The intensities of the X-ray yields in the and atoms calculated with the Monte Carlo code [62,56] are shown in Table 3. The cascade model used is in good agreement with the experimental data on the X-ray yields [63] and in fair agreement with data [56,64].
|
Important for the proposed experiment is the fact that the muonic and transitions are about an order of magnitude stronger than the corresponding pionic transitions. This compensates the lower stop efficiency for muons. An extension of the measurement to the transition can also be considered; the intensity, however, decreases significantly for higher pressures. In addition the Bragg angles are becoming small and make this transition unfavorable. Rate estimates based on the yields of Table 3 are given in chapter 3.6.
In Figures 1 -4 calculated distributions of kinetic energies are shown for a pressure of 15 for the exotic hydrogen atoms at the instant of the and the transition. (We always give the values for the pressures at a temperature of 293K.) The influence of these distributions on the form of the X-ray lines is depicted in Fig. 8-9.
|
|
|
|