An extended solution space for Chern-Simons gravity: the slowly rotating Kerr black hole

Details An extended solution space for Chern-Simons gravity: the slowly rotating Kerr black hole An extended solution space for Chern-Simons gravity: the slowly rotating Kerr black hole

2010-10-21

arxiv.org/abs/1010.4526v1

Phys.Rev.D82:101502,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, PRD accepted

Scientific paper

10.1103/PhysRevD.82.101502

In the Einstein-Cartan formulation, an iterative procedure to find solutions in non-dynamical Chern-Simons (CS) gravity in vacuum is proposed. The iterations, in powers of a small parameter $\beta$ which codifies the CS coupling, start from an arbitrary torsionless solution of Einstein equations. With Schwarzschild as the zeroth-order choice, we derive a second-order differential equation for the $\mathcal{O}(\beta)$ corrections to the metric, for an arbitrary zeroth-order embedding parameter. In particular, the slowly rotating Kerr metric is an $\mathcal{O}(\beta)$ solution in either the canonical or the axial embeddings.

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