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The TIARA target chamber is designed specifically to allow charged
particle and gamma-ray coincidences to be studied efficiently for a large range
of reactions using radioactive beams. The primary design objectives may
therefore be summarized as:
- the charged particle array should be as compact as possible, to fit
inside the most efficiently configured gamma-ray array available,
- the charged particle coverage should be as close to
as possible,
- the charged particle detectors should not interfere with the gamma-ray
detection,
and these criteria have largely determined the rest of the general design. It
has been a guiding principle that any compromises necessarily introduced by
engineering constraints should be in other properties of the array and not in
these main objectives. This, in turn, introduces major challenges into the
detailed design, for example with target changing, beam alignment, access to
detectors, signal connections, flange connections, etc. In an initial design
study, it has been possible to identify solutions in principle to all of these
problems and to provide an estimate of the construction costs for the chamber.
In summary, therefore, the main component of the array is a small chamber to
house the central part of the silicon array, to fit inside the most closely packed
geometry of the Exogam gamma-ray array. This chamber is shown in fig.
5.
Figure 5:
Main vacuum vessel for the TIARA array, viewed from the
back.
![\begin{figure}
~\\
\mbox{} \hfill \framebox[0.95\textwidth]{\rule{0cm}{0.45\textheight}{\footnotesize TIARA vacuum vessel}}\hfill \mbox{}
\end{figure}](img28.gif) |
The forward and rear parts of the
silicon array are allowed to fill a larger volume as they are further from the
target and out of the way of the gamma-ray detectors. A plunger that enters
through a small gap in the silicon array is used for target changing. In order
to protect the fragility and alignment of the central vacuum vessel and
silicon detectors, and of course also to protect the heavy gamma-ray detectors
themselves, a substantial framework is necessary to support the Exogam
detectors. The best way to assure the safety of the Exogam detectors during
their operation with TIARA was to use Exogam's own detector support structure
and to mount TIARA within in. However, the design study revealed that this was
not possible owing to some specific properties of the Exogam support. As an
alternative, a close copy of the framework for supporting the ring of
gamma-ray detectors was adapted for TIARA. As an added benefit, this structure
will allow the possibility of setting up TIARA independently, so for example if
Exogam were set up on the VAMOS spectrometer with its maximum complement of 12
detectors for that application, then TIARA could be set up on an adjacent beam
line with the remaining 4 Exogam detectors mounted in the gamma-cube geometry.
Next: Flexible modes of operation
Up: Design of the TIARA
Previous: Design of the TIARA
Wilton Catford
2000-11-03