We derive in full generality the equations that govern the time dependence of
the energy of the decay electrons in a muon experiment. We
include both electromagnetic and gravitational effects and we estimate possible
systematics on the measurements of , whose experimental
uncertainty will soon reach . In addition to the
standard modulation of when the motion is orthogonal to a
constant magnetic field , with angular frequency , we
study effects due to: (1) a non constant muon factor, in presence of
electric fields , (2) a correction due to a component of the muon velocity
along (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 ${\mathcal E}$ 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
and subleading effects of
about $\Delta \omega_a/\omega_a \approx {\rm few} \times {\cal
O}(10^{-8}-10^{-9})E$ fields. Finally we show that GR effects are
dominated by the Coriolis force, due to the Earth rotation with angular
frequency , leading to a correction of about $\Delta
\omega_a/\omega_a \approx \omega_T/(\gamma \omega_a) \approx {\cal
O}(10^{-12})$. A similar correction might be more appreciable for future
electron experiments, being of order $\Delta \omega_a/\omega_{a, {\rm
el}} \approx \omega_T/(\omega_{a, {\rm el}}) \approx 7\times 10^{-13}$,
compared to the present experimental uncertainty, $\Delta a_{\rm el}/a_{\rm
el}\approx 10^{-10}\Delta a_{\rm el}/a_{\rm
el}\approx 10^{-11}$.

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