Authors: Reinhard Meinel
Date: 25 Nov 2009
Abstract: Analytical and numerical results on equilibrium configurations of rotating fluid bodies within Einstein's theory of gravitation are reviewed. Particular emphasis is placed on continuous parametric transitions to black holes. In this connection the uniqueness of extremal Kerr black holes is discussed.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis