Privacy and Security Notice
GWU Status Report: 6-27-07
GWU Status Report: 6-27-07
Default geometry: CuPb primary collimator: 20 radiation lengths (~21.66 cm), theta_max 10.25, 25 cm upstream from VT line 20. NB: All backgrounds presented here have the appropriate weighting (cross section, asymmetry, photoelectric efficiency).
Item 1
Thickness of primary collimator (again): We re-evaluated the background versus primary collimator thickness for the CuPb collimator, results for 5, 10, 15, and 20 radiation lengths shown in the plots below or you can see the table here. When a lintel is used, it means a 15 radiation length Pb lintel.
 |
 |
| Conclusion: NB: suppressed zero! FOM is essentially insensitive. |
Conclusion: With a lintel (blue points), 10, 15, and 20 radiation lengths are the same. However, for 5 and 10 radiation lengths we depend on the lintel much more. |
 |
 |
| Conclusion: With a lintel, the photon backgrounds are all the same (blue points), but 5 and 10 radiation lengths depend on the lintel more. For electrons (red points), 15 radiation lengths seems best |
Conclusion: Same story. Moller electrons will decrease when a shielding wall is added. |
Conclusion: Overall, for 5 and 10 radiation legnths we depend on the lintel a lot. However, it seems like we can get by with using 15 radiation lengths.
Item 2
Line of sight? This is an image looking upstream from the Cernkov along the angle of the accepted electrons - is this a problem?:
Can see through 2nd octant of coll. 3 through 3rd octant of coll. 2 into space upstream of the primary collimator. Can eliminate by extending collimator 1 to 80 cm (previously 43.18 cm):
Item 3
Up to this point, we have only been generating events in the theta range 5-14 degrees, which covers the extreme rays through the primary collimator. We should have been including everything that gets through the first collimator, which we determined to be covered by the range 2.5-14.5 degrees in theta. Table's 3 and 4 show how this affects the backgrounds.
Plots of elastic and inelastic backgrounds for 5-14 degrees (black points) and 2.5-14.5 degrees (green points) without a lintel (left) and with a lintel (right): [can click on image for full size]
Conclusion: When opening the range from 5-14 to 2.5-14.5 as long as we are using a lintel there is no significant change. We will start using this range.
Table 3: Theta range 5-14 degrees
| |
w/o lintel |
with lintel |
| Rate (MHz) |
801.995 |
802.237 |
| < Q^2 > |
0.025753 |
0.025768 |
| Error (%) |
4.3087 |
4.3074 |
| Elastic Photons (%) |
0.20796 +/- 0.00519 |
0.14824 +/- 0.00477 |
| Elastic Photons from coll. region |
0.06864 +/- 0.00269 |
0.00583 +/- 0.00069 |
| Inelastic Photons (%) |
0.02771 +/- 0.00141 |
0.01087 +/- 0.00088 |
| Inelastic Electrons (%) |
0.10833 +/- 0.00536 |
0.11787 +/- 0.00561 |
| Moller Photons (%) |
0.87131 +/- 0.03194 |
0.18208 +/- 0.01431 |
| Moller Electrons (%) |
1.42232 +/- 0.08872 |
1.08812 +/- 0.08066 |
|
Table 4: Theta range 2.5-14.5 degrees
| |
w/o lintel |
with lintel |
| Rate (MHz) |
802.204 |
799.045 |
| < Q^2 > |
0.025757 |
0.025740 |
| Error (%) |
4.3092 |
4.3159 |
| Elastic Photons (%) |
0.23705 +/- 0.00850 |
0.14343 +/- 0.00687 |
| Elastic Photons from coll. region |
0.07852 +/- 0.00423 |
0.01127 +/- 0.00161 |
| Inelastic Photons (%) |
0.03112 +/- 0.00118 |
0.01048 +/- 0.00062 |
| Inelastic Electrons (%) |
0.12426 +/- 0.00470 |
0.11595 +/- 0.00448 |
| Moller Photons (%) |
0.94076 +/- 0.03043 |
0.18676 +/- 0.01277 |
| Moller Electrons (%) |
1.71436 +/- 0.07785 |
1.45482 +/- 0.07107 |
|
Item 4
I think I have been able to implement Juliette's codes for reading in the new field map.