arXiv · 1301.1347
Non-Fefferman-Graham asymptotics and holographic renormalization in New Massive Gravity
Abstract
The asymptotic behavior of new massive gravity (NMG) is analyzed for all values of the mass parameter satisfying the Breitenlohner-Freedman bound. The traditional Fefferman-Graham expansion fails to capture the dynamics of NMG, and new terms in the asymptotic expansion are needed to include the massive graviton modes. New boundary conditions are discovered for a range of values $-1<2m^2l^2<1$ at which non-Einstein modes decay more slowly than the Brown-Henneaux boundary conditions. The holographically renormalized stress tensor is computed for these modes, and the relevant counterterms are identified up to unphysical ambiguities.
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Colin Cunliff. 2013-02-19. Non-Fefferman-Graham asymptotics and holographic renormalization in New Massive Gravity. https://doi.org/10.1007/jhep04(2013)141
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