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D = 5 Einstein-Maxwell-Chern-Simons black holes.

Jutta Kunz1, Francisco Navarro-Lérida

  • 1Institut für Physik, Universität Oldenburg, Postfach 2503, D-26111 Oldenburg, Germany.

Physical Review Letters
|April 12, 2006
PubMed
Summary
This summary is machine-generated.

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Five-dimensional Einstein-Maxwell-Chern-Simons theory reveals supersymmetric black holes with specific properties. Higher Chern-Simons coefficients lead to rotational instabilities and unique black hole characteristics.

Area of Science:

  • Theoretical physics
  • Gravitational physics
  • String theory

Background:

  • Five-dimensional Einstein-Maxwell-Chern-Simons theory is a framework for studying black hole solutions.
  • Supersymmetry in black hole physics often relates to stability and unique properties.

Purpose of the Study:

  • To investigate the properties of supersymmetric black holes in five-dimensional Einstein-Maxwell-Chern-Simons theory.
  • To analyze the impact of the Chern-Simons coefficient (lambda) on black hole stability and characteristics.

Main Methods:

  • Theoretical analysis of the five-dimensional Einstein-Maxwell-Chern-Simons theory.
  • Examination of black hole solutions based on the Chern-Simons coefficient lambda.

Main Results:

Related Experiment Videos

  • For lambda = 1, supersymmetric black holes exhibit vanishing horizon angular velocity but finite angular momentum.
  • For lambda > 1, a rotational instability emerges, leading to counterrotating black holes.
  • For lambda > 2, black holes are not uniquely defined by global charges, and rotating black holes with vanishing angular momentum appear.

Conclusions:

  • Supersymmetry in this theory is linked to a critical point between stability and instability.
  • The Chern-Simons coefficient significantly influences black hole behavior, including stability and the emergence of exotic solutions.