PIRSA:09020005

Warped Wilson Line Inflation

APA

Zavala, I. (2009). Warped Wilson Line Inflation. Perimeter Institute. https://pirsa.org/09020005

MLA

Zavala, Ivonne. Warped Wilson Line Inflation. Perimeter Institute, Feb. 17, 2009, https://pirsa.org/09020005

BibTex

          @misc{ pirsa_PIRSA:09020005,
            doi = {10.48660/09020005},
            url = {https://pirsa.org/09020005},
            author = {Zavala, Ivonne},
            keywords = {Cosmology},
            language = {en},
            title = {Warped Wilson Line Inflation},
            publisher = {Perimeter Institute},
            year = {2009},
            month = {feb},
            note = {PIRSA:09020005 see, \url{https://pirsa.org}}
          }
          

Ivonne Zavala

Rheinische Friedrich-Wilhelms-Universität Bonn

Talk number
PIRSA:09020005
Talk Type
Subject
Abstract
I will discuss the possibility that a 'Wilson line' degree of freedom can play the role of an inflaton in a warped flux compactification, in the context of the DBI inflationary scenario. I will show how warped DBI Wilson line inflation offers an attractive alternative to ordinary (position field) DBI inflation, inasmuch as observational and theoretical constraints get considerably relaxed. Thus, besides the large non-Gaussianities produced in DBI scenarios, Wilson lines allow for an observable amount of gravitational waves, within consistent approximations.