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Options for E906/Drell-Yan with a Solid Iron Magnet (Fe906?) Paul E. Reimer 20 June 2008. Solid Iron magnet Target dump separation Chamber rates Resolution—Mass, x F , x 1 , x 2 Acceptance. Why a Solid Iron Magnet?. E906 budget is very tight. - PowerPoint PPT Presentation
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Options for E906/Drell-Yan with a
Solid Iron Magnet(Fe906?)
Paul E. Reimer20 June 2008
1. Solid Iron magnet
2. Target dump separation
3. Chamber rates
4. Resolution—Mass, xF, x1, x2
5. Acceptance
220 June 2008 Paul E. Reimer
Why a Solid Iron Magnet?
E906 budget is very tight. – We are expecting ≈$2M for DOE/Nuclear Physics. Of this $1.6M will be used to produce
coils for an open aperture magnet. The remainder is for spectrometer upgrades.– NSF, Taiwan and Japan are planning contributions to the spectrometer upgrades
Fermilab has requested that we contribute an additional $1.5M for M&S that they need to spend for E906
– Some tasks e.g. flammable gas system (Illinois) and cryotargets may be done by collaborators.
– RIKEN may to contribute ≈$600k to “common fund” items– Still short ≈$500k
Solid Iron Magnet– Essentially free—coils and iron exist, Iron must be cut ($100k)– Reprogram DOE/ONP funds to Fermilab (Under discussion with Brad Tippens)
– Increased acceptance--larger “aperture” (if you can call it that)– Decreased resolution
320 June 2008 Paul E. Reimer
Magnet Description
Use existing coils from SM3
– 3 coil packs:
191, 163 or 135 inch coils
– Iron blocks from SM12 (E866) magnet
– Simulations shown for 191” Suggested by Chuck BrownSuggested by Chuck Brown 135”
191”
SM3 coils which were constructed in 1981 for E605 by Sumitomo and supervised by KEK and Kyoto. Supervised by Prof. Miyake, Dr. Maki and Dr. Sakai
420 June 2008 Paul E. Reimer
Magnet Description
Use existing coils from SM3
– 3 coil packs
– 191, 163 or 135 inch coils
– Simulations shown for 189” Issues:
– Target/dump separation
– Chamber rates
– Mass Resolution
– x2 resolution
– Field simulation • no measurements• Accurately determine saturation curve
– Acceptance (i.e. statistical uncertainty at the end of the day)
Field simulation for 189” solid Fe magnet (DFG)
520 June 2008 Paul E. Reimer
Dump/Target Separation
Resolution significantly worse
Trigger and reconstruction cuts allow for clean separation
– Remove events with tracks at dump face within 2.25” of beam axis
– Remove events with tracks greater than 10” from beam axis at targets
Recall dump starts at 0”. These cuts effectively remove all events from the front of the dump!!
Target
Open aperture in redSolid Fe in Blue
Dump
DumpTarg
et
Slight problem from dump J/’s
620 June 2008 Paul E. Reimer
Dump/Target Sep., Solid Fe Magnet Only Target—solid histograms
-70 < z < -50 Dump—dashed histo.
0<z
Magenta, all events Green: Magneta and
– xF>0 and
– M>4.5 GeV
– and pz>20 GeV
Blue: Green and
– |ytrack|>2.25 in at z=0 (dump face)
Red: Blue and
– |ytrack|<10.0 in at z=-60 (target)
Reconstructed
Generated
720 June 2008 Paul E. Reimer
Station 1 Chamber Rates
Occasionally a muon showers in the absorber If this happens in the center of the absorber,
no effect is seen as shower is also absorbed If this happens in the last few inches of the
absorber, shower can create extremely large rates in Station 1 (of low momentum particles)
Solution is to have an absorber-free region at the end of the field volume and use field as a sweeper
In Solid Iron magnet, there is no absorber-free sweeper region! (Can we find a wide gap sweeper magnet?)
Requires GEANT MC to see magnitude of effect
Absorber and B Field
Sta. 1
Absorber and B Field
Absorber and B Field
B Field only
820 June 2008 Paul E. Reimer
Mass Resolution
Reconstruction of Muon tracks yields virtual photon properties:
– M2, xF, pT
Mass resolution dictates J/ cut Critical for x2 (and x1) resolution
Drell-Yan
J/450 MeV(and don’t forget about the 0)
Drell-Yan
J/470 MeV(and don’t forget about the 0)
“Standard” E906 Analysis Mass cut of 4.5 GeV
920 June 2008 Paul E. Reimer
Mass Calibration
Track reconstruction apparently skews virtual photon mass
Events with tracks which significantly miss target have poor mass reconstruction
yrtp and yrtn are the reconstructed y offsets of the two tracks at a plane perpendicular to the beam in the center of the target. P and n denote positive and negative.
