Constraining the neutrino mass using a multi-tracer combination of two galaxy surveys and CMB lensing

Abstract

Measuring the total neutrino mass is one of the most exciting opportunities available with next-generation cosmological data sets. We study the possibility of detecting the total neutrino mass using large-scale clustering in 21cm intensity mapping and photometric galaxy surveys, together with CMB information. We include the scale-dependent halo bias contribution due to the presence of massive neutrinos, and use a multi-tracer analysis in order to reduce cosmic variance. The multi-tracer combination of an SKAO-MID 21cm intensity map with Stage~4 CMB dramatically shrinks the uncertainty on total neutrino mass to $\sigma (M_{\nu })\simeq 45$meV, using only linear clustering information ($k_{\max }=0.1h/$Mpc) and without a prior on optical depth. When we add to the multi-tracer the clustering information expected from LSST, the forecast is $\sigma (M_{\nu })\simeq 12$meV.

3 figures, 3 tables, 7 pages

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Cited by in corpus (5)

• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Neutrino winds on the sky
• A wide-angle formulation of foreground filters for HI intensity mapping
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping