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Mar 20/25 PionLT/KaonLT Analysis Meeting Notes
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----------------------------------------------
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(Notes by GH)
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Today: PionLT will be discussed first
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Present
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Regina - Garth Huber, Nathan Heinrich, Ali Usman, Alicia Postuma,
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Muhammad Junaid, Vijay Kumar, Nacer Hamdi
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JLab - Dave Gaskell
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Virginia - Richard Trotta
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CUA - Tanja Horn
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FIU - Pete Markowitz
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Nathan
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------
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PionLT Coin Lumi scan update
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- LH2 boiling correction for singles is applied throughout, 2.8%/100uA
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- randoms subtraced and pion PID are applied
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- two studies presented:
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Pass 10: boiling and tracking (both arms), EDTM TLT, BCM correction all applied
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- normalized yield vs Beam current shows a decrease of ~6% @ 80uA with lots of
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scatter
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- best set (least decrease) is SIDIS setting 2
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- same data vs PS5 rate gives a bimodal distribution, one lobe with steeper
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slope than the other
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- vs SHMS rate also bimodal dist
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- vs HMS rate, data merge closer to one dist, but much scatter
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Pass 12: same as 10 plus DMack hodo corr (both arms) - beam off periods are
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removed when calculating hodo correction
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- Dave: concerned that applying DMack hodo correction is double counting
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- Nathan: maybe it's actually an inefficieincy in the hodo at high rate??
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- normalized yield vs Beam current shows scatter but less than Pass 10
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- vs SHMS rate gives fairly flat distribution but still lots of scatter
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- Nathan interprets to mean that the SHMS rate dependence is correctly
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modeled when applying DMack correction
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- vs HMS rate, strong correlation of 3.4%/100kHz but much less scatter, with
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the data extending up to ~180kHz, i.e. ~5% correction, which would be
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presumably different at high and low epsilon
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Dave: the data seem convincing that there is an unresolved rate dependence,
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still concerned applying DMack correction and EDTM is double counting
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- Nathan will make a version with CPULT and DMack hodo correction instead
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- Dave expects there will be a rate dependence, but is interested to see if
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the scatter in the data is less
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Garth: baffled that the strong correlation is with HMS rate, which is not
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large, and not with SHMS rate which is 3x larger
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- would like a better explanation to justify such a large correction to the data
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Dave: in the 6-GeV era we had to determine a coincidence blocking correction from
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CoinTime data, maybe something similar is going on here?
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- we discuss whether coincidence blocking is still possible with the 12-GeV
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DAQ
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- Nathan will give Dave some run numbers where the HMS rate correction is
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fairly large to look for evidence of coincidence blocking in the CoinTime
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histo
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Junaid
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Setting up for Q2=3.8 physics analysis
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- ran SIMC for these settings
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- calculating MM offsets to be applied to data to line up with SIMC
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- then will finalize MM cut and Diamond cuts
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Vijay
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Diamond cut for Q2=0.425 PionLT
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- checked SIMC diamond cut compared to data and found a shift
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- it turned out the kinematic offsets weren't applied to MC
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- when offsets appied, shift in SIMC diamond is much less
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- will adjust diamond in one corner which is not filled by SIMC
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- will shift data MM peaks to overlap SIMC
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Nacer
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KaonLT Q2=0.50 physics analysis
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- all cuts applied to data but not random subtracted for purposes of
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determining t-binning and diamond cuts
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- Lambda: chose 7 bins, ~15k events/bin at both high and low epsilon
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- made plot of SIMC t-ti to check t-migration
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- ti has no radiation or multiple scattering, while t is simulated detected
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data
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- fits t-ti with a Gaussian, sigma ~0.002 for both high and low epsilon
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however there is a tail (due to radiation) which is about 0.02 long
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- the narrowest t-bin is 0.007 wide
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- Dave: theere will be a small amount of t-bin migration but this should be
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acceptable
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- Vijay notes that one bin limit looks wrong, there is a gap between bins,
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Nacer will investigate
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- t-phi plots at high and low epsilon, with all SHMS settings superposed
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- Garth: the highest t-bin extends to 0.166 and the t-phi plot looks very
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sparsely populated there at 6 and 12 o-clock
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- Nacer will make binned plots
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- also no diamond cut was applied so actual t-coverage will be smaller
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- most likely the t-range of the data needs to be narrowed, such as by
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dropping the highest t-bin
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- Garth also suggests that Vijay and Junaid make similar plots when
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finalizing their t-binning
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Richard
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KaonLT high Q2 analysis
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- summarizes meeting on Wed with Tanja, Pete, Garth
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- if possible, we should aim to have an xB=0.40 scan in our first paper
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- summary of xB=0.40 status:
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Q2=3.0, W=2.32 hasn't been looked at in ~1 year. There have been lots of
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improvements since then, will look at again
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- a question to be investigated is whether this point can use the same
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functional form as W=2.72 points, given that W=2.32
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Q2=4.4, 5.5: nearly done, will try to finish them up soon
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- likely only 1 t-bin for Q2=5.5 due to statistics
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- status of other points:
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Q2=2.115, W=2.95 was looked at last summer, seemed OK. Will look at briefly
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again but not expecting problems
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Q2=3.0, W=3.1 nearly finalized. T,TT forms different than Q2=4.4,5.5
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- updates on Q2=4.4 L/T-sep
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- removed Q2-dependence to give very simple parameterizations
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- this seems to work very nicely for the lowest t-bin, -t=0.470 with ratios
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fairly flat and close to 1
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- ratios increase for higher t-bins, but still seem fairly flat
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- comparison of data and MC for kinematic and acceptance plots
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- integrated over t-bin, not renormalized to data
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- agreement looks pretty good, which is encouraging
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Alicia
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------
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Proton absorption Geant4 model
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- earlier, some anomalous absorption was reported for electrons
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- this was traced to a problem with S2Y NPE and Energy step action, data were
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being reset for each step through detector instead of being accumulated
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- with this fixed, things look more reasonable now
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- detection efficiency vs momentum for all particle types
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- very low efficiency for P<0.4 GeV/c
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- no protons for P<0.1 GeV/c reach the hodoscope at all
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- plot of absorption vs momentum
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- a significant momentum dependence is observed which is unexpected
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- electrons have a flat momentum dependence for P>3 GeV/c
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- pions ~1 GeV/C have very large absorption
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- can check the MM but expecting this to be in the resonance region, where
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the proton absorption cross section is very large due to Delta resonance
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creation
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- will plan to run larger event samples for next week to remove some possible
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statistical scatter (10k vs 2k events)
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- Ali: good to look at where the particles stop in the detectors for different
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momenta
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- yes, this is in progres
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- Garth: the simulation covers the full focal plane, using actual (x,x',y,y')
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focal plane values from data
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- maybe some of what is seen is due to edge effect issues. One way to study
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this might be to use particle gun covering only the edge of the focal plane
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- if the gun sees a smaller momentum dependence, this would indicate the
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observed dependence here is due to edge effects
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- spreadsheet of DEMP data for Simonetta Liutti
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- version 1 of spreadsheet is completed
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Next Meeting
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-------------
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- Thur Mar 27 @ 16:30 Eastern/14:30 Regina
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- KaonLT will go first
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- NOTE: meetings start 16:30 Eastern/14:30 Regina from March 13-April 10
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- after that, we can return to 15:30 Eastern for the convenience of our USA
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colleagues
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