On systematic and GR effects on muon g-2 experiments

Abstract

We derive in full generality the equations that govern the time dependence of the energy E of the decay electrons in a muon g-2 experiment. We include both electromagnetic and gravitational effects and we estimate possible systematics on the measurements of g-2 2(1+a), whose experimental uncertainty will soon reach a/a≈ 10-7. In addition to the standard modulation of E when the motion is orthogonal to a constant magnetic field B, with angular frequency ωa=e a |B|/m, we study effects due to: (1) a non constant muon γ factor, in presence of electric fields E, (2) a correction due to a component of the muon velocity along B (the `pitch correction'), (3) corrections to the precession rate due to E fields, (4) non-trivial spacetime metrics. Oscillations along the radial and vertical directions of the muon lead to oscillations in E with a relative size of order 10-6, for the BNL g-2 experiment. We then find a subleading effect in the `pitch' correction, leading to a frequency shift of ωa/ωa ≈ O(10-9) and subleading effects of about ωa/ωa ≈ few × O(10-8-10-9) due to E fields. Finally we show that GR effects are dominated by the Coriolis force, due to the Earth rotation with angular frequency ωT, leading to a correction of about ωa/ωa ≈ ωT/(γ ωa) ≈ O(10-12). A similar correction might be more appreciable for future electron g-2 experiments, being of order ωa/ωa, el ≈ ωT/(ωa, el) ≈ 7× 10-13, compared to the present experimental uncertainty, a el/a el≈ 10-10, and forecasted to reach soon a el/a el≈ 10-11.

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