Tunnelling of relativistic particles from new type black hole in new massive gravity
Özet
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.
Anahtar kelimeler
Atıf için künye
Geçim, G., & SUCU, Y. (2013). Tunnelling of relativistic particles from new type black hole in new massive gravity. Journal of Cosmology and Astroparticle Physics, 2013(2). https://doi.org/10.1088/1475-7516/2013/02/023
BibTeX
@article{gecim2013-78890,
author = {Geçim, Ganim and SUCU, YUSUF},
title = {Tunnelling of relativistic particles from new type black hole in new massive gravity},
journal = {Journal of Cosmology and Astroparticle Physics},
year = {2013},
volume = {2013},
number = {2},
issn = {1475-7516},
doi = {10.1088/1475-7516/2013/02/023},
url = {https://akademik.atauni.edu.tr/yayinlar/78890-tunnelling-of-relativistic-particles-from-new-type-black-hole-in-new-massive}
}