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In this paper, we probe in 4D Einstein-Gauss-Bonnet black hole and itsthermodynamics. We illustrate the three asymptotically 4D EGB spacetime as anasymptotically flat, de Sitter, and Anti-de Sitter. Also, we apply thetunneling of the massless particles from the horizon of 4D EGB gravity and weinvestigate the correlation between the emission modes and temperature of thehorizon. In asymptotically flat spacetime, the existence of the couplingconstant alone constructs the regular spacetime, the radiation deviates fromthe pure thermal, and the temperature of the black hole horizon would be zeroin the final stage of the black hole evaporation. In Asymptotically de Sitterspacetime, results illustrate that the evolution of the temperatures is indirection of the remaining rest mass with the probably same temperature for theblack hole and the cosmological horizon. In addition, the exciting result isthat temperature behaviors exactly match with the temperature behaviors of aregular black hole in Lovelock gravity in a higher dimension.

Radiation from Einstein-Gauss-Bonnet de Sitter Black Hole via Tunneling Process