Thermodynamics variables of the BTZ Black Hole with a Minimal Length and its Efficiency

Hawking radiation and entropy of a BTZ black hole with minimum length

“…Therefore, by solving the Einstein equations with these modifications, was determined the metric of a deformed Schwarzschild black hole due to noncommutativity. In addition, many papers have appeared in the literature suggesting different ways of introducing noncommutativity into Bañados-Teitelboim-Zanelli (BTZ) black holes [56][57][58][59][60][61][62][63][64][65][66]. Furthermore, the thermodynamic properties of noncommutative BTZ and noncommutative Schwarzschild black holes have been explored via Lorentzian distribution with GUP and logarithmic corrections for entropy have been obtained due to the noncommutativity effect [67,68].…”

Study of thermodynamical geometries of conformal gravity black hole

“…One can argue that there are many ambiguities in Hawking-Bekenstein entropy which are partially covered in logarithmic corrected entropy, higherorder corrected entropy, etc. Many authors [5][6][7][8][9][10] discussed in detail the Hawking-Bekenstein area relationship and found various useful results. One can not completely deny the idea of the Hawking-Bekenstein area entropy relationship.…”