Observational constraints on varying neutrino-mass cosmology

2016

Closed access Metadata (CSL-JSON)
DOI 10.1088/1475-7516/2016/01/049
Data confidence 85 high
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Abstract

We consider generic models of quintessence and we investigate the influence of massive neutrino matter with field-dependent masses on the matter power spectrum. In case of minimally coupled neutrino matter, we examine the effect in tracker models with inverse power-law and double exponential potentials. We present detailed investigations for the scaling field with a steep exponential potential, non-minimally coupled to massive neutrino matter, and we derive constraints on field-dependent neutrino masses from the observational data.