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Extended solution space for Chern-Simons gravity

Extended solution space for Chern-Simons gravity

EC + CS: Comments on the

EC + CS: Comments on the Kerr solution• The consistency conditions are properly satisfied, at least to O(β).• Furthermore, the solution is also valid for an axial embedding parameter produces asymmetry breaking direction parallel to the rotation axis of the Kerr metric at infinity.ϑ = M r cos θ ,L = a zrθ• Rotation breaks Spherical to Axialsymmetry: Schw. → Kerr,f ( r ) = f ( r, )θVIII Silafae - UTFSM, Valparaíso, 2010 Mauro Cambiaso New solutions in Chern-Simons gravity – p. 14

EC + CS: Comments on the Kerr solution• The consistency conditions are properly satisfied, at least to O(β).• Furthermore, the solution is also valid for an axial embedding parameter produces asymmetry breaking direction parallel to the rotation axis of the Kerr metric at infinity.ϑ = M r cos θ ,L = 0v = 0µ• This non-canonical choice for v µ reproducesthe previous situation.VIII Silafae - UTFSM, Valparaíso, 2010 Mauro Cambiaso New solutions in Chern-Simons gravity – p. 14

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