- All News & Features
- All Events
-
- Archived Events
-
-
2013
-
2012
-
2011
-
2010
-
2009
-
2008
-
2007
-
2006
-
2005
-
-
2003
-
2002
-
2001
-
2000
-
1999
-
HEP Astro
-
Astronomy Colloquium
-
Biophysics Seminar
-
CM - AMO Seminars
-
CM Theory Seminars
-
Complex Systems
-
Department Colloquia
-
Quantitative Biology Seminars
-
HET Brown Bag Series
-
HET Seminars
-
Life After Grad School Seminars
-
Farrand Memorial Lecture
-
Workshops & Conferences
-
Miscellaneous
-
Saturday Morning Physics
-
Special Lectures
- Search Events
-
- Special Lectures
- K-12 Programs
- Saturday Morning Physics
- Seminars & Colloquia
Wednesday, February 8, 2012
5:00 AM
3481 Randall (Oskar Klein Conference Room)
Speaker: Paul McFadden (Perimeter)
We present a holographic framework for cosmology enabling four-dimensional inflationary universes to be described in terms of three-dimensional dual quantum field theories. Cosmological observables, such as the primordial power spectra and non-Gaussianities, are related to correlation functions of the dual QFT through specific holographic formulae. Through perturbative calculations for a simple class of dual QFTs, we compute holographically the observational signatures of a universe emerging from a non-geometric phase in which the gravitational description in strongly coupled at early times.
