Exploring the Landscape with Classical Transitions
APA
Yang, I. (2011). Exploring the Landscape with Classical Transitions. Perimeter Institute. https://pirsa.org/11060064
MLA
Yang, I-Sheng. Exploring the Landscape with Classical Transitions. Perimeter Institute, Jun. 22, 2011, https://pirsa.org/11060064
BibTex
@misc{ pirsa_PIRSA:11060064, doi = {10.48660/11060064}, url = {https://pirsa.org/11060064}, author = {Yang, I-Sheng}, keywords = {Cosmology}, language = {en}, title = {Exploring the Landscape with Classical Transitions}, publisher = {Perimeter Institute}, year = {2011}, month = {jun}, note = {PIRSA:11060064 see, \url{https://pirsa.org}} }
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Abstract
Classical transition is one of the simplest consequences of cosmic bubble collisions. In quite a few simple toy model landscapes, collisions always result in classical transitions. Can it be generalized to the "real" string theory landscape? If so, does it imply some sort of hidden structure of the landscape?