The MICE TPG
project
Status and
links
prepared
by Alain Blondel, Uni Geneva.
This
note describes the proposal of a Time Projection chamber for MICE with
GEM read out. It is understood as a beginner’s introduction with the sake
of providing references for those interested in the project.
The
MICE LOI submitted to PSI and RAL can be found here:
http://proj-bdl-nice.web.cern.ch/proj-bdl-nice/cool/loi-final-ral.pdf
One
can see there that the tracking devices that were considered in November
2001 were either scintillating fiber trackers or silicon trackers. A sketch
of MICE with these trackers is here: http://proj-bdl-nice.web.cern.ch/proj-bdl-nice/cool/micesketchold.pdf
One
of the problems of these proposals was the expected noise from photons
and electrons generated by the RF cavities of the cooling section. In particular,
the combination of inefficiencies in the scintillating fibers and noise
made it feared that reconstruction would be seriously hampered by ambiguities.
G. Barr discussed this in this note:
http://proj-bdl-nice.web.cern.ch/proj-bdl-nice/cool/barrnoisenote.pdf
In
February 2002 Ugo Gastaldi suggested
that one could use a TPC with GEM readout for the trackers of MICE. The
first ideas and sketches together with a possible scheme for the readout
can be found in this talk:
http://proj-bdl-nice.web.cern.ch/proj-bdl-nice/talks/ugo.pdf,
or
in the draft note: http://proj-bdl-nice.web.cern.ch/proj-bdl-nice/cool/gastalditpgdraft.pdf
These
were presented in one of the MICE detector working groups meetings
http://hep04.phys.iit.edu/cooldemo/detectors/detectors.html
see
the March meeting:
http://hep04.phys.iit.edu/cooldemo/detectors/detectormeetingMar2002.html
This
having a rather imprecise timing information (100 ns time slots at least)
it would have to be complemented with at least one plane of scintillating
fibers and a segmented time-of-flight system. Nevertheless, the fact that
it could provide hundreds of space points along a track with potentially
very small multiple scattering (for a He-isobutene filled TPG) allied with
very small mass for photon conversions, make it a very interesting option.
The space resolution with Helium filling needs to be evaluated.
The
readout has been discussed by
Emilio
Radicioni and seems to be quite OK:
http://proj-bdl-nice.web.cern.ch/proj-bdl-nice/cool/tpgemiliomarch2002.pdf
Finally
the issue of pulling out the signals will have to be investigated in detail,
for reasons of noise and of the relationships with the other detectors.
A possible sketch of how to do this for the downstream spectrometer can
be found here.
http://proj-bdl-nice.web.cern.ch/proj-bdl-nice/cool/micesketch.pdf
What
needs to be done?
The
first and most urgent thing to do in my opinion is to begin the hardware
test of the readout cleanliness in the vicinity of a mega-monster: the
RF cavities are a mere three meters away in the MICE set up and at the
time when the muons pass by there are being powered by an instantaneous
power of 4 MW! this is bound to require very careful shielding of the readout
system, if it can work at all.
Also
needed is a simulation of the performance of this device plugging in first
the space resolution as function of drift time, then the possible effect
of noise.