CESR Test Accelerator – Investigation of the physics of charged particle beams
description
Transcript of CESR Test Accelerator – Investigation of the physics of charged particle beams
David L. Rubin 1November 18, 2011
CESR Test Accelerator – Investigation of the physics of charged particle beams
Circumference = 768m - Beam energy 1.8-5.5 GeV - Electrons and Positrons
David L. Rubin 2November 18, 2011
Linear Collider Energy/beam = 250-500 GeV ECM = 0.5-1.0 TeV
David L. Rubin 3November 18, 2011
Electron cloud
David L. Rubin 4
Shielded pickup
November 18, 2011
David L. Rubin 5
Shielded Pickup
November 18, 2011With no magnetic field, electrons come from the floor of the chamber
Cloud Evolution: Witness Bunch Studies
TiN Chamber
November 18, 2011 6David L. Rubin
Cloud is generated by the first bunch. The witness bunch follows and kicks the cloud electrons into the pickup. Decay time of the cloud is evident.
7
Example: Positron Witness Bunch Study at 2GeV
November 18, 2011 David L. Rubin
Peak SEY ScanCoherent Tune Shifts (1 kHz ~ 0.0025), vs. Bunch Number - 21 bunch train, followed by 12 witness bunches - 0.8×1010 particles/bunch - 2 GeV. - Data (black) compared to POSINST simulations.
SEY=2.0
SEY=1.8
SEY=2.2Train
Witnesses
David L. Rubin 8November 18, 2011
Low emittance tuning procedure typically yields sub 20pm in one or two iterations
σ =17μmεv = 18pm
D-line xbsm - positrons
David L. Rubin 9
32 Channel Detector Output For 20 Bunches, 1 mA Per Bunch
November 18, 2011
C-line – electron beam size20 bunches,14 ns spacing, 32 channels, pinhole optics Capability to measure bunches spaced by as few as 4ns
David L. Rubin 10November 18, 2011
C-line – electron beam size
Joe Calvey – Electron cloudJim Shanks – Low Emittance TuningMike Ehrlichman – Intra-beam scattering
CesrTA Grad students
David L. Rubin 11November 18, 2011
David L. Rubin 12November 18, 2011
David L. Rubin 13November 18, 2011
David L. Rubin 14November 18, 2011