Future precision cosmology and neutrinos
March 02, 2017
June 20, 2017
In the next decade future measurements of the Cosmic Microwave Background anisotropies are expected to reach the sensitivity
to constrain the inverse and direct neutrino hierarchies. A cosmological detection of non-zero neutrino mass seems therefore around
the corner. However one important aspect is often neglected: current predictions are done under the assumption of the standard
$\Lambda$CDM model, while several hints for tensions and anomalies are currently present in current data that stills leave as open
the possibility of new physics.
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