Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-02-11
Phys.Lett.B663:160-164,2008
Astronomy and Astrophysics
Astrophysics
6 pages, 5 figures
Scientific paper
10.1016/j.physletb.2008.03.060
A growing neutrino mass can stop the dynamical evolution of a dark energy scalar field, thus explaining the 'why now' problem. We show that such models lead to a substantial neutrino clustering on the scales of superclusters. Nonlinear neutrino lumps form at redshift z \sim 1 and could partially drag the clustering of dark matter. If observed, large scale non-linear structures could be an indication for a new attractive 'cosmon force' stronger than gravity.
Mota David F.
Pettorino Valeria
Robbers Georg
Wetterich Christof
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