Inflationary Constraints on String Theory
APA
Hertzberg, M. (2008). Inflationary Constraints on String Theory. Perimeter Institute. https://pirsa.org/08060185
MLA
Hertzberg, Mark. Inflationary Constraints on String Theory. Perimeter Institute, Jun. 06, 2008, https://pirsa.org/08060185
BibTex
@misc{ pirsa_PIRSA:08060185, doi = {10.48660/08060185}, url = {https://pirsa.org/08060185}, author = {Hertzberg, Mark}, keywords = {Quantum Fields and Strings, Particle Physics, Cosmology}, language = {en}, title = {Inflationary Constraints on String Theory}, publisher = {Perimeter Institute}, year = {2008}, month = {jun}, note = {PIRSA:08060185 see, \url{https://pirsa.org}} }
Collection
Talk Type
Abstract
It is an important task to embed inflation in a fundamental microphysical theory such as string theory. Since string theory possesses a vast landscape of 4-dimensional theories, we would like to know which portions contain inflation and which do not. I prove a no-go theorem that inflation and de Sitter vacua are forbidden in an exponentially large number of infinite families of simple and well understood compactifications of type IIA string theory. I also mention more complicated and less well understood compactifications, which may have the ingredients for our cosmology.