Nonlinear growing neutrino cosmology

The energy scale of dark energy, ∼2×10−3 eV, is a long way off compared to all known fundamental scales—except for the neutrino masses. If dark energy is dynamical and couples to neutrinos, this is no longer a coincidence. The time at which dark energy starts to behave as an effective cosmological c...

Full description

Bibliographic Details

Main Authors:	Ayaita, Youness (Author) , Baldi, Marco (Author) , Führer, Florian (Author) , Puchwein, Ewald (Author) , Wetterich, Christof (Author)
Format:	Article (Journal)
Language:	English
Published:	11 March 2016
In:	Physical review Year: 2016, Volume: 93, Issue: 6
ISSN:	2470-0029
DOI:	10.1103/PhysRevD.93.063511
Online Access:	Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.93.063511 Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.93.063511
Author Notes:	Youness Ayaita, Marco Baldi, Florian Führer, Ewald Puchwein, and Christof Wetterich