  In loop quantum gravity, the quantum geometry of a black hole horizon consist
of discrete non-perturbative quantum geometric excitations (or punctures)
labeled by spins, which are responsible for the quantum area of the horizon. If
these punctures are compared to a gas of particles, then the spins associated
with the punctures can be viewed as single puncture area levels analogous to
single particle energy levels. Consequently, if we {\it assume} these punctures
to be {\it indistinguishable}, the microstate count for the horizon resembles
that of Bose-Einstein counting formula for gas of particles. For the
Bekenstein-Hawking area law(BHAL) to follow from the entropy calculation in the
large area limit, the Barbero-Immirzi parameter($\g$) approximately takes a
constant value.
