PIRSA:10030037
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Resonant non-Gaussianity Speaker(s): Enrico Pajer
Abstract: Two of the most exciting observables in the cosmic microwave background (CMB) radiation, which could deeply impact our picture of the early universe, are non-Gaussianity and tensor modes. A potential detection of tensor modes can be explained in terms of a model of large field inflation. Theoretical... read more
Date: 16/03/2010 - 11:00 am
Series: String Seminars
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PIRSA:09050063
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Inflation from axion monodromy Speaker(s): Enrico Pajer
Abstract: TBA
Date: 22/05/2009 - 2:00 pm
Collection: Effective Field Theories in Inflation
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