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Neutrino charge constraints from scattering to the weak gravity conjecture to neutron stars
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In various extensions of the Standard Model of particle physics, and intriguingly even in the three-generation Standard Model without neutrino masses, neutrinos are allowed to have very tiny electric charges. After a review of the theoretical scenarios that allow the emergence of such charges, we discuss the existing observational limits and we derive new stringent direct upper bounds for the charges of the muon and tau neutrinos. We also point out a flavor-universal lower bound on neutrino charges which is obtained from the weak gravity conjecture, that is based on the hypothesis that gravity is the weakest force. We finally present a new flavor-universal upper bound on neutrino charges based on astrophysical observations of Magnetars.
Forward citations
Cited by 2 Pith papers
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Probing Terrestrial Relic Neutrino Charge with Mach-Zehnder Interferometer
A Mach-Zehnder interferometer with one vertical arm is proposed to probe relic neutrino charge, with claimed sensitivity down to epsilon_nu ~ 10^-22, but the signal calculation is flawed.
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How Charged Can Neutrinos Be?
Mini-charged neutrinos are viable only for flavor-universal U(1)_X extensions such as U(1)_{B-L} and U(1)_L, and their experimental constraints are model-dependent, with upper bounds ranging from 10^-19 e to 10^-21 e.
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