Mass is the difference between generate and reconstructed mass in the Monte Carlo
Drell-Yan (M>4.5 GeV) MC in blackJ/ MC in red
Use known mass (J/) to calibrate this correction
– Effect is slightly different, but similar to higher mass Drell-Yan
1020 June 2008 Paul E. Reimer
Calibrated mass resolution
Introduces mass offset in Drell-Yan mass range (4.5 < M<8.5 GeV) but better than uncorrected
Drell-Yan
J/298 MeV
Significant improvement near J/ General improvement at all masses
1120 June 2008 Paul E. Reimer
xF Resolution
No Known xF point to use for calibration.
1220 June 2008 Paul E. Reimer
x1 Resolution
x1 resolution worseworse with correction
Resolutio
n
for all x 1
Resolutio
n
x 1≥ 0.75
1320 June 2008 Paul E. Reimer
x2 Resolution
x2 resolution improved by correction.
Resolution significantly worse for high x2—is this a problem?
Resolutio
n
for all x 2
Resolutio
n
x 2≥ 0.35
Recall D-Y falls exponentially with x2.
Events may be reconstructed into neighboring bins.
1420 June 2008 Paul E. Reimer
x2 resolution—solid iron and miss reconstruction
Can we live with this Can we live with this misidentification? Or find an misidentification? Or find an additional correctionadditional correction
Red events have reconstructed to the correct x2 bin
For a significant fraction of the events, x2
true is
one (blue) or
two (green)
bins lower than x2
recon.
Ess
entia
lly n
o da
ta in
thi
s bi
n
1520 June 2008 Paul E. Reimer
x2 resolution— Open ApertureOpen Aperture and miss reconstruction Red events have
reconstructed to the correct x2 bin
Open aperture design also suffered from misreconstruction, but not as much as solid iron design E
ssen
tially
no
data
in
the
se b
ins
Does anyone want to look at this in E866 data?
1620 June 2008 Paul E. Reimer
Statistical Precision
Increased statistical precision w/Solid Fe Magnet
Larger transverse “aperture” in Solid Fe Magnet (34” vs. 25”)
Larger Station 3 wire chamber
– Needed to take advantage of larger aperture
– Note: open aperture would also benefit from larger station 3
– Part of Japanese contribution
Significant gain in large-x2 region
Open Ap. Design may also gain in Stat. as well from larger Station 2 & 3 combination
1720 June 2008 Paul E. Reimer
Drell-Yan Ratio Statistical Uncertainty
Better Statistical Uncertainty at high x2
Crude trigger matrix applied
– not used in previous plots
– Accounts for fall-off at low x2 in solid iron magnet
1820 June 2008 Paul E. Reimer
126 inch Magnet
Resolution in Mass and x2 not better
Lower acceptance at high-x2
– See relative normalization
Mass All x2 x2 for x2 > 0.35
1920 June 2008 Paul E. Reimer
Magnet Polarity:which events do we want?
We really want the high-x2 events
All the other events come for free
2020 June 2008 Paul E. Reimer
Magnet polarity 8 GeV
2120 June 2008 Paul E. Reimer
Magnet Polarity 6 GeV
2220 June 2008 Paul E. Reimer
Magent Polarity 4 GeV
2320 June 2008 Paul E. Reimer
Magnet Polarity 3 GeV
Conclusion Running in opposite polarity may allow smaller chambers
– Important for Station 3 which is LARGE
– Acceptance must be verified with Monte Carlo
Preliminary Monte Carlo shows resolution is the same (expected)
2420 June 2008 Paul E. Reimer
Things left to do
Independent verification of results
1. Background rate simulations See GEANT MC talk—this seems to be in hand
2. Opposite Polarity MC with reduced Sta. 3 size I’ve run the MC and could have results next week
3. Resolution improvements with target retrace?
4. Angular resolution for cos 2 distributions
5. Partonic Energy Loss—is x1 resolution good enough?
6. What is the saturation curve of the SM12 iron—this clearly effects the field Some data from Chuck et al. that must be analyzed
2520 June 2008 Paul E. Reimer
Resolution is poorer with Solid iron magnet, but acceptable?
– x2 bin resolution
Dump/Target separation is achievable
Conclusion: Solid Fe magnet will work (always listen to Chuck)
Ess
en
tially
no
dat
a in
thi
s b
in
Larger aperture provides better statistical precision at high x2
Opposite polarity configuration may allow for smaller Station 3 and 4 chambers