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In the present paper we study the Hawking radiation as a quantum tunnelingeffect of spin-$1$ particles from a five-dimensional, spherically symmetric,Einstein-Yang-Mills-Gauss-Bonnet (5D EYMGB) black hole. We solve the Procaequation (PE) by applying the WKB approximation and separation of variables viaHamilton-Jacobi (HJ) equation which results in a set of five differentialequations, and reproduces in this way, the Hawking temperature. In the secondpart of this paper, we extend our results beyond the semiclassicalapproximation. In particular, we derive the logarithmic correction to theentropy of the 5D EYMGB black hole and show that the quantum corrected specificheat indicates the possible existence of a remnant.

Quantum Tunneling of Spin-1 Particles from a 5D Einstein-Yang-Mills-Gauss-Bonnet Black Hole Beyond Semiclassical Approximation