Quantum tunneling from scalar fields in rotating black strings

Abstract

Using the Hamilton-Jacobi method of quantum tunneling and complex path integration, we study Hawking radiation of scalar particles from rotating black strings. We discuss tunneling of both charged and uncharged scalar particles from the event horizons. For this purpose, we use the Klein-Gordon equation and find the tunneling probability of outging scalar particles. The procedure gives Hawking temperature for rotating charged black strings as well.

Corrections and changes

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Cited by in corpus (11)

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• Quantum tunneling from three-dimensional black holes
• Tunneling of Massive Vector Particles From Rotating Charged Black Strings
• Hawking Radiation of Mass Generating Particles From Dyonic Reissner Nordström Black Hole
• Hawking radiation of scalars from charged accelerating and rotating black holes with NUT parameter
• Stationary Scalar Clouds Around Maximally Rotating Linear Dilaton Black Holes
• First-order correction of tunneling and entropy in the Horndeski gravity-like hairy black hole
• Quantum tunneling from generalized $(2+1)$ dimensional black holes having Noether symmetry
• Kiselev black strings: the charged rotating solutions
• Scalar Clouds and Quasinormal Modes
• Hawking non-thermal and Purely thermal radiations of Kerr-de Sitter black hole by Hamilton-Jacobi method