Relativit\'e g\'en\'erale: solutions exactes stationnaires
G\'erard Cl\'ement

TL;DR
This paper reviews stationary exact solutions in general relativity, focusing on black hole spacetimes and using sigma models to generate new solutions from Einstein-Maxwell equations.
Contribution
It introduces a sigma model reformulation of stationary Einstein-Maxwell equations, enabling the generation of new solutions and deepening understanding of black hole geometries.
Findings
Several stationary solutions interpreted as black holes
Reformulation as a gravitating sigma model
Method for generating new solutions
Abstract
After a brief summary of the foundations of general relativity, we will concentrate on the stationary exact solutions of the Einstein and Einstein-Maxwell equations. A number of these solutions can be interpreted as black holes, corresponding to a special spacetime geometry. Then, we will show that the reformulation of the stationary Einstein-Maxwell equations as a gravitating sigma model provides us with a powerful tool to generate new solutions.
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Taxonomy
TopicsRelativity and Gravitational Theory · Cosmology and Gravitation Theories · Algebraic and Geometric Analysis
