[Primex] preparations for the PrimEx-II run
Ashot Gasparian
gasparan at jlab.org
Sun Feb 7 19:58:48 EST 2010
Dear PrimEx-II Collaborators,
The chances are increasing that the PrimEx-II experiment
may run earlier than it is currently listed in the schedule.
There is a high probability that we may run in the fall of
this year or in the beginning of the next year. The final
decision, looks like, will be made sometime in April/May.
In all cases we have extremely short time to prepare the
experiment itself and the experimental setup to reach the
long promised 1.4% precision. This task is getting more
difficult when we look at the availability of Hall B to
work on our setup. There are ONLY to time periods for this
work, one is already ongoing and it will end in March 10
with the closing of Hall B. The next opening is scheduled
from the middle of July to sometime in August 20.
Besides the inspection and preparation of the previous
experimental setup to make it physically ready for the new
run, we have to come up with critical improvements in the
setup to reach the promised (in PAC33) more statistics
(with the approved less beam time) and control of all
backgrounds in the data set to possibly reach the stable
and controllable extraction of the decay width on a
percent level.
Summarizing many discussions on this subject, done in the
past, here is the itemized list of work for those possible
improvements:
1)The statistics: the only effective way to improve the
statistics is to revisit the DAQ system and increase
the event rate for more than a factor of 5 ( ~ 5KHz).
This was discussed in the PAC33.
Some initial activities are already started on this part.
Any suggestions or comments are more than welcomed.
2)Redaction of the backgrounds: up to now we came up with
a 3 major ways to significantly decrease the backgrounds
in the experiment:
a)e+e- background possibly coming from the collimators
and deflected by the permanent magnet. This background
is reflected in the Compton data, therefore it is not
a direct contribution for the pi0 data set. However,
given to the importance of the Compton, we need to fix
it. Some very initial work already started to try to
increase the Bdl of the permanent magnet.
Any help and idea are more than welcomed.
b)The veto counters are critical for the charged background
redaction. It was initially designed on that way and we
also saw their importance in the background redaction
process in data analysis.
We need to inspect the veto counters. If it is necessary
we need to redo them to provide a robust set of "veto
efficiencies" with their well known errors for the entire
HyCal calorimeter.
This process needs to start now.
c)Timing information from HyCal channels: We hope that if
we instrument each channel (or in wars case, each summing
group) of the HyCal with a TDC, that will significantly
help to reduce the accidental background in the experiment.
This needs more work and electronics. But, given to its
importance, we need to try everything possible to do that.
Initial work is already started, TDCs are potentially
located, but we need to come up with the discriminators
and cabling. Any help on this part is more than welcomed.
For sure, items listed above are subject for more discussions
and improvements. Given to the short time left for the
preparation we need to effectively combine email discussions
with the Friday meetings.
We are critically short with onsite manpower to work on the
setup. We need more onsite manpower (professors, postdocs,
students) now, for the summer period and during the run.
Please come up with your contributions on this important
part of the collaborative work for the successful preparation
of the PrimEx-II setup and the run.
Best regards,
Ashot
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Ashot Gasparian Phone:(336)285-2112 (NC A&T)
Professor of Physics
Physics Department (757)-269-7914 JLab
NC A&T State University Fax:(757)-269-6273 JLab
Greensboro, NC 27411 email: gasparan at jlab.org
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