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We compute the three point correlation functions for primordial scalar andtensor fluctuations in single field inflationary models. We obtain explicitexpressions in the slow roll limit where the answer is given terms of the twousual slow roll parameters. In a particular limit the three point functions aredetermined completely by the tilt of the spectrum of the two point functions.We also make some remarks on the relation of this computation to dS/CFT andAdS/CFT. We emphasize that (A)dS/CFT can be viewed as a statement about thewavefunction of the universe.Comment: harvmac, 38 pages. V5: One error corrected in section 3.

Non-gaussian features of primordial fluctuations in single field inflationary models