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Presentation transcript:

Recent Progress in the ECLOUD Simulation for the Cloud Lifetime Study Using Witness Bunch Data All material for this talk may be obtained at www.lepp.cornell.edu/~critten/cesrta/ecloud/3nov10 See also previous talks on simulations for the shielded button data on 4/21, 4/28, 5/12, 7/7, 7/14, 8/4, 9/8, 9/22/2010 A primary purpose of the shielded pickup project (time-resolved measurements) is to measure the cloud lifetime. This lifetime is sensitive to the secondary yield for low-energy cloud particles hitting the vacuum chamber wall. First results on the sensitivity to the parameter d0 using witness bunch data was shown on 9/22/2010 and at ECLOUD10. Those results showed problems with the rising edge of the primary signal and normalization discrepancies at the level of a factor of 4. These have been resolved recently. Also, the modeling of secondaries generated in the SPU port holes has been added to ECLOUD. Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education Electron Cloud Meeting 3 November 2010

ECLOUD simulation for the cloud lifetime study using 5 mA/bunch e+ data at 15E (TiN) Secondary Yield Model True secondary yield: 0.9 True secondary peak energy: 400 eV Rediffused yield: 0.1 Elastic yield d0: 0.55 Two 5-mA bunch spaced by 14, 28, 42, 56, 70, 84 ns. ECLOUD statistical errors are shown. The measured button signals are shown as smooth dotted lines. The measured signals are scaled by an arbitrary factor of 7. Simulated cloud lifetime too long: reduce elastic yield?

ECLOUD cloud lifetime sensitivity to elastic yield d0 -- Status as of ECLOUD10 -- The optimal value for d0 (0.15) is lower than has been generally assumed (0.5-0.7). Note that not only the simulated peak signal value for witness bunch signals is better, but also the width. Could such a low elastic yield be a characteristic of TiN coating? Our tune shift simulations gave reasonable cloud decay times with a value of 0.5 for uncoated aluminum chambers.

New photoelectron energy distribution Green: ECLOUD original Red: ECLOUD10 Blue: better match to data

New SPU Acceptance Model I) Transparency for perpendicular incidence: Aq = 0 = 0.298 II) Angle acceptance: Aq= (1 – q / qmax) 2 III)Position Acceptance: Ax = sqrt(1-x2/r2) IV) Energy acceptance: E > 0.01 eV After the photoelectron energy distribution was corrected a very low energy tail of signal macroparticles inconsistent with the measured signal appeared. John pointed out that these will not traverse the holes if 1 Gauss stray field is present. q qmax

Secondaries generated in the SPU port holes Red: All signal macroparticles Blue: Hole secondaries 1) Direct signal: Qmp Aq=0 Aq Ax 2) Signal from secondaries: Qmp Aq=0 AxAq 2 The acceptance in the secondary angle Aq 2 depends on the average depth and hence on the incident angle q. 3) Normal secondaries generated with Qmp ( 1 - Aq=0 Ax) 4) Ignore hole secondaries which hit the hole wall 5) Ignore secondaries which re-enter the beampipe Time (ns)

ECLOUD cloud lifetime sensitivity to elastic yield d0 -- Present status -- After the SPU acceptance model was implemented, the normalization to the 4-ns 15w Al 5/17 data was within 10%. For this 14-ns 15e TiN 3/27 data, the normalization was high by a factor of 2, so the quantum efficiency has been halved in this simulation. The ratio of the first bunch signal to those of the witness bunches requires a reflectivity of 40% rather than 20%, consistent with SYNRAD3D. The model of the width of the witness bunch signals was improved by lowering the total secondary yield value from 1.0 to 0.8.