25 June 2007 to 10 August 2007
CERN PH-TH
Europe/Zurich timezone

Session

Seminar

9 Aug 2007, 14:00
CERN PH-TH

CERN PH-TH

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  1. Christof Wetterich
    09/08/2007, 14:00
    Seminar
    The time evolution of a cosmological scalar field can be stopped by an increasing mass of the neutrinos. This leads to a transition from a cosmological scaling solution with dynamical dark energy at early time to a cosmological constant dominated universe at late time. The trigger for the transition is set at the time when the neutrinos become non-relativistic. This is a possible...
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