Thermodynamics of charged and rotating black strings

Abstract

We study thermodynamics of cylindrically symmetric black holes. Uncharged as well as charged and rotating objects have been discussed. We derive surface gravity and hence the Hawking temperature and entropy for all these cases. We correct some results in the literature and present new ones. It is seen that thermodynamically these black configurations behave differently from spherically symmetric objects.

References in corpus (1)

• Rotating Black String with Nonlinear Source

Cited by in corpus (5)

• Hawking Radiation from Elko Particles Tunnelling across Black Strings Horizon
• Are Black Holes Springy?
• Emission of scalar particles from cylindrical black holes
• Charged slowly rotating toroidal black holes in the (1+3)-dimensional Einstein-power-Maxwell theory
• Quantum tunneling from scalar fields in rotating black strings