Thermodynamics evaluation in Einstein–Gauss–Bonnet gravity like black holes

From D-dimensional black holes, we investigate the Hawking radiation of charged boson particles from charged black holes without and with quantum gravity. We apply the field equation and WKB approximation to solve the Einstein–Gauss–Bonnet gravity like spacetime and obtain the tunneling radiation from charged black holes using complex path integration. We also calculate the temperature of the radiation from these black holes using the tunneling probability of outgoing particles without and with the influence of quantum gravity. We also look into the entropy and heat capacity of well-known thermodynamic properties for the geometry under consideration. It is concluded that the D dimension like black holes is stable or unstable under Einstein–Gauss–Bonnet gravity.