Non-Gaussian features of primordial fluctuations in single field inflationary models Export

@article{citeulike:899225, abstract = {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.}, archivePrefix = {arXiv}, author = {Maldacena, Juan}, citeulike-article-id = {899225}, citeulike-linkout-0 = {http://arxiv.org/abs/astro-ph/0210603}, citeulike-linkout-1 = {http://arxiv.org/pdf/astro-ph/0210603}, day = {6}, eprint = {astro-ph/0210603}, keywords = {inflation, nongaussianities, toread}, month = {May}, posted-at = {2006-10-16 11:46:50}, priority = {2}, title = {Non-Gaussian features of primordial fluctuations in single field inflationary models}, url = {http://arxiv.org/abs/astro-ph/0210603}, year = {2005} }

TY - JOUR ID - citeulike:899225 L3 - citeulike-article-id:899225 N2 - 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. TI - Non-Gaussian features of primordial fluctuations in single field inflationary models KW - inflation KW - nongaussianities KW - toread AU - Maldacena, Juan PY - 2005/May/06/ UR - http://arxiv.org/abs/astro-ph/0210603 ER -