1
|
May 29/25 PionLT/KaonLT Analysis Meeting Notes
|
2
|
----------------------------------------------
|
3
|
(Notes by GH)
|
4
|
|
5
|
Today: PionLT will be discussed first
|
6
|
|
7
|
Please remember to post your slides at:
|
8
|
https://redmine.jlab.org/projects/kltexp/wiki/Kaon_LT_Meetings
|
9
|
|
10
|
Present
|
11
|
-------
|
12
|
Regina - Garth Huber, Nathan Heinrich, Ivan Zhenchuk, Alicia Postuma,
|
13
|
Muhammad Junaid, Nacer Hamdi, Vijay Kumar
|
14
|
FIU - Pete Markowitz
|
15
|
Virginia - Richard Trotta
|
16
|
JLab - Dave Gaskell
|
17
|
JMU - Ioana Niculescu
|
18
|
Ohio - Julie Roche
|
19
|
CUA - Tanja Horn
|
20
|
|
21
|
Nathan
|
22
|
------
|
23
|
PionLT deadtime effects
|
24
|
- follow-up to weird dip in HMS-delta (H.gtr.dp vs H.gtr.beta) found by Dave
|
25
|
Gaskell, run 14613
|
26
|
- also seen by Junaid in HMS-delta comparison to SIMC
|
27
|
- Dave says the dip only appears if he places a narrow cut on the prompt CT
|
28
|
peak
|
29
|
- Nathan reran Hodoscope calibrations, doesn't see any dip, no change before
|
30
|
and after calib
|
31
|
- will look again at Reference Times
|
32
|
|
33
|
- return to this topic near end of meeting
|
34
|
- Dave shows a plot of CoinTime vs position at 2X plane in HMS, run 14613
|
35
|
- 2 clear shifts in time are seen, associated with specific paddles
|
36
|
- suggests that Nathan look at the param files to see what might be wrong
|
37
|
|
38
|
- Carbon Lumi scans after Reference Time fixes
|
39
|
- Tracked yield is fairly flat, looks generally acceptable
|
40
|
- however, there are a few outliers. These are being looked at, either to
|
41
|
fix them, or find a reason to exclude them
|
42
|
- before the Ref Time fix, Carbon was flat, so it should be possible to get
|
43
|
it flat again
|
44
|
|
45
|
- LH2 boiling scans after Reference Time fixes
|
46
|
- scaler analysis flat (with old boiling corr applied)
|
47
|
- NoTrack and Track analyses not flat
|
48
|
- still investigating, no details yet
|
49
|
|
50
|
Junaid
|
51
|
------
|
52
|
PionLT LTsep initial setup
|
53
|
- last week showed calculated Data/MC ratios, where SIMC uses the default
|
54
|
Bosted physics_pion.f model
|
55
|
- still going through the Fortran codes
|
56
|
- next step will be un-iterated sig_unsep, using Bosted SIMC model
|
57
|
- will show draft CAP slides next week
|
58
|
|
59
|
Ali
|
60
|
---
|
61
|
piDelta BSA
|
62
|
- GH gives a few remarks from Ali, his thesis defense is tomorrow
|
63
|
- asymmetry extraction from rebinned data is done
|
64
|
- LT'/sig0 ratios with new binning also done, results look promising
|
65
|
- will show results and draft CAP slides next week
|
66
|
|
67
|
Nacer
|
68
|
-----
|
69
|
KaonLT LTsep initial setup
|
70
|
- shows calculated Data/MC ratios, where SIMC uses the default Koltenuk
|
71
|
physics_kaon.f model
|
72
|
- problematic missing bins resolved, the problem was caused by low statistics
|
73
|
phi bins for Left and Right SHMS settings, resolution was to set the errors
|
74
|
for these bins to be very large when calculating the average ratios
|
75
|
- ratios have nearly symmetric phi dependence, which is good
|
76
|
- some notable phi-oscillations, we note that the Koltenuk model has no
|
77
|
LT,TT terms, hence no phi-dependence, which we will resolve when doing
|
78
|
iterations
|
79
|
|
80
|
- un-iterated sig_unsep, using Koltenuk SIMC model
|
81
|
- calc_xsect.f gives a theta* disagreement between data and calc, will have a
