  Here we study the effects of the Generalized Uncertainty Principle in the
tunneling formalism for Hawking radiation to evaluate the quantum-corrected
Hawking temperature and entropy for a Schwarzschild black hole. We compare our
results with the existing results given by other candidate theories of quantum
gravity. In the entropy-area relation we found some new correction terms and in
the leading order we found a term which varies as $\sim \sqrt{Area}$. We also
get the well known logarithmic correction in the sub-leading order. We discuss
the significance of this new quantum corrected leading order term.
