Semiclassical corrections to black hole entropy and the generalized uncertainty principle

Understand

In this paper, employing the path integral method in the framework of a canonical description of a Schwarzschild black hole, we obtain the corrected inverse temperature and entropy of the black hole.

• The corrections are those coming from the quantum effects as well as from the Generalized Uncertainty Principle effects.
• Furthermore, an equivalence between the polymer quantization and the Generalized Uncertainty Principle description is shown provided the parameters characterizing these two descriptions are proportional.