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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• Fermions tunnelling with quantum gravity correction
• The Effects of Minimal Length, Maximal Momentum and Minimal Momentum in Entropic Force
• Modified Hawking radiation of stationary and nonstationary Kerr-Newman-de Sitter black hole
• Charged fermions tunneling from stationary axially symmetric black holes with generalized uncertainty principle
• Black Hole Radiation with Modified Dispersion Relation in Tunneling Paradigm: Free-fall Frame
• Minimal Length Effects on Entanglement Entropy of Spherically Symmetric Black Holes in Brick Wall Model
• HBAR entropy of Infalling Atoms into a GUP-corrected Schwarzschild Black Hole and equivalence principle
• Hawking radiation of massive bosons via tunneling from black strings
• Deformed Hamilton-Jacobi Method in Covariant Quantum Gravity Effective Models
• Free-fall Rainbow BTZ Black Hole
• Kiselev black strings: the charged rotating solutions
• Quantum gravity corrections to the tunneling radiation of scalar particles
• Scalar particles tunneling radiation in the Demianski-Newman spacetime with influences of quantum gravity