Neutrino Magnetic Moment and the Process e → e γ
Abstract
The contribution of a neutrino magnetic moment μ to the cross section of the process e-→ e- γ has been calculated and compared with the Standard Electroweak one. The radiative process allows to reach low enough values of Q2 without the need to operate at very small energies of recoil electrons. Regions in the phase space which are more favourable to set bounds on μ are suggested.
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