The tunnelling process always occur nearby the event horizon of the black
hole. In this paper, we investigate the tunnelling radiation in the background
of the Kerr-Newman-Taub-NUT black hole. The new coordinate system for
Kerr-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 at
event horizon. With the help of conservation of angular momentum, self
gravitational effect and energy, we will show that Hawking's radiation is not
exclusively thermal.Comment: 14 pages, 15 figure