5.1 The Mazur IdentityStationary Black Holes: Uniqueness and 4.5 The Stationary Einstein-Maxwell System

5 Applications of the Coset Structure 

The tex2html_wrap_inline3625 -model structure is responsible for various distinguished features of the stationary Einstein-Maxwell (EM) system and related self-gravitating matter models. This section is devoted to a brief discussion of some applications: We argue that the Mazur identity [133Jump To The Next Citation Point In The Article], the quadratic mass formulas [89Jump To The Next Citation Point In The Article] and the Israel-Wilson class of stationary black holes [102Jump To The Next Citation Point In The Article], [145Jump To The Next Citation Point In The Article] owe their existence to the tex2html_wrap_inline3625 -model structure of the stationary field equations.





5.1 The Mazur IdentityStationary Black Holes: Uniqueness and 4.5 The Stationary Einstein-Maxwell System

image Stationary Black Holes: Uniqueness and Beyond
Markus Heusler
http://www.livingreviews.org/lrr-1998-6
© Max-Planck-Gesellschaft. ISSN 1433-8351
Problems/Comments to livrev@aei-potsdam.mpg.de