arXiv · 1012.2180
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 $μ\geq1$. 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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Colin Cunliff. 2011-04-25. Topologically Massive Gravity from the Outside In. https://doi.org/10.1088/0264-9381%2F28%2F19%2F195024
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