Dynamic noncommutative BTZ black holes
arXiv:2105.11130 · doi:10.1016/j.physletb.2021.136391
Abstract
We have studied the charged BTZ black holes in noncommutative spaces arising from two independent approaches. First, by using the Seiberg-Witten map followed by a dynamic choice of gauge in the Chern-Simons gauge theory. Second, by inducing the fuzziness in the mass and charge by a Lorentzian distribution function with the width being the same as the minimal length of the associated noncommutativity. In the first approach, we have found the existence of non-static and non-stationary BTZ black holes in noncommutative spaces for the first time in the literature, while the second approach facilitates us to introduce a proper bound on the noncommutative parameter so that the corresponding black hole becomes stable and physical. We have used a contemporary tunneling formalism to study the thermodynamics of the black holes arising from both of the approaches and analyze their behavior within the context.
16 pages, 5 figures
References in corpus (13)
- Noncommutative geometry inspired charged black holes
- Hawking Radiation as Quantum Tunneling from Noncommutative Schwarzschild Black Hole
- Non-commutative geometry inspired higher-dimensional charged, black holes
- q-deformed noncommutative cat states and their nonclassical properties
- Time-dependent q-deformed coherent states for generalized uncertainty relations
- Squeezed coherent states for noncommutative spaces with minimal length uncertainty relations
- Entangled squeezed states in noncommutative spaces with minimal length uncertainty relations
- PT-symmetric noncommutative spaces with minimal volume uncertainty relations
- Noncommutative quantum mechanics in a time-dependent background
- Probing noncommutative theories with quantum optical experiments
- Noncommutative BTZ Black Hole in Polar Coordinates
- Asymptotic quasinormal modes of a noncommutative geometry inspired Schwarzschild black hole
- Cylindrical symmetric, non-rotating and non-static or static black hole solutions and the naked singularities