The Expansion On A Compact Manifold Of Exceptional Holonomy
arXiv:1404.2460 · doi:10.1007/JHEP06(2014)051
Abstract
In the approximation corresponding to the classical Einstein equations, which is valid at large radius, string theory compactification on a compact manifold of or holonomy gives a supersymmetric vacuum in three or two dimensions. Do corrections to the Einstein equations disturb this statement? Explicitly analyzing the leading correction, we show that the metric of can be adjusted to maintain supersymmetry. Beyond leading order, a general argument based on low energy effective field theory in spacetime implies that this is true exactly (not just to all finite orders in ). A more elaborate field theory argument that includes the massive Kaluza-Klein modes matches the structure found in explicit calculations. In M-theory compactification on a manifold of or Spin(7) holonomy, similar results hold to all orders in the inverse radius of -- but not exactly. The classical moduli space of metrics on a manifold is known to be locally a Lagrangian submanifold of . We show that this remains valid to all orders in the or inverse radius expansion.
arXiv comment34 pp
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