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fzero
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atyy said:Just trying to see if I understand. Does this correspond to the statement that any consistent background for perturbative string theory must be Ricci flat?
Flux vacua need not be Ricci flat, but there is an analogous constraint on the Ricci curvature. There can be further global constraints from anomaly cancellation.
Also, is it true that any Ricci flat background that has the same topology can be obtained from Minkowski spacetime (or in the first place, what are the Ricci flat solutions with the same topology)?
Depends on what you mean by "obtained." The Schwarzschild BH and Minkowski space don't quite have the same topology but the [tex]m\rightarrow 0[/tex] limit of the SBH is Minkowski space (to be precise I guess we'd say [tex]M_4/\{0\}[/tex]).
The classification of Ricci flat metrics in [tex]D\geq 4[/tex] is by no means complete. Even for the stronger CY condition (which may be taken as Ricci flat + admits a Kaehler structure), there is no complete classification. At least in the compact case, it's believed that there probably aren't many more inequivalent CYs than have been discovered, but I don't believe this is proven. I believe that noncompact CYs which are resolutions of orbifolds [tex]\mathbb{C}^n/\Gamma[/tex] are more or less classified: this is associated to the so-called McKay correspondence.