Monodromy in the CMB: Gravity Waves and String Inflation
APA
Westphal, A. (2008). Monodromy in the CMB: Gravity Waves and String Inflation. Perimeter Institute. https://pirsa.org/08060140
MLA
Westphal, Alexander. Monodromy in the CMB: Gravity Waves and String Inflation. Perimeter Institute, Jun. 03, 2008, https://pirsa.org/08060140
BibTex
@misc{ pirsa_PIRSA:08060140, doi = {10.48660/08060140}, url = {https://pirsa.org/08060140}, author = {Westphal, Alexander}, keywords = {Quantum Fields and Strings, Particle Physics, Cosmology}, language = {en}, title = {Monodromy in the CMB: Gravity Waves and String Inflation}, publisher = {Perimeter Institute}, year = {2008}, month = {jun}, note = {PIRSA:08060140 see, \url{https://pirsa.org}} }
Stanford University
Collection
Talk Type
Abstract
We present a simple mechanism for obtaining large-field inflation, and hence a gravitational wave signature, from string theory compactified on twisted tori. For Nil manifolds, we obtain a leading inflationary potential proportional to phi^(2/3) in terms of the canonically normalized field phi, yielding predictions for the tilt of the power spectrum and the tensor-to-scalar ratio, $n_sapprox 0.98$ and $rapprox 0.04$ with 60 e-foldings of inflation; we note also the possibility of a variant with a candidate inflaton potential proportional to phi^(2/5). The basic mechanism involved in extending the field range -- monodromy in D-branes as they move in circles on the manifold -- arises in a more general class of compactifications, though our methods for controlling the corrections to the slow-roll parameters require additional symmetries.