Neutrino magnetic moments meet precision N eff measurements

Abstract

Abstract In the early universe, Dirac neutrino magnetic moments due to their chirality-flipping nature could lead to thermal production of right-handed neutrinos, which would make a significant contribution to the effective neutrino number, N eff. We present in this paper a dedicated computation of the neutrino chirality-flipping rate in the thermal plasma. With a careful and consistent treatment of soft scattering and the plasmon effect in finite temperature field theories, we find that neutrino magnetic moments above 2.7 × 10 −12 μ B have been excluded by current CMB and BBN measurements of N eff, assuming flavor-universal and diagonal magnetic moments for all three generation of neutrinos. This limit is stronger than the latest bounds from XENONnT and LUX-ZEPLIN experiments and comparable with those from stellar cooling considerations.

Keywords

• Cosmology of Theories BSM
• Early Universe Particle Physics
• Neutrino Interactions
• Non-Standard Neutrino Properties