  In this paper we obtain the black hole metric from a semiclassical analysis
of loop quantum black hole. Our solution and the Schwarzschild one tend to
match well at large distances from Planck region. In r=0 the semiclassical
metric is regular and singularity free in contrast to the classical one. By
using the new metric we calculate the Hawking temperature and the entropy. For
the entropy we obtain the logarithmic correction to the classical area law.
Finally we study the mass evaporation process and we show the mass and
temperature tend to zero at infinitive time.