|
82
|
short discussion with Richard about this at end of meeting
|
83
|
- LTsep framework is mostly set up now
|
84
|
- will show draft CAP slides next week
|
85
|
|
86
|
Vijay
|
87
|
-----
|
88
|
pion and proton "absorption" study for Q2=0.425 PionLT data
|
89
|
- pi+, P_SHMS=2.326 GeV/c
|
90
|
- no Cherenkov cuts uses in analysis, only CoinTime PID needed to get clean
|
91
|
data
|
92
|
- Geant4 gives 2.16% bad events, so correction factor=0.9784
|
93
|
|
94
|
- Heep protons:
|
95
|
P_SHMS=1.729 bad=3.43%
|
96
|
P_SHMS=2.300 bad=3.50%
|
97
|
P_SHMS=2.792 bad=2.84%
|
98
|
- 10k events run for all 3 simulations, finds the higher middle bad value a
|
99
|
bit odd
|
100
|
- GH: suggests to run at least 50k events for all settings (including pi+) to
|
101
|
see if the Heep number changes
|
102
|
- Alicia: if the middle absorption value says higher with more stats, it
|
103
|
means this is due to the Geant4 cross section momentum dependence
|
104
|
- absorption is expected to be higher for P<1 GeV/c, should be fairly flat
|
105
|
for higher momenta
|
106
|
|
107
|
- will implement absorption correction into physics yield calculation
|
108
|
|
109
|
- Vijay's contract ends in ~10 days, his future plans still uncertain
|
110
|
|
111
|
Richard
|
112
|
-------
|
113
|
KaonLT high Q2 LTsep
|
114
|
- fixed very high theta* values problem noted earlier
|
115
|
- issue was that the recoil mass in eps_n_theta.f was still set to proton
|
116
|
instead of lambda mass
|
117
|
- the theta* values are now lower, initial results show an improvement in
|
118
|
higher t-bin ratios
|
119
|
- unfortunately, the change did not get properly pushed to his main analysis,
|
120
|
rerunning the data again
|
121
|
|
122
|
Ivan
|
123
|
----
|
124
|
Low Q2 KaonLT BSA
|
125
|
- K+ PID investigations
|
126
|
- switched from HGC PID (shown last week) to RF PID that Nacer uses
|
127
|
- RF time is not properly aligned at zero for Kaons, unlike Nacer's analysis
|
128
|
- Nacer had adjusted RF time but the updated Hodoscope calibs did not
|
129
|
properly get pushed to GitHub
|
130
|
- Alicia will coordinate with Nacer on a new replay using Nacer's calibs
|
131
|
and Alicia's helicity scripts
|
132
|
|
133
|
- K+ MM spectra with dummy target and pion leakthrough subtractions
|
134
|
- the pion leakthrough subtraction seems to work well, leaves clean Lambda
|
135
|
and Sigma peaks on little background
|
136
|
- a future study will have to be to vary the pion subtraction and see how
|
137
|
the BSA results change
|
138
|
|
139
|
- first look at K+ BSA results
|
140
|
- integrates around the clean Lambda peak, only ~1/3 of Center SHMS setting,
|
141
|
no Right and Left SHMS yet
|
142
|
- errors look large, but the beam polarization is only 38%, which magnifies
|
143
|
uncertainties by ~2.6x
|
144
|
- mostly sees random scatter around zero
|
145
|
- we note that YCK model (for pi+n) predicts small BSA at low Q2, the
|
146
|
asymmetry grows to a plateau value above a Q2-threshold
|
147
|
|
148
|
- also looks at pi+ BSA for same data
|
149
|
- the pion leakthrough sample is used for this check, calculated the same way
|
150
|
as for K+
|
151
|
- asymmetry is about +/-0.02, so very small
|
152
|
- a clear sinusoidal dependence is seen, not the random scatter as for K+
|
153
|
|
154
|
- also looks at BSA of pi+ background underneath the Lambda (corresponding to
|
155
|
piDelta region)
|
156
|
- the asymmetry is very small, less than the +/-0.02 seen for the exclusive
