Neutrino forces in neutrino backgrounds

Abstract

The Standard Model predicts a long-range force, proportional to $G_F^2/r^5$, between fermions due to the exchange of a pair of neutrinos. This quantum force is feeble and has not been observed yet. In this paper, we compute this force in the presence of neutrino backgrounds, both for isotropic and directional background neutrinos. We find that for the case of directional background the force can have a $1/r$ dependence and it can be significantly enhanced compared to the vacuum case. In particular, background effects caused by reactor, solar, and supernova neutrinos enhance the force by many orders of magnitude. The enhancement, however, occurs only in the direction parallel to the direction of the background neutrinos. We discuss the experimental prospects of detecting the neutrino force in neutrino backgrounds and find that the effect is close to the available sensitivity of the current fifth force experiments. Yet, the angular spread of the neutrino flux and that of the test masses reduce the strength of this force. The results are encouraging and a detailed experimental study is called for to check if the effect can be probed.

v4: 38 pages, 5 figures, 4 tables, correction of a factor of 2 for neutrino forces in the cosmic neutrino background in Section 3

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• On neutrino-mediated potentials in a neutrino background
• Detecting Ultralight Dark Matter with Matter Effect
• Neutrino force at all length scales
• Probing Long-Range Forces Between Neutrinos with Cosmic Structures
• The dark Stodolsky effect: constraining effective dark matter operators with spin-dependent interactions
• Neutrino Effects on Atomic Measurements of the Weinberg Angle