The efficiencies for the delayed electron and telescope cuts were determined
from the ratio of the
signal yields with and without the Del
cuts. From each spectrum the background was subtracted,
usually using a pure H2 target in which no fusion takes
place
.
The
events were selected with an energy cut of [2000, 3700] ch,
and a time cut of [0.02, 0.4]
s was applied to the Si signals.
Columns 3 to 5 in Table 6.17 show the Del cut
efficiency,
for Si1, Si2, and their average. Run A is
the same as that in Tables 6.14 and
6.15. Run C was similar to A but had no downstream
layers (500 T
H2 and 3 T
D2 were present for Run A).
Run D had a 6 T
upstream overlayer (as opposed to 14 T
as
in others), testing possible effects of the layer thickness and the
reaction depth. Given in brackets for
are statistical
errors. Run A had sufficient statistics, while Runs C and D, as well as
Del-t cuts (Tel1, Tel2) had relatively poor statistical precision.
Some variations of the Del cut efficiencies are observed in
Table 6.17: Run C and D have a lower
than
A by 2 to 3
,
possibly pointing to a systematic effect due to the
target conditions.
The interpretation of the
results requires some caution;
recall that in the present analysis, detection of the fusion reactions is
used to tag the muon as a well-defined source for the electron, into which
it decays. Detecting the fusion
,
however, biases the electron
source to preferentially concentrate towards the region where the
acceptance for the particular Si detector is higher, e.g., the
beam-left edge of the target for Si1 (see Fig. 3.18,
page
). The overall efficiency of the Del cuts, which
is a convolution of the
particle acceptance in the Si detector and
the electron acceptance in the scintillators (telescope), is thus higher in
the case of the Del coincidence in the same side of the target than that in
the opposite side (Fig 3.18); e.g., for Si1,
is higher for Ege at the beam left than En1 at the beam right, as
can be seen in Table 6.17. This acceptance bias effect can
be largely avoided by taking the average of Si1 and Si2, yet the effect
persists to increase
(unless the target is infinitely
small), and is at the several percent level in our case.
On the other hand, the downstream electron detectors (En2, Tel2), which
were on the beam (Z) axis (as opposed to the perpendicular axis (X)),
are less susceptible to the bias effect, since they have relatively uniform
acceptance over the entire target. This can be seen in the consistency
between Si1 and Si2 in
for En2 and Tel2 in
Table 6.17. En2 and Tel2, which have lower values of
,
are thus more reliable compared to other detectors.
With all the factors in Eq. 6.26 determined, the stopping
fraction with the absolute yield method can now be computed and the results
are given in the last column of Table 6.17. The error includes
3.6% systematic uncertainty due to the delayed electron life time,
,
which dominates the total error for Run A, but is comparable to
the statistical error for Runs C and D. The values in bold face are for the
detectors downstream (En2, Tel2), which are more reliable than other
detectors, as discussed above. Among these
SFABSHvalues for En2 and Tel2, there are about % variations depending on
the target conditions or the choice of the detector (i.e., En2 versus
Tel2), which indicates a measure of further systematic effects. Note that
unlike the case for the relative amplitude method, in which there was some
30% discrepancy in
between the scintillators and
telescopes (see Table 6.6 in page and
6.8 in page
), the results in the two
detectors are nearly consistent in the absolute yield method here. Taking
the average of the two extremes of the downstream
SFABSH, we quote
,
where with the assumption that the
uncertainty is dominated by the systematics, the 5% error is given by a
quadratic addition of the 3.6% systematic error from each measurement
and 3.3% due to run variations.