Hawking Radiation of Charged Particles via Tunneling from a Cylindrically Symmetric Black Hole in Anti-de Sitter Space-Time

Applying Parikh-Wilzcek's semi-classical quantum tunneling model, we study the Hawking radiation of charged particles as tunneling from the event horizon of a cylindrically symmetric black hole in anti-de Sitter space-time. The derived result shows that the tunneling rate of charged particles is related to the change ofBekenstein-Hawking entropy and that the radiation spectrum is notstrictly pure thermal after taking the black hole background dynamicaland self-gravitation interaction into account, but is consistentwith the underlying unitary theory.