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Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 1/27 Instabilities Simulations with Wideband Feedback Systems: CMAD, HeadTail, WARP K. Li 1 , H. Bartosik 1 , J. Cesaratto 2 , J. D. Fox 2 , W. Höfle 1 , M. Furman 3 , G. Iadorola 1 , M. Pivi 2 , C. Rivetta 2 , G. Rumolo 1 , R. Secondo 1 , O. Turgut 2 , S. Uemuda 2 , J.-L. Vay 3 1 European Organization for Nuclear Research 2 SLAC National Accelerator Laboratory 3 Lawrence Berkeley National Laboratory Work supported by DOE

Instabilities Simulations with Wideband Feedback Systems

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Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 1/27

Instabilities Simulations with Wideband Feedback Systems: CMAD, HeadTail,

WARP

K. Li 1, H. Bartosik 1, J. Cesaratto 2, J. D. Fox 2, W. Höfle 1, M. Furman 3, G. Iadorola 1, M. Pivi 2, C. Rivetta 2, G. Rumolo 1, R.

Secondo 1, O. Turgut 2, S. Uemuda 2, J.-L. Vay 3

1 European Organization for Nuclear Research2 SLAC National Accelerator Laboratory

3 Lawrence Berkeley National Laboratory

Work supported by DOE

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 2/27

Outline

i. Simulation models – CMAD, HeadTail, WARP

ii.Feedback system model

iii.Damping the centroid motion

iv.Electron cloud instabilities

v.Damping the intra-bunch motion

vi.Conclusions and outlook

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 3/27

C-MAD, HeadTail, WARP - Models

CMAD HeadTail WARP

Language Fortran C++ Fortran with Python interface

Parallel yes no yes

Optics Smooth or lattice(MAD-X import)

Smooth or lattice (MAD-X import)

Smooth or lattice

PIC 2D FFT 2D FFT AMR (includes space charge)

Binning Constant space or constant charge

Constant space Constant space

Distributions Internal & external Internal & external Internal, external & build-up

Extras IBS, radiation damping, quantum excitation

ZBASE impedance database

Build-up + tracking (strong-strong)

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 4/27

Feedback system implementation

Filter receiver● Pick-up● Cables● Receiver● ADC● Saturation

Processing channel

● FIR-IIR filterswith intrinsic delay

Noise receiver

Filter kicker● DAC● Amplifier● Cables● Kicker● Saturation

Gain

Noise amplifier Excitation

yout

vout

yslice

ykick

yin

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 5/27

Feedback system - specifications

5 tap delay

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 6/27

Feedback system - specifications

5 tap delay

FIR transfer functions (left)

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 7/27

Feedback system - specifications

5 tap delay

FIR transfer functions (left)

Kicker transfer functions (right)

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 8/27

Centroid motion – gain scanBandwidths:200MHz, 500MHz, 700MHz, 1GHz

Perturbation: 2mm initial vertical offset → monitor bunch response

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 9/27

Centroid motion – gain scanBandwidths:200MHz, 500MHz, 700MHz, 1GHz

Perturbation: 2mm initial vertical offset → monitor bunch response

For high gains, the limited (200MHz) bandwidth makes the system become unstable

200 MHz

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 10/27

Centroid motion – gain scanBandwidths:200MHz, 500MHz, 700MHz, 1GHz

Perturbation: 2mm initial vertical offset → monitor bunch response

For high gains, the limited (200MHz) bandwidth makes the system become unstable

For all cases, the bunch response (centroid motion) to the initial perturbation is similar → the systems perform equally well

0 2 4 6 8 10 120

0.5

1

1.5

2

2.5

3

3.5

200 MHz

500 MHz

700 MHz

1000 MHz

Gain [1e-3]

Da

mp

ing

tim

e [m

s]