|
157
|
pi+n
|
158
|
- this is an important systematic check on the analysis that we will need for
|
159
|
any publication
|
160
|
|
161
|
Alicia
|
162
|
------
|
163
|
Draft CAP slides on u-channel motivation and analysis
|
164
|
- Bill Li had a recent talk using the Verton (baryon junction) motivation, but
|
165
|
that is more closely linked to u-channel SIDIS than u-channel exclusive
|
166
|
- also shows Zach Sweger talk from CFNS Baryon Junction workshop, where he
|
167
|
frames the motivation in terms of TDA and distribution of Baryon # vs
|
168
|
Momentum
|
169
|
- also shows CLAS-6 BSA results for pi+n channel, comparing forward (t-channel)
|
170
|
and backward (u-channel) and the unexpected sign flip in the BSA between them
|
171
|
|
172
|
- Tanja comments:
|
173
|
- one of the issues is that it's hard to find clean Verton observables, to
|
174
|
avoid a lot of questions that may be difficult to answer, recommends not to
|
175
|
make it the main emphasis of the talk
|
176
|
- suggests to emphasize the data and what kind of impact they are likely to
|
177
|
make
|
178
|
- it's okay to mention Verton, but don't over promise
|
179
|
- suggests to focus more on TDAs and use Verton as one way to describe why
|
180
|
TDAs may be interesting
|
181
|
|
182
|
- Garth:
|
183
|
- given the audience, comparing more clearly the forward and backward angle
|
184
|
regions would really be helpful, not only in terms of the differences of
|
185
|
the detected processes, but also in terms of what you learn from the two
|
186
|
regions
|
187
|
- should coordinate closely with Junaid and Ali on the description of
|
188
|
experimental details (to avoid needless overlap) and on the complementarity
|
189
|
of the forward (Junaid and Ali) and backward (Alicia) data sets
|
190
|
|
191
|
Short discussion between Nacer and Richard on theta* discrepancy
|
192
|
- Richard uses average_kinematics.f to make his average kinematic tables
|
193
|
- need an error-weighted average over not only the different SHMS settings,
|
194
|
but also over all epsilons
|
195
|
- average_kinematics.f also uses eps_n_theta.f to find theta* and epsilon
|
196
|
values for each (Q2bar, Wbar), the theta* values don't come from hcana
|
197
|
- the cross check between theta* values in calc_xsect.f is mainly to be sure
|
198
|
everything is done consistently, both values come from the same code and
|
199
|
should agree
|
200
|
- Nacer was taking theta* values from data directly, not calculating them in
|
201
|
this way
|
202
|
- calc_xsect.f overwrites these theta* values, the expt values are not used
|
203
|
- this method should be fine, as long as the (Q2bar, Wbar) values are
|
204
|
averaged correctly
|
205
|
- Nacer will modify his averaging routine (python) and do some checks
|
206
|
|
207
|
- Garth briefly mentions new CLAS-12 K+ results from Q2=0.3 to 4.5 GeV2
|
208
|
arXiv: 2505.12030
|
209
|
- they see strong dependence in Sigma/Lambda ratio, similar to what we can
|
210
|
tell from Richard and Nacer data
|
211
|
- Sigma nearly the same size as Lambda peak at low Q2
|
212
|
- Sigma/Lambda ratio drops rapidly with increasing Q2
|
213
|
|
214
|
Next Meeting
|
215
|
-------------
|
216
|
- Thur June 5 @ 15:30 Eastern/13:30 Regina
|
217
|
- KaonLT will go first
|
218
|
- lots of slides to show, so the meeting might go a bit longer than usual
|
219
|
|
220
|
|
221
|
|
222
|
|
223
|
|
224
|
|
225
|
|