Remarks on remnants by fermions' tunnelling from black strings

Abstract

Hawking's calculation is unable to predict the final stage of the black hole evaporation. When effects of quantum gravity are taken into account, there is a minimal observable length. In this paper, we investigate fermions' tunnelling from the charged and rotating black strings. With the influence of the generalized uncertainty principle, the Hawking temperatures are not only determined by the rings, but also affected by the quantum numbers of the emitted fermions. Quantum gravity corrections slow down the increases of the temperatures, which naturally leads to remnants left in the evaporation.

16pages, Publised in Advances in High Energy Physics, Volume 2014, Article ID 620157

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Cited by in corpus (8)

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• Minimal Length Effects on Tunnelling from Spherically Symmetric Black Holes
• Fermions tunnelling with quantum gravity correction
• The Effects of Minimal Length, Maximal Momentum and Minimal Momentum in Entropic Force
• Deformed Hamilton-Jacobi Method in Covariant Quantum Gravity Effective Models
• Hawking radiation of massive bosons via tunneling from black strings
• Quantum gravity corrections to the tunneling radiation of scalar particles
• Scalar particles tunneling radiation in the Demianski-Newman spacetime with influences of quantum gravity