Abstract
In the framework of the three dimensional New MassiveGravity theory introduced by Bergshoeff, Hohm and Townsend, weanalyze the behavior of relativistic spin-1/2 and spin-0 particlesin the New-type Black Hole backgroud, solution of the New MassiveGravity.We solve Dirac equation for spin-1/2 and Klein-Gordonequation for spin-0. Using Hamilton-Jacobi method, we discuss tunnellingprobability and Hawking temperature of the spin-1/2 and spin-0particles for the black hole. We observe that the tunnellingprobability and Hawking temperature are same for the spin-1/2 and spin-0.
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