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We study the quantum corrections to the four-dimensional Schwarzschild Anti
de Sitter black hole using effective field theory approach. We compute the
quantum correction to Hawking temperature upto order $\mathcal{O}{(G^{2})}$ for
a Schwarzschild AdS black hole when the emitted object is massless and massive.
We use the expression of the modified horizon radius to compute the quantum
corrected entropy upto order $\mathcal{O}{(G^{2})}$. Finally we compute quantum
corrected thermodynamic parameters specific heat, free energy and pressure.

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