Using tune shifts to evaluate electron cloud effects on beam dynamics at cesrta
Download
1 / 17

Using Tune Shifts to Evaluate Electron Cloud Effects on Beam Dynamics at CesrTA - PowerPoint PPT Presentation


  • 104 Views
  • Uploaded on

Using Tune Shifts to Evaluate Electron Cloud Effects on Beam Dynamics at CesrTA. Jennifer Chu Mentors: Dr. David Kreinick and Dr. Gerry Dugan. Outline. Review of Electron Clouds and Tune Shifts Simulations of New Data Varying the Simulation Parameters. Electron Clouds.

loader
I am the owner, or an agent authorized to act on behalf of the owner, of the copyrighted work described.
capcha
Download Presentation

PowerPoint Slideshow about ' Using Tune Shifts to Evaluate Electron Cloud Effects on Beam Dynamics at CesrTA' - abiba


An Image/Link below is provided (as is) to download presentation

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.


- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -
Presentation Transcript
Using tune shifts to evaluate electron cloud effects on beam dynamics at cesrta

Using Tune Shifts to Evaluate Electron Cloud Effects on Beam Dynamics at CesrTA

Jennifer Chu

Mentors: Dr. David Kreinick and Dr. Gerry Dugan

REU Final Presentation


Outline
Outline Dynamics at CesrTA

  • Review of Electron Clouds and Tune Shifts

  • Simulations of New Data

  • Varying the Simulation Parameters

REU Final Presentation


Electron clouds
Electron Clouds Dynamics at CesrTA

  • ILC will collide electrons and positrons

  • Accelerating charges radiate

  • Photons knock electrons off walls of beampipe

  • Photoelectrons are accelerated by beam and knock off more electrons, forming a cloud

  • Electrons in the cloud are attracted to positive beams

REU Final Presentation


Tune shifts
Tune Shifts Dynamics at CesrTA

  • Beams are displaced from nominal path

  • Tune (Q): number of oscillations of a particle about nominal path, per turn around the ring

  • Tune shift (ΔQ): difference in tune caused by electric field of electron cloud

Qy = 9.52

REU Final Presentation


Taking data
Taking Data Dynamics at CesrTA

  • CesrTA is used to measure tune shifts

  • Beams are set into oscillation

  • BPMs measure the position for 2048 turns

  • Fourier transform is used to calculate tune shifts

REU Final Presentation


Posinst
POSINST Dynamics at CesrTA

  • POSINST is a simulation code used to model the electron cloud effects

  • Simulations are run for different values for each of five parameters which describe the physics of electron cloud generation

  • Simulations are compared to data to test accuracy of the model

REU Final Presentation


Comparing data to simulations
Comparing Data to Simulations Dynamics at CesrTA

REU Final Presentation


Goals
Goals Dynamics at CesrTA

  • We want to find the optimal set of parameters that most accurately models electron clouds

  • The simulation can then be used to predict the behavior of electron clouds in damping rings of future linear colliders

REU Final Presentation


Submitting jobs to the queue
Submitting Jobs to the Queue Dynamics at CesrTA

  • Simulations were run on Cornell’s batch nodes

  • Each job is only allowed 48 hours of CPU time

  • I wrote code to parallel process the simulations to get more statistics

I monopolized the queues for the summer:

87 data sets

x 5 simulation parameters

x 2 for x, y tune shifts

x 6 jobs per submission

-----------------------------------

> 5000 total jobs

REU Final Presentation


Calculating tune shifts
Calculating Tune Shifts Dynamics at CesrTA

  • I used Mathematica to post-process the results of POSINST to calculate the tune shifts

  • I superimposed the tune shifts from multiple simulations onto plots of the data for comparison

REU Final Presentation


June 2011 coherent tune shift data
June Dynamics at CesrTA2011 Coherent Tune Shift Data

  • 2.085 GeV e+: 20 x 0.5 mA

  • 2.085 GeV e+: 45 x 0.5, 1.0, 1.5, 2.0mA

  • 4.00 GeV e+: 20 x 0.2, 0.4, 0.6, 0.8, 1.0, 1.2, 1.4, 1.6, 1.8, 2.0 mA

  • 4.00 GeV e+: 45 x 0.2, 0.4, 0.6, 0.8, 1.0, 1.2 mA

  • 5.3 GeV e+: 20 x 0.5, 1.0, 2.0 mA

  • 5.3 GeV e-: 20 x 1.0, 2.0, 3.0, 4.0, 5.0, 6.0, 7.0, 8.0, 9.0 mA

  • 5.3 GeV e+: 45 x 0.2, 0.4, 0.6, 0.8, 1.0, 1.2 mA

  • 5.3 GeV e-: 45 x 0.2, 0.4, 0.6, 0.8, 1.0, 1.2, 1.4, 1.6, 1.8, 2.0, 2.2, 2.4, 2.6 mA

    Bunch spacing studies:

  • 2.085 GeV e-: 30 x 0.2, 0.4, 0.6, 0.8, 1.0, 1.2 mA for 12, 16, 20 ns spacing

  • 2.085 GeV e-: 45 x 0.2, 0.4, 0.6, 0.8, 1.0, 1.2 mA for 4, 8, 12 ns spacing

REU Final Presentation


2 1 gev 4 0 gev 5 3 gev
2.1 GeV Dynamics at CesrTA 4.0 GeV 5.3 GeV

0.50 mA/bunch

0.40 mA/bunch

0.50 mA/bunch

1.00 mA/bunch

1.00 mA/bunch

1.00 mA/bunch

REU Final Presentation


Simulation parameters
Simulation Parameters Dynamics at CesrTA

  • Parameters describe the physics of electron cloud generation

  • When a radiated photon from the beam knocks into the wall of the beampipe, photoelectrons are generated

  • (1) Quantum Efficiency: number of electrons generated for every photon

REU Final Presentation


Secondary emission
Secondary Emission Dynamics at CesrTA

  • Photoelectrons are accelerated by the electric field of the beam and continue to produce more electrons

  • (2) Secondary Emission Yield (SEY): number of secondary electrons generated for every primary electron

  • (3) Energy at the SEY Peak

REU Final Presentation


Types of secondary electrons
Types of Secondary Electrons Dynamics at CesrTA

  • When a photoelectron hits a wall of the vacuum chamber, it can:

  • Bounce off (elastic)

  • Interact with material (rediffused)

  • Knock off electrons in material (true)

  • (4) Fraction of Secondaries that are Rediffused

  • (5) Fraction of Secondaries that are Elastic

Sketch of the currents that are used to define the different components of secondary emission.

Figure taken from M. Furman and G. Lambertson, “The electron-cloud instability in the arcs of the PEP-II positron ring”

REU Final Presentation


Varying the simulation parameters
Varying the Simulation Parameters Dynamics at CesrTA

REU Final Presentation


Summary
Summary Dynamics at CesrTA

  • Tune shifts are used to study electron clouds

  • Simulations were run and compared to data for all five parameters and all 77 new data sets

  • Model seems to work reasonably well for a variety of beam energies and bunch currents

  • Finding the optimal parameters will allow the model to be used for future linear colliders

REU Final Presentation


ad