Analyzing #397

Variation of the parameters

Added by Vratislav Chudoba almost 5 years ago. Updated over 4 years ago.

Status:ОткрытаStart date:11/15/2019
Priority:НормальныйDue date:
Assignee:Ivan Muzalevsky% Done:

82%

Category:-
Target version:-

Description

Initial form of the 9Li missing mass will be determined in this issue together with input parameters. All variations of the stated parameters will be reported as an individual subtask of this issue.

The initial parameters:

number parameter value unit
1 beam energy beamDet thickness: 630 micron of Si   
2* thin SSD calibration parameters pars for 2 thin detector (ssd_20u_2.cal) from issue 284

pars for 1 3 and 4 detectors from issue 391 
(SSD_20u_1_cal.txt,
SSD_20u_3_cal.txt 
SSD_20u_4_cal.txt )
 
3 thick SSD calibration parameters issue 391  
4 central DSD calibration parameters issue 391  
5 thin detector front dead layer not used mcm
6 thin detector rear dead layer not used mcm
7 thick SSD front dead layer issue 391 mcm
8 thin detector position issue 293 mm
9 thick detector position issue 293  mm
10 central DSD position (0,0,323) mm
11 target density (same pressure as for 7H) 0.0020646 g.cm-3
12 target density, low  0.001005 g.cm-3
13** full target thickness 6 mm
14 target mylar window thickness 3.5 mcm
15 target stainless steel window thickness 6 mcm
16*** CsI calibration parameters not used  
17 map of thickness for thin SSD issue 392  
18 target selection circle of 9 mm radius
with center in ( 0.4673,0.0262) mm at the target plane
 
19 MWPC positions MWPC1 (-0.9,-3,-815)
MWPC2 (0.3,-1.55,-270)
mm

* Energy deposit in the first layer of side telescopes is calculated according to the map of thickness. Calibration parameters are used exclusively for particle identification.
** Target is taken as a cylinder of homogeneous thickness for the purposes of reconstruction.
*** When needed, identification of 9Li is performed without calibration parameters using the CsI response in channel values.

Two expositions are at disposal:

  • for the thin gaseous target (be10_ct_39* and be10_ct_40*)
  • for the thick gaseous target (be10_ct_*)

Provide the resulting spectrum together with the mean value of the ground state in two separate comments:

  • one spectrum from all telescopes for the thin target;
  • one spectrum from all telescopes for the thick target and four spectra for individual telescopes.

Subtasks

Analyzing #399: Target thicknessОткрытаIvan Muzalevsky

Analyzing #400: Z-position of the side telescopesОткрытаIvan Muzalevsky

Analyzing #414: Offsets of the 3He telescopeОткрытаIvan Muzalevsky

Developing #416: BeamDet thicknessОткрытаIvan Muzalevsky

Developing #418: thin detector thickness variationОткрытаIvan Muzalevsky

Analyzing #420: Effect of rime growing on target surfaceОткрытаIvan Muzalevsky

History

#1 Updated by Ivan Muzalevsky almost 5 years ago

  • Description updated (diff)

#2 Updated by Vratislav Chudoba almost 5 years ago

  • Description updated (diff)

#3 Updated by Ivan Muzalevsky almost 5 years ago

  • Description updated (diff)

#4 Updated by Ivan Muzalevsky almost 5 years ago

  • Description updated (diff)

The content was deleted on 17.01.2020. The deleted results were incorrect.

#5 Updated by Ivan Muzalevsky almost 5 years ago

  • Description updated (diff)

#6 Updated by Ivan Muzalevsky almost 5 years ago

  • Description updated (diff)

#7 Updated by Vratislav Chudoba almost 5 years ago

  • Description updated (diff)
  • Assignee set to Ivan Muzalevsky

#8 Updated by Ivan Muzalevsky almost 5 years ago

  • Description updated (diff)
  • Assignee deleted (Ivan Muzalevsky)

#9 Updated by Vratislav Chudoba almost 5 years ago

  • Description updated (diff)
  • Assignee set to Ivan Muzalevsky

#10 Updated by Ivan Muzalevsky almost 5 years ago

  • Description updated (diff)

#11 Updated by Ivan Muzalevsky over 4 years ago

Summed spectrum from all 4 telescopes for thin target

Green lines - coincidence with 9Li


The position of the g.s. is 0.048 MeV which was estimated as a mean value of the main peak of the black histogram

Separated spectra from 4 telescopes for thick target


Red lines - ground state selection

Ground state positions (means of red histograms): 
-0.118 MeV (776 events)
0.359 MeV (634 events)
0.085 MeV (712 events)
0.149 MeV (711 events)

Summed spectrum from all 4 telescopes for thick target

Green lines - coincidence with 9Li


From the summed spectrum the g.s. position was calculated as a statistical average from 4 values:
position = (-0.118071*776 + 0.358727*634 + 0.0849232*712 + 0.149297*711)/28330.107 MeV

#12 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#13 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#14 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#15 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#16 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#17 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#18 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#19 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

#20 Updated by Ivan Muzalevsky over 4 years ago

  • Description updated (diff)

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