Using non-extensive statistical mechanics, the Bekenstein–Hawking area law is obtained
from microstates of black holes in loop quantum gravity, for arbitrary real positive values of …

In this paper, we carry out the entanglement calculations on the coherent intertwiners. We
first consider the entanglement introduced by the group averaging of the tensor-product-type …

The Barbero–Immirzi parameter,(γ), is introduced in loop quantum gravity (LQG), whose
physical significance is still the biggest open question because of its profound traits. In some …

We articulate the fact that the loop quantum gravity (LQG) description of the quantum
macrostates of black hole horizons, modeled as quantum isolated horizons (QIHs), is …

An attempt is made to demystify loop quantum gravity (LQG) in a concise and lucid way.
LQG is a background-independent as well as non-perturbative approach of the theory of …

We present a semi-rigorous justification of Bekenstein's Generalized Second Law of
Thermodynamics applicable to a universe with black holes present, based on a generic …

This chapter covers the attempt to quantise general relativity, through a reformulation in
terms of the Ashtekar variables. These are introduced, and the role and significance of the …

Using concomitantly the generalized second law of black hole thermodynamics and the
holographic Bekenstein entropy bound embellished by loop quantum gravity corrections to …

Following a recent proposal, we consider the most general structure possible for the
Hamiltonian operator associated with the quantum isolated horizon (QIH) with explanations …

In loop quantum gravity the quantum geometry of a black hole horizon consists of discrete
nonperturbative quantum geometric excitations (or punctures) labeled by spins, which are …