Topologically Massive Gravity from the Outside In
Abstract
The asymptotic solutions of cosmological topologically massive gravity (TMG) are analyzed for values of the mass parameter in the range μ≥1. At non-chiral values, a new term in the Fefferman-Graham expansion is needed to capture the bulk degree of freedom. The CDWW modes provide a basis for the pure non-Einstein solutions at all μ, with nonlinear corrections appearing at higher order in the expansion.
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