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.

    Source link


    Leave A Reply