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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
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Stationary Black Holes: Uniqueness and Beyond
1ITP, University of Zurich, CH-8057 Zurich, Switzerland.
Summary
Black hole solutions are more diverse than previously thought, with new configurations not defined solely by mass or angular momentum. This challenges previous understandings of black hole uniqueness and symmetry in advanced theories.
Area of Science:
- Theoretical Physics
- General Relativity
- Black Hole Physics
Background:
- The characterization of black hole solutions has traditionally relied on mass, angular momentum, and global charges.
- Symmetry properties of vacuum and electro-vacuum black hole spacetimes are well-established.
Purpose of the Study:
- To review recent advancements in black hole solutions beyond traditional characterizations.
- To discuss the implications of these new solutions for black hole uniqueness theorems, particularly the Einstein-Maxwell system.
Main Methods:
- Review of recent theoretical developments in stationary black hole solutions.
- Analysis of black hole configurations in self-gravitating non-linear field theories.
- Discussion in the context of the Einstein-Maxwell uniqueness theorem.
Main Results:
- The spectrum of known black hole solutions has unexpectedly expanded.
- Not all black hole equilibrium configurations are solely determined by mass, angular momentum, and global charges.
- High symmetry observed in vacuum/electro-vacuum spacetimes is lost in self-gravitating non-linear field theories.
Conclusions:
- Recent findings challenge the completeness of mass, angular momentum, and global charges in characterizing all black hole solutions.
- The study highlights a departure from the high symmetry expected in simpler black hole spacetimes when considering non-linear field theories.
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