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2010
DOI: 10.1007/s10773-010-0453-8
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Fermion Tunneling from an Axis-Symmetric Black Hole beyond the Semiclassical Approximation

Abstract: Based on the Hamilton-Jacobi method beyond the semiclassical approximation proposed by R. Baberjee and B.R. Majhi, Hawking radiation of Dirac particle as tunneling through the event horizon is calculated. It is shown that all quantum corrections in the fermion particle action are proportional to the usual semiclassical contribution. Under the conception of irreducible mass and the first law of thermodynamics, the modifications to Hawking temperature and Bekenstein-Hawking entropy are given for a Kerr-Newmann b… Show more

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Cited by 3 publications
(4 citation statements)
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References 31 publications
(39 reference statements)
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“…where S is the classical action function of a particle trajectory [38][39][40][41][42]. Therefore, in order to discuss tunneling probability, one needs to calculate the imaginary part of a classical action function, S, regarding the tunnelling probability.…”
Section: Jcap02(2013)023mentioning
confidence: 99%
See 2 more Smart Citations
“…where S is the classical action function of a particle trajectory [38][39][40][41][42]. Therefore, in order to discuss tunneling probability, one needs to calculate the imaginary part of a classical action function, S, regarding the tunnelling probability.…”
Section: Jcap02(2013)023mentioning
confidence: 99%
“…(2.18), we find that ImK + (r) = −ImK − (r) (see also [43]). Therefore, the tunneling probability of the Dirac particle from the outer event horizon is given by [38][39][40][41][42] Γ = e − 2 ImS = P out…”
Section: 19)mentioning
confidence: 99%
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“…For instance, the Hamilton-Jacobi approach is an effective way to study the Hawking radiation as a quantum tunneling process of particles from black holes. In this context, Hawking radiation is seen to be extensively investigated in the literature in the context of quantum tunneling of a pointlike elementary particle [7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34]. These studies show that Hawking radiation of a black hole must be completely independent from the mass, total angular momentum, energy, charge of a tunneling point particle.…”
Section: Introductionmentioning
confidence: 99%