Tunnelling of relativistic particles from new type black hole in new massive gravity

Journal Article · Fri Feb 01 00:00:00 EST 2013 · Journal of Cosmology and Astroparticle Physics

DOI:https://doi.org/10.1088/1475-7516/2013/02/023· OSTI ID:22282911

Gecim, Ganim; Sucu, Yusuf ^[1]

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1. Department of Physics, Akdeniz University, Antalya (Turkey)

In the framework of the three dimensional New Massive Gravity theory introduced by Bergshoeff, Hohm and Townsend, we analyze the behavior of relativistic spin-1/2 and spin-0 particles in the New-type Black Hole backgroud, solution of the New Massive Gravity.We solve Dirac equation for spin-1/2 and Klein-Gordon equation for spin-0. Using Hamilton-Jacobi method, we discuss tunnelling probability and Hawking temperature of the spin-1/2 and spin-0 particles for the black hole. We observe that the tunnelling probability and Hawking temperature are same for the spin-1/2 and spin-0.

• OSTI ID: 22282911
• Journal Information: Journal of Cosmology and Astroparticle Physics, Vol. 2013, Issue 02; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ASTROPHYSICS
BLACK HOLES
BOSONS
COSMOLOGY
DIRAC EQUATION
FERMIONS
GRAVITATION
HAMILTON-JACOBI EQUATIONS
KLEIN-GORDON EQUATION
MATHEMATICAL SOLUTIONS
PROBABILITY
RELATIVISTIC RANGE
SPIN
THREE-DIMENSIONAL CALCULATIONS
TUNNEL EFFECT