The comparison of the calculated Doppler broadening of the
and
lines with the result of the proposed experiment
will allow us to perform a fine tuning of the Coulomb and deceleration rates.
The
data on the kinetic energy distribution obtained with the
nToF method will also be used for this goal. By transferring this information
into the
part of the cascade calculations we are confident
that the current uncertainties in the calculated energy distributions of the
atom at the instant of the X-ray transitions will be reduced
to the level allowing to predict the Doppler broadening correction to the X-ray
lines profile with an error of better than 1% in the hadronic width.