Project

General

Profile

Kaon LT Meetings » mtg_24nov21.txt

Garth Huber, 11/22/2024 01:20 PM

 
1
                 Nov 21/24 PionLT/KaonLT Analysis Meeting Notes
2
                 ----------------------------------------------
3
                                (Notes by GH)
4

    
5
                     Today: PionLT will be discussed first
6

    
7
Present
8
-------
9
Regina - Garth Huber, Alicia Postuma, Nathan Heinrich, Muhammad Junaid,
10
   Ali Usman, Nacer Hamdi
11
Virginia - Richard Trotta
12
CUA - Tanja Horn
13
FIU - Pete Markowitz
14
Ohio - Julie Roche
15
JLab - Dave Gaskell
16

    
17
Nathan
18
------
19
- no report, preparing for tomorrow's committee meeting
20

    
21
Junaid
22
------
23
PionLT tracking updates
24
 - updated geometry parameter files (better drift chamber position data),
25
   improves residuals
26
   
27
- Mark's tracking algorithm changes
28
 - implemented new parameter values to turn on Mark's algorithm changes
29
   - using his default parameter values for now
30
 - Heep replays using the new algorithm
31
   - 5.986 GeV and 10.56 GeV Coin
32
   - change to W distribution is subtle, tail to left of elastic peak has a bit
33
     steeper slope (log scale), fewer slightly fewer events
34
   - 10.56 Exp/MC ratio changed from 1.006 to 1.010, more events passing cuts
35
     so ratio went up
36
     - however, the Exp yield was calculated with the old tracking efficiency
37
     - *NB* new tracking efficiencies using the new algorithm need to be used
38
     - that will probably result in the ratio getting closer to 1.0
39
     
40
- updated HMS matrix elements for 6.7, 5.9, 6.1 GeV/c
41
  - NPS group is still working on 5.6 GeV/c matrix elements
42

    
43
  - some discussion about hdelta_offset hphi_offset values to use
44
    - *NB* need to use the same values used for matrix element fits
45
    - this means that for momenta with "old" matrix elements, offset values of
46
      zero should be used, while for "NPS" matrix elements, non-zero offset
47
      values that they used need to be retained
48
    - *NB* i.e. two different sets of parameter files are needed, please be
49
      careful thiese are implemented correctly
50

    
51
  - Ali: do we need to use the same offsets in SIMC?
52
    - Dave: SIMC uses its own matrix elements, reconstruction matrix is not
53
      changed in SIMC, do not apply the matrix element offsets to SIMC
54

    
55
Nacer
56
-----
57
KaonLT Heep singles
58
- submitted jobs to reanalyze w/Mark's tracking chagnes, but iFarm slow
59

    
60
- investigated a tighter W-cut for HMS, SHMS singles
61
  - high tail cut ~1.05
62
  - moved lower cut from 0.8 to 0.9 to see what happens
63
  - 8.2 GeV: left tail data extend all the way to W=0
64
  - 10.6 GeV: W peak is wider, 0.9 cut is clearly too tight, obtain Exp/MC
65
    ratio R=0.75(!)
66
  - *NB* need to use W cut that results in less sensitivity, GH suggests a cut
67
    near the change in slope of left background for each beam energy
68

    
69
Richard
70
-------
71
- having problems with iFarm cache being read-only
72
  - Julie: can only write to cache from batch now
73
  - Nathan: for interactive login, there is a command to specifically put a
74
    file on cache
75
  - will look up the documentation and add to RedMine notes
76

    
77
Trying KaonLT iterations w/ new TT functional form
78
- reduced chi-square now <1.5
79
- having an issue with MM_K spectra
80
  - lambda peaks not lined up correctly with expected mass, different shifts
81
    for high and low epsilon
82
    - shift is less for 10.6 GeV Q2=3.0, W=2.32 setting, which was done right
83
      after Heep (where beam energy offset was determined), other 10.6 GeV settings
84
      have a larger shift
85
   - Ali, Alicia saw some ~MeV shifts in their pi+ analyses that had to be
86
     corrected
87
     *NB* should cross compare what offsets are needed for all 3 analyses, to
88
     see if they're consistent
89
   - GH: *NB* you should write a script to fit just the top part of the MM peak
90
     for each run, and line it up to SIMC peak location on run-by-run basis
91

    
92
Alicia
93
------
94
- PRL manuscript still with reviewers
95

    
96
Geant4 proton absorption correction
97
- read in focal plane variables for an actual data sample
98
- store hit position and time in each hodoscope
99
- implementing thicknesses from spreadsheet
100
  - hodoscope (x,y) will be limiting dimension for all materials except the
101
    aerogel
102
- Dave: is it obvious what physics list to use, we're interested in hadronic
103
  interactions?
104
  - will start with StandardPhysics list
105

    
106
Ali
107
---
108
- no update, working on thesis
109

    
110
Next Meeting
111
-------------
112
- Thur Dec 5 @ 16:00 Eastern/15:00 Regina
113
  - *NOTE* no meeting next week due to US Thanksgiving holiday
114
  - KaonLT will go first
115

    
116

    
117

    
118
      
(562-562/570)