Abstract
The asymptotically anti-de Sitter solutions of cosmological topologically massive gravity 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 Carlip–Deser–Waldron–Wise 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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