Role of the remnant symmetries in gravitational theories based on absolute parallelism: a 2D standpoint
arXiv:2112.12381 · doi:10.1088/1361-6382/ac5eb9
Abstract
By using simplified 2D gravitational, non-local Lorentz invariant actions constructed upon the torsion tensor, we discuss the physical meaning of the remnant symmetries associated with the near-horizon (Milne) geometry experienced by a radial observer in Schwarzschild spacetime. We then fully characterize the remnant symmetries corresponding to this near-horizon 2D geometry by solving the motion equations adapted to 2D Milne space. This symmetries, which represent special or privileged \emph{diads}, acquire the form of uniformly accelerated (Rindler) observers whose constant acceleration is proportional to the black hole mass .
11 pages, 1 figure, accepted for publication in Classical and Quantum Gravity
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