  Recent suggestion, that the emission of a quantum of energy corresponding to
the asymptotic value of quasinormal modes of a Schwarzschild black hole should
be associated with the loss of spin one punctures from the black hole horizon,
fixes the Immirzi parameter to a definite value. We show that saturating the
horizon with spin one punctures reproduces the earlier formula for the black
hole entropy, including the $ln (area)$ correction with definite coefficient (-
3/2) for large area.
