We compute the three point correlation functions for primordial scalar and tensor fluctuations in single field inflationary models. We obtain explicit expressions in the slow roll limit where the answer is given terms of the two usual slow roll parameters. In a particular limit the three point functions are determined 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 and AdS/CFT. We emphasize that (A)dS/CFT can be viewed as a statement about the wavefunction of the universe.
Journal of High Energy Physics
- Pub Date:
- May 2003
- Physics of the Early Universe Large Scale Structure Formations Cosmology of Theories beyond the SM;
- High Energy Physics - Phenomenology;
- High Energy Physics - Theory
- harvmac, 38 pages. V5: One error corrected in section 3.1