In our proposed staged approach to this measurement we will first need
a low intensity continuous muon beam, then an intermediate intensity
beam, and finally a high intensity chopped beam. The properties of
the existing PSI beam lines are well described in documents available
on the WWW. For each beam line the flux, focus, purity and other
properties are given. It is clear that several of the beam lines can
provide surface muon and/or low energy muon fluxes at low and
intermediate intensities, e.g. E1. It is also clear that some
beam lines can provide muon fluxes comfortably in excess of 107 Hz.
For example,
E3 provides in its achromatic mode a surface muon
flux of 6 x 107 Hz per mA of primary protons. With such an
initial flux, even at a 10% duty factor, the primary requirement of
12 muons collected in 1
s can be realized. Beam line
E3 was
chosen by Kammel et al. [3] for their
chopped-beam feasibility studies. There would be no difficulty in
using, for example,
M3 for our low and intermediate intensity
work, and the chopped-beam facility for our high intensity. The above
mentioned beam lines also have appropriate focus and purity.
The chopped beam is central to the lifetime measurement. Three
parameters serve to describe the beam: the rise and fall times, the
repetition rate, and the extinction factor. The beam developed at
LAMPF, described by Ciskowski et al.[17], had rise
and fall times of 100 ns, a maximum repetition rate of 100 kHz, and an
extinction factor of 0.3%. In their work they would collect muons
for 1 to 5 s and count for 10 to 20
s. These times are well
matched to the lifetime measurement. The extinction factor could,
perhaps, have been better if the chopper were located further
upstream, allowing magnet elements to deflect scattered muons. The
extinction factor is not critical because it is monitored continuously
with the highly efficient beam scintillator. It is clear then that an
appropriate chopped beam is technically feasible. This conclusion is
also made in the LOI of Kammel et al. [3].
The surface muon beam has a range of approximately 150 mg/cm2.
This limited range requires some attention to materials in the beam
path. The muon beam can exit through the standard 150 m mylar
window. Upstream of this window in the beam line vacuum, we would
suspend a 200
m thick scintillator, which would be viewed
directly by two photomultiplier tubes. A surface muon would deposit
sufficient energy in the scintillator to provide approximately a 50
photoelectron signal in each photomultiplier tube. This signal should
provide for greater than 99% efficient detection of beam particles.
A highly efficient beam counter is needed to detect errant muon
injection during the measuring period. This counter will be monitored
using the same waveform digitizers which we will use for the detector
timing tiles as described later.
The µLan Detector will be placed directly downstream of the
vacuum window. The beam then must be transported 28 cm to the
stopping target. The beam must be transported through helium to
minimize multiple scattering. The detector allows the insertion of up
to a 5.7 cm diameter cylinder. Helium at slightly above one
atmosphere pressure can be efficiently contained in a 25 m
aluminized nylon bag. At least two stopping targets will be employed.
We will use a non-depolarizing target such as Al for studies of the
asymmetry of the detector. For the main experiment, a sulfur target
of 1 mm thickness will be suspended in the helium bag. The stopping
target would be approximately 5 cm in diameter. Multiple scattering
in the beam scintillator and vacuum window together would produce a
beam spot of 1.1 cm rms. This multiple scattering increases
only slightly the typical beam focus of
20 x 30 mm2. The
sulfur target is known [18] to depolarize the muon
distribution to a level below approximately 3%. We will assume
that the muon population has a residual polarization of 3% in the
systematic studies which are outlined in a later section.