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logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting crab cavities E. Cano Pleite, A. Amorim, J. S. Swieszek, K. Artoos, O. Capatina CERN COMSOL CONFERENCE – LAUSSANE – 22/10/2018

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Page 1: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting crab

cavities

E. Cano Pleite, A. Amorim, J. S. Swieszek, K. Artoos, O. Capatina

CERN

COMSOL CONFERENCE – LAUSSANE – 22/10/2018

Page 2: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Outline

Introduction

Numerical model

Results

Overall results

Tunability

Pressure sensitivity

Lorentz force detuning

Conclusions

Page 3: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Outline

Introduction

Numerical model

Results

Overall results

Tunability

Pressure sensitivity

Lorentz force detuning

Conclusions

Page 4: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Introduction - CERN

1

• Radio Frequency System (Acceleration)

• Superconducting magnets (bend trajectory)

• 2 Collimation Regions (Beam Cleaning and Machine

Protection)

• CERN accelerator complex is the largest in the world

• LHC is the last stage and CERN’s flagship

• 27 km underground tunnel

• 2 counter-rotating proton beams• Collisions (experiment location) which generate other particles

Page 5: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Introduction - CERN

1

• Radio Frequency System (Acceleration)

• Superconducting magnets (bend trajectory)

• 2 Collimation Regions (Beam Cleaning and Machine

Protection)

• CERN accelerator complex is the largest in the world

• LHC is the last stage and CERN’s flagship

• 27 km underground tunnel

• 2 counter-rotating proton beams• Collisions (experiment location) which generate other particles

Page 6: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Introduction - HL-LHC

2

Peak luminosities a factor of five larger than LHC

Update on superconducting magnets, high-power superconducting links withzero energy dissipation. New demands on vacuum, cryogenics and machineprotection, and will require new concepts for collimation and diagnostics.

Crab cavities. Transverse deflection of particle bunches.

Double Quarter Wave

RFDipole

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Introduction - Crab cavities

3

Double Quarter Wave (DQW) RF Dipole (RFD)

Operated at 2 K

Page 8: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Introduction - Crab cavities

4

Operated at 2 K

3.4 MV deflecting kick

400.79 MHz fundamental frequency. Tuning system

Double Quarter Wave (DQW) RF Dipole (RFD)

Page 9: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Introduction - Crab cavities

5

Operated at 2 K

3.4 MV deflecting kick

400.79 MHz fundamental frequency. Tuning system.

Pressure sensitivity requirements. Changes of the cavity fundamental frequency due to pressure fluctuations of the cold He bath.

Lorentz force detuning requirements. Change of the cavity fundamental frequency due to radiation forces.

Double Quarter Wave (DQW) RF Dipole (RFD)

Page 10: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Introduction - Crab cavities

5

Operated at 2 K

3.4 MV deflecting kick

400.79 MHz fundamental frequency. Tuning system.

Pressure sensitivity requirements. Changes of the cavity fundamental frequency due to pressure fluctuations of the cold He bath.

Lorentz force detuning requirements. Change of the cavity fundamental frequency due to radiation forces.

Double Quarter Wave (DQW) RF Dipole (RFD)

Page 11: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Outline

Introduction

Numerical model

Results

Overall results

Tunability

Pressure sensitivity

Lorentz force detuning

Conclusions

6

Page 12: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Numerical model

7

Double Quarter Wave

RF Dipole

Page 13: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Numerical model

7

Double Quarter Wave

RF Dipole

Two models:

DQW for tunabilty, validation and mesh sensitivity

RFD for pressure sensitivity (PS), Lorentzforce detuning (LFD) and designoptimization

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Numerical model

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Double Quarter Wave

RF Dipole

Niobium RRR300 for the cavities

55Ti45Nb for the tuning interfaces

Vacuum volume inside the cavity

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Numerical model

9

Double Quarter Wave

RF Dipole

Fundamental frequency of the cavity without any imposed load

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Numerical model

10

Double Quarter Wave

RF Dipole

Structural & moving mesh coupled simulation to capture the cavity and vacuum volume deformation.

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Numerical model

11

Double Quarter Wave

Boundary conditions:

Symmetry

Fixed ports

DQW: imposed displacement in the tuners

Fixed ports

Tuner connection

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Numerical model

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RF Dipole

Boundary conditions:

Fixed ports

Internal pressure

Tuning interfaces

Pressure sensitivity

External pressure of 1 bar(negative internal pressure)

Spring between the tuning interfaces

Fixed ports

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Numerical model

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RF Dipole

Boundary conditions:

Fixed ports

Internal pressure

Tuning interfaces

Lorentz force detuning

Radiation pressure14

Integration of beam kick along the axis

,

,

, cos μ c sin

Page 20: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Numerical model

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Double Quarter Wave

RF Dipole

Fundamental frequency of the deformed cavity

Tunability[kHz/mm]

PS [Hz/mbar]

LFD [Hz/MV2]

,

Page 21: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Outline

Introduction

Numerical model

Results

Overall results

Tunability

Pressure sensitivity

Lorentz force detuning

Conclusions

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Results – DQW cavity

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Cavity displacement (mm)

Comparison with experimental results of the cavity cooldown at CERN at the end of 2017.

Very good agreement between numerical and experimental results.

Cavity tunability = = 315.5 kHz/mm, well in line with expected values.

Incertitude associated to COMSOL and the transformation from displacement to force in the tuning system.

Cavity fundamental frequency vs. force on the tuning system

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Results – RFD cavity

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Pressure sensitivity

244Hz/mbar

Cavity deformation (mm)

Overall results

Energy stored in the cavity for3.4 MV deflecting kick = 10.7 J

Scaling Factor for radiationpressure, SF=7.086·108

Electric field (V/m)

Magnetic field (A/m)

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Results – RFD cavity

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Lorentz force detuning

Magnetic repulsive force

Electric attractive force

Cavity deformation (mm)