Evaporation phenomena in f(T) gravity
M. J. S. Houndjo, D. Momeni, R. Myrzakulov, M. E. Rodrigues

TL;DR
This paper investigates evaporation phenomena in generalized teleparallel gravity, showing that the choice of tetrad basis (diagonal vs. non-diagonal) crucially affects whether black holes can evaporate or remain stable.
Contribution
It demonstrates that non-diagonal tetrads allow evaporation and anti-evaporation phenomena in f(T) gravity, unlike diagonal tetrads which freeze black hole evolution.
Findings
Diagonal tetrads prevent evaporation, freezing black holes.
Non-diagonal tetrads enable both evaporation and anti-evaporation.
Phenomena depend on initial horizon perturbation phase.
Abstract
We formulate evaporation phenomena in a generic model of generalized teleparallel gravity in Weitzenbock spacetime with diagonal and non-diagonal tetrads basis. We also perform the perturbation analysis around the constant torsion scalar solution named Nariai spacetime which is an exact solution of field equations as the limiting case of the Schwarzschild-de Sitter and in the limit where two back hole and their cosmological horizons coincide. By a carefully analysis of the horizon perturbation equation, we show that (anti)evaporation can not happen if we use a diagonal tetrad basis. This result implies that a typical black hole in any generic form of generalized teleparallel gravity is frozen in its initial state if we use the diagonal tetrads. But in the case of non-diagonal tetrads the analysis is completely different. By a suitable non trivial non-diagonal tetrad basis we investigate…
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