

TL;DR
This paper explores black hole solutions within TeVeS gravity, demonstrating that their thermodynamic properties mirror those in general relativity, and discusses implications for Lorentz symmetry violation.
Contribution
It analytically solves the TeVeS equations for black holes and shows their thermodynamics align with general relativity, advancing understanding of gravity and thermodynamics in alternative theories.
Findings
Reissner-Nordstrom metric as physical metric in TeVeS
Black hole entropy and temperature match GR predictions
Thermodynamics should be based on the physical metric
Abstract
TeVeS, a relativistic theory of gravity, was designed to provide a basis for the modified Newtonian dynamics. Since TeVeS differs from general relativity (e.g., it has two metrics, an Einstein metric and a physical metric), black hole solutions of it would be valuable for a number of endeavors ranging from astrophysical modeling to investigations into the interrelation between gravity and thermodynamics. Giannios has recently found a TeVeS analogue of the Schwarzschild black hole solution. We proceed further with the program by analytically solving the TeVeS equations for a static spherically symmetric and asymptotically flat system of electromagnetic and gravity fields. We show that one solution is provided by the Reissner-Nordstrom metric as physical metric, the TeVeS vector field pointing in the time direction, and a TeVeS scalar field positive everywhere (the last feature protects…
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