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RF background, update on analysis Rikard Sandström, Geneva University MICE Analysis phone conference, October 30, 2007.

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Presentation on theme: "RF background, update on analysis Rikard Sandström, Geneva University MICE Analysis phone conference, October 30, 2007."— Presentation transcript:

1 RF background, update on analysis Rikard Sandström, Geneva University MICE Analysis phone conference, October 30, 2007

2 Outline  What is new  Reminder of radiation yield, attenuation.  “New” MTA data.  Angles.  Number of photons per electron.  At 10.5 MV/m, simulated and calculated.  At 8 MV/m.  Rate in MICE Stage 6.  Other effects.  Phasings of cavities.  RF electrons heating absorbers.  Summary. 2R. Sandström

3 What is new  Distances are now have more exact values.  Al thicker, Cu thinner.  A bug in G4MICE prevented some photons to be registered by the Virtual Planes. It has been circumvented.  Only affected photons at large angles.  As recommended by D. Huang, using PMT#16 data (NaI) instead of PMT#8 data (Sci. paddle).  This makes a difference in rate, but NaI data is more reliable, below saturation point.  When using a series of cavities, maximum rates is downstream.  Calculations from 2004 contained a sign error on the phase. 3R. Sandström

4 Radiation yield = fraction of kinetic energy lost through radiative processes. Heavy elements (X 0 ) give higher radiation yield. Range of 1 MeV e- in Al = 2 mm. MICE: 0.18 mm Al window. Hence, combination of photon production in Al and LiH2 (+ Be, Cu). MTA: Electron ranges out in copper. R. Sandström4

5 Attenuation for PMT#16 5R. Sandström

6 MTA data Raw data scaled to events per RF period (5ns). PMT#8 data taken over full 125  s. PMT#16 data taken over 88.6  s flattop only. PMT#16 is smaller, but closer, than PMT#8. Virtually all photons hitting PMT#16 deposit all their energy in the detector, while only a fraction interact with the paddle, and not all energy is confined in active volume. PMT#16 is saturated at ~10MV/m. R. Sandström6 Areas mark where I have confidence in results

7 Simulation, angles In order to cross check, MTA was simulated using 3.6 million initial electrons. Solid black line is angular spectrum (after attenuation in metal) if isotropic angular distribution. R. Sandström7 e-e-

8 Results, number of photons per electron  At 10.5 MV/m, simulation gave  The calculation gave  The results show very good agreement!  For PMT8 even better agreement, within 0.4%. R. Sandström8

9 At 8 MV/m  This value is energy dependant  rad. yield, photon energy spectrum, attenuation, fraction above threshold  Simulation with E=1.226 MeV corresponding to 8MV/m:  Extrapolation between points of MTA data gave n  =4.03·10 -5 at 8 MV/m.  This implies n e = 705 per RF (half-) period.  Equivalent to 142 GHz per cavity and direction. 9R. Sandström

10 MICE Stage 6 @ 8 MV/m, 200 MeV/c   These values implies total RF electron emission in MICE Stage 6 is 2.27 THz.  At the tracker ref plane with worst photon rate (per total number of electrons), based on old G4 simulations:  Hence, 2 GHz of photons in the tracker reference plane.  Electrons in track ref 23 MHz.  But very small statistical sample. 10R. Sandström

11 Other unaccounted effects  The multipactorlike avalanche effect I mentioned at CM19 would increase number of electrons from linac.  Unknown if rate increase is significant.  B > 0 increases background.  With a factor according to D. Huang, based on 805 MHz cavity data.  This would give a factor 16 at 3 T if applicable to 201 MHz cavity. 11R. Sandström

12 Old sins not forgotten  An error on the sign of the phasing of cavities was found.  It implies that maximum BG rate is always highest downstream. If running at negative polarity, same rates, but delayed by ½ RF period.  The rates per electron and energy spectrum based on those results unchanged, but upstream should be changed for downstream and vice versa. 12R. Sandström

13 13 http://dpnc.unige.ch/users/rikard/RFBG/

14 Phasing of cavities The energy of most electrons rather insensitive to exact phasing. The “turnaround electrons” however are very sensitive. Left: Phases optimized for 140 MeV/c muon. Note the double reversing electron. R. Sandström14 Downstream Upstream timeposition

15 On request: Heating of absorbers  142 GHz electrons emitted per cavity and direction.  Electron energy almost fully contained within AFC module.  For due to reversing electrons, upstream absorber sees 2 peaks, downstream absorber 6, and center absorber 8.  Thus, center absorber always has maximum load, no matter if electrons are reversing.  For cavities phased by reference 200 MeV/c muon, average electron energy is 3.80 MeV.  142*8*3.8 = 4.317·10 18 eV Hz = 0.691 W  Less for other absorbers.  This is within MICE specifications (TRD: 15 W). 15R. Sandström

16 Summary  MTA PMT16 (NaI) data more reliable for field strengths relevant to MICE.  Calculated rates agree with simulated rates.  Old simulations of MICE + new simulations of MTA + MTA data results in 2 GHz of photons at the downstream tracker reference plane.  One order of magnitude lower rate upstream. 16R. Sandström


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