Clustering in growing neutrino cosmologies
Valeria Pettorino, David F. Mota, Georg Robbers, Christof Wetterich

TL;DR
Growing neutrino cosmologies predict significant neutrino clustering at supercluster scales, potentially revealing a new force mediated by dark energy scalar fields, with observable large-scale structures forming around redshift 1.
Contribution
This paper demonstrates that growing neutrino models can produce large-scale neutrino clustering and suggests observable signatures of a new force beyond gravity.
Findings
Neutrino lumps form at redshift ~1
Neutrino clustering influences dark matter distribution
Large-scale structures could indicate a new scalar-mediated force
Abstract
We show that growing neutrino models, in which the growing neutrino mass stops the dynamical evolution of a dark energy scalar field, lead to a substantial neutrino clustering on the scales of superclusters. Nonlinear neutrino lumps form at redshift z ~ 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 force stronger than gravity and mediated by the 'cosmon' dark energy scalar field.
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