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2011

Neutrino Halos in Clusters of Galaxies and their Weak Lensing Signature

Villaescusa-Navarro, Francisco, Miralda-Escudé, Jordi, Peña-Garay, Carlos et al.

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We study whether non-linear gravitational effects of relic neutrinos on the development of clustering and large-scale structure may be observable by weak gravitational lensing.

We compute the density profile of relic massive neutrinos in a spherical model of a cluster of galaxies, for several neutrino mass schemes and cluster masses.
Relic neutrinos add a small perturbation to the mass profile, making it more extended in the outer parts.
In principle, this non-linear neutrino perturbation is detectable in an all-sky weak lensing survey such as EUCLID by averaging the shear profile of a large fraction of the visible massive clusters in the universe, or from its signature in the general weak lensing power spectrum or its cross-spectrum with galaxies.

Neutrino Halos in Clusters of Galaxies and their Weak Lensing Signature · Around

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