GlueX Luminosity Limits
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Transcript GlueX Luminosity Limits
GlueX Collaboration Meeting, Newport News, May 8-10, 2008
GlueX Luminosity Limits
Richard Jones, University of Connecticut
1. Design luminosity
2. Physics possibilities at higher luminosities
3. Limiting factors in current design
Design Luminosity
Goal – produce sufficient samples of exclusive reations to
be systematics-limited (maximum sensitivity to weak exotic
waves) in amplitude analysis for key channels.
Translation – when that occurs depends on the final state,
ie. specific backgrounds, PID demands, …
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Rule of thumb: 10 events is sufficient for a decent PWA
Consider a hypothetical case:
s = 50 nb
BR = 30%
e
= 25%
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Design Luminosity
L
= .071 g 3
cm
x
30 cm
x
6.0 1023 1
g
x
2
10-33 cm
nb
x
Ibeam
= 1.3 10-9 nb-1 x Ibeam
At Ibeam = 10 g/s, it would take 57 khr (~ 20 years) to
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collect these statistics.
At Ibeam = 10 g/s, it would take 6 khr (~ 2 years) to collect
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these statistics.
Result: 10 g/s is sufficient to complete the hybrid
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spectroscopy program. But is it optimal ?
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Design Luminosity
Define: tagger figure of merit
• Factor that rescales the
amount of run time needed
to reach a given level of
statistical error in a tagged
histogram.
• Reference for FOM shown
is the GlueX tagged beam
under nominal conditions at
9 GeV, but with no mistags.
1. Assumes detector identifies correct
beam bucket 100% of the time.
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2. Shows some gains up to 3 10 Hz.
3. Gains are only about 25% for factor
3 in backgrounds.
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Design Luminosity
For 25% more statistics, what do we lose?
x3 radiation damage in FCal
x3 accidentals in the TOF and Start
x3 pileup in the FDC, extra tracks, etc.
x3 in channel count in the microscope – $$$
x3 in radiator thickness – reduced polarization
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Design Luminosity
If this argument was not made before, what
was the basis of the design goal of 10 g/s?
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the intuitive criterion of 50% accidental tags
evidence from Monte Carlo simulation that detector
backgrounds are going to preclude higher luminosities
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1. FCal radiation damage – already an issue at 10
2. TOF occupancy – within a factor of 3-5 of ceiling
3. FDC pileup and extra tracks – within factor of 3-5
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Physics at Higher Luminosity
What physics might make this interesting?
inverse DVCS – looks feasible
threshold J/Y – statistically difficult
Cascade baryons – needs kaon PID
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Beam Limiting Factors
Tagging near the end-point
no polarization
no significant collimation
amorphous radiator – factor 100 more luminosity
available (if untagged)
current tagger design has full coverage over
9-11.4 GeV, designed to run up to 50 MHz / GeV.
at 50 MHz / GeV in end-point region, detector
backgrounds are comparable to nominal conditions
with polarized beam at 108 g/s.
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Detector Limiting Factors
FCal radiation damage
Inner blocks could be shielded, giving up lowangle g acceptance, ok for some physics.
FTOF occupancy
ditto.
FDC pile-up – will be ultimate limiting factor.
essential for just about any physics
no effective means to shield them
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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Conclusions
Design luminosity is optimized for carrying out the hybrid
spectroscopy program.
Nominal high-intensity running conditions are consistent
with tagging at 50 MHz / GeV at the end-point.
The photon source will produce as much intensity as the
experiment can handle in any scenario.
With a dedicated end-point tagger, one can tag effectively
up to 250 MHz, provided the detector can trigger.
With 250 MHz on 11 < Eg < 12 GeV, detector background
would be x5 nominal, probably an upper limit.
FDC pile-up will be the limiting factor – how to estimate it?
GlueX Collaboration Meeting, Newport News,
May 8-10, 2008
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