Radiation from Einstein–Gauss–Bonnet de Sitter black hole via tunneling process

Abstract In this paper, we probe in 4D Einstein–Gauss–Bonnet black hole and its thermodynamics. We illustrate the three asymptotically EGB spacetime as an flat, de Sitter, Anti-de Sitter. Also, apply tunneling of massless particles from horizon gravity investigate correlation between emission modes temperature horizon. flat spacetime, existence coupling constant alone constructs regular radiation deviates pure thermal, would be zero final stage evaporation. Asymptotically Sitter results that evolution temperatures is direction remaining rest mass with probably same for cosmological addition, exciting result behaviors exactly match a Lovelock higher dimension.