The question of how to describe a natural ultraviolet cutoff in an expanding space-time is of significance in several respects. First, it concerns the fate of general covariance in the presence of a natural UV cutoff. Second, it concerns the continued generating of degrees of freedom through expansion, which carries with it the possibility of an associated generating of vacuum energy. Finally, through inflation, a natural ultraviolet cutoff may have left observable imprints in the CMB.
Organizer(s): Justin Khoury
Collection URL: http://pirsa.org/C06011
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PIRSA:06090029
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Thoughts on vacuum growth Speaker(s): Ted Jacobson
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Date: 06/09/2006 - 5:00 pm
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PIRSA:06090033
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Effective actions for gravity Speaker(s): Koenraad Schalm
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Date: 07/09/2006 - 9:00 am
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PIRSA:06090030
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QFT with minimum length Speaker(s): Sabine Hossenfelder
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Date: 08/09/2006 - 9:00 am
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PIRSA:06090031
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Generalized Uncertainty Principle Speaker(s): Ulrich Harbach
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Date: 08/09/2006 - 11:00 am
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PIRSA:06090032
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Inflationary cosmological pertubations of quantum mechanical origin Speaker(s): Jerome Martin
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Date: 08/09/2006 - 12:00 pm
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