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- W2765343018 abstract "The Cosmic Neutrino Background is a prediction of the standard cosmological model, but it has been never observed directly. In the experiments with the aim of detecting relic CNB neutrinos, currently under development, the expected event rate depends on the local density of relic neutrinos. Since massive neutrinos can be attracted by the gravitational potential of our galaxy and cluster around it, a local overdensity of cosmic neutrinos should exist. Considering the minimal masses guaranteed by neutrino oscillations, we review the computation of the local density of relic neutrinos and we present realistic prospects for a PTOLEMY-like experiment." @default.
- W2765343018 created "2017-11-10" @default.
- W2765343018 creator A5070455391 @default.
- W2765343018 date "2017-10-18" @default.
- W2765343018 modified "2023-09-27" @default.
- W2765343018 title "Neutrino clustering in the Milky Way" @default.
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