200 MHz

500 MHz

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 11/27

Comparision CMAD-HeadTail

Perturbation: 2mm initial vertical offset

Gain g ≈ 8.5e-3

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 12/27

ECI – ρe scan

Intensity 1.1e11 ppb

Energy 26 GeV

Emittances [epsx, epsy] 2.8, 2.8 microns

Beta-functions [βx, βy] 42, 42 m

Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059

E-cloud region Bends

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 13/27

ECI – ρe scan

Intensity 1.1e11 ppb

Energy 26 GeV

Emittances [epsx, epsy] 2.8, 2.8 microns

Beta-functions [βx, βy] 42, 42 m

Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059

E-cloud region Bends

The instability threshold is around ρ

e ≈ 4e11 m-3

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 14/27

ECI – ρe scan

Intensity 1.1e11 ppb

Energy 26 GeV

Emittances [epsx, epsy] 2.8, 2.8 microns

Beta-functions [βx, βy] 42, 42 m

Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059

E-cloud region Bends ρe = [1,16] x 1e11 m-3

The instability threshold is around ρ

e ≈ 4e11 m-3

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 15/27

ECI – ρe scan

The instability threshold is around ρ

e ≈ 4e11 m-3

Unstable modes are {0, -1, -2}

Intensity 1.1e11 ppb

Energy 26 GeV

Emittances [epsx, epsy] 2.8, 2.8 microns

Beta-functions [βx, βy] 42, 42 m

Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059

E-cloud region Bends ρe = [1,16] x 1e11 m-3

ρe [1e11 m-3]

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 16/27

ECI – ρe ≈ 6e11 m-3

Clear coherent motion above the instability threshold

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 17/27

ECI – ρe ≈ 6e11 m-3

Clear coherent motion above the instability threshold

The mode evolution reveals the presence of predominantly modes {0, -1, -2} (shifted)

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 18/27

Intra-bunch – ρe ≈ 6e11 m-3 – gain scan

Perturbation: electron cloud

Bandwidths:200MHz, 500MHz, 700MHz, 1GHz

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 19/27

Intra-bunch – ρe ≈ 6e11 m-3 – gain scan

Perturbation: electron cloud

Bandwidths:200MHz, 500MHz, 700MHz, 1GHz

For high gains, the limited (200MHz) bandwidth makes the system become unstable

200 MHz

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 20/27

Intra-bunch – ρe ≈ 6e11 m-3 – gain scan

Perturbation: electron cloud

Bandwidths:200MHz, 500MHz, 700MHz, 1GHz

For high gains, the limited (200MHz) bandwidth makes the system become unstable

A gain of 6e-3 appears to damp the ECI

200 MHz

500 MHz

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 21/27

500MHz – ρe scan – gain = 6e-3

Coherent motion is damped within the rangeρ

e = [1,10] x 1e11 m-3

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 22/27

500MHz – ρe scan – gain = 6e-3

Coherent motion is damped within the rangeρ

e = [1,10] x 1e11 m-3

The power in modes{-1,0,1} is effectively diminished

The remaining power appears to be distributed over a wide range of modes

ρe [1e11 m-3]

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 23/27

500MHz – ρe ≈ 6e11 m-3 – gain = 6e-3

Clear damping of the coherent motion

Remaining power is distributed over modes {2,6}

24/27

Feedback power required

Same scale: Low feedback power is required to stabilize the beam in the presence of electron cloud

Feedback ON: no electron cloud Feedback ON: ecloud density 5e11/m3

Kick applied to individual bunch slices by the feedback system

x 1e-5x 1e-5

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 25/27

500MHz – ρe ≈ 14e11 m-3 – gain = 6e-3

Clear re-emerging of the coherent motion

Power is concentrated predominantly in modes {6} (shifted)

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 26/27

Conclusions & outlook

Successful implementation of realistic feedback system into multi-particle instability codes

Mode analysis of ECI reveals unstable modes up to mode 2 (for the investigated configuration)

200MHz feedback is insufficient to damp ECI

500MHz feedback provides damping withinfor gains > 6e-3

Study the impact of noise on the feedback effectiveness

Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 27/27

Thank you for your attention!