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2016

Tests of Neutrino and Dark Radiation Models from Galaxy and CMB surveys

Banerjee, Arka, Jain, Bhuvnesh, Dalal, Neal et al.

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We analyze the ability of galaxy and CMB lensing surveys to constrain massive neutrinos and new models of dark radiation.

We present a Fisher forecast analysis for neutrino mass constraints with the LSST galaxy survey and the CMB S4 survey.
A joint analysis of the three galaxy and shear 2-point functions, along with key systematics parameters and Planck priors, constrains the neutrino masses to $\sum m_\nu = 0.041\,$eV at 1-$\sigma$ level, comparable to constraints expected from Stage 4 CMB lensing.
If low redshift information from upcoming spectroscopic surveys like DESI is included, the constraint becomes $\sum m_\nu = 0.032\,$eV.

Tests of Neutrino and Dark Radiation Models from Galaxy and CMB surveys · Around

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