A simple, approximate method for analysis of Kerr-Newman black hole dynamics and thermodynamics

In this work we present a simple approximate method for analysis of the basic dynamical and thermodynamical characteristics of Kerr-Newman black hole. Instead of the complete dynamics of the black hole self-interaction, we consider only the stable (stationary) dynamical situations determined by cond...

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Bibliographic Details
Main Authors: Panković V., Ciganović S., Glavatović R.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2009-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2009/1450-698X0978039P.pdf