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The tunnelling process always occur nearby the event horizon of the blackhole. In this paper, we investigate the tunnelling radiation in the backgroundof the Kerr-Newman-Taub-NUT black hole. The new coordinate system forKerr-Newman-Taub-NUT is introduced, which helps us to form new line element.This line element helps us to show that new coordinate is exhaustively acted atevent horizon. With the help of conservation of angular momentum, selfgravitational effect and energy, we will show that Hawking's radiation is notexclusively thermal.

Kerr-Newman-Taub-NUT Black Hole Tunnelling Radiation