Update on Simulation Studies of the CEDAR Optics

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Update on Simulation Studies of the CEDAR Optics. Helen Heath 9 th December 2009. Reminder (see N.Brook’s talk from August). Use Lau’s CEDAR simulation provide Cerenkov photons to current quartz window -> position(x,y,z) and direction(n x ,n y ,n z ) and wavelength - PowerPoint PPT Presentation

Transcript of Update on Simulation Studies of the CEDAR Optics

Update on Simulation Studies of the CEDAR Optics

Helen Heath9th December 2009

Reminder (see N.Brook’s talk from August)

• Use Lau’s CEDAR simulation• provide Cerenkov photons to current quartz

window • -> position(x,y,z) and direction(nx,ny,nz) and

wavelength• Optical path simulation

• Use ROOT and its geometry manager

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Z=646mm

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Z=996mm

Parabaloidal “cones”10mm depth 25mm depth

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Summary of results in August

• 10mm cone • 82-87% photon reach PMT cathode• 68-90% of photons reflected off cone reflect

off PMT window• 25mm cone

• 87-91% photon reach PMT cathode• 29-67% of photons reflected off cone reflect

off PMT window

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Cone v Parabaloid

80.0%

82.0%

84.0%

86.0%

88.0%

90.0%

92.0%

94.0%

600 700 800 900 1000

25mm Conical collectors

25mm Parabaloid Collectors

10mm Short ConicalCollectors10mm Parabaloid Collectors

Efficiency for photons to reach the PMT cathode v z position

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Efficiency for different cone depths

80.0%

82.0%

84.0%

86.0%

88.0%

90.0%

92.0%

500 700 900 1100

10mm cone15mm cone20mm cone25mm cone30mm cone12mm cone11mm cone9mm cone

Shown for conical collection cones

Note: there is little increase in efficiency one the cones are above 15mm in length

The parabaloid is similar but the efficiency falls more quickly

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Source of Losses

• Previous simulations assumed losses at surfaces due to • 5nm roughness for mirror• 10nm roughness for cones

• Look at cone roughness

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10nm Roughness

-5.0%

0.0%

5.0%

10.0%

15.0%

20.0%

25.0%

30.0%

35.0%

40.0%

0 5 10 15 20 25 30

Reflection at the mirrorRoughness of coneReflection from PMTescapedtotal loss

Photon loss v cone depth z=646

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Escapees10

5nm Roughness

0.0%

5.0%

10.0%

15.0%

20.0%

25.0%

30.0%

35.0%

40.0%

0 5 10 15 20 25 30

Reflection at the mirrorRoughness of coneReflection from PMTescapedtotal loss

Photon loss v cone depth z=64611

15nm Roughness

0.00%

5.00%

10.00%

15.00%

20.00%

25.00%

30.00%

35.00%

40.00%

0 5 10 15 20 25 30

Reflection at the mirrorRoughness of coneReflection from PMTescapedtotal loss

Photon loss v cone depth z=646

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Summary of Efficiency Studies

• Dominant contributions to the photon loss are• Photons escaping the system for depth<7mm• Reflection from the PMT surface

7mm<depth<~10mm• Beyond 10mm the loss at the cone surface

may become the dominant contribution but it increases slowly above ~15mm

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Photon distributions at PMT

• Nick’s studies observed a double peak in the photon angle at the PMT.

• Confirmed to be photons reflected from the cone and those that enter directly (see next slide)

• Also noted that the distribution across the PMT face is different for these two cases

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10mm cone, photon angle to PMT face. Red photons not reflected from cone, blue photons reflected from cone

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25mm cone, photon angle to PMT face. Red photons not reflected from cone, blue photons reflected from cone

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1725mm cone, photon position at PMT face. Red, photons not reflected from cone, black photons reflected from cone

Efficiencies for photons from Pions

• 25000 photons• 25mm cone

• Efficiency 0.10% for all z

Z 646 696 746 796 846 896 946 996# Arrived at PMT 25 26 25 26 23 26 25 24

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Future plans

• To look at the muon halo • Feed in any mechanical design constraints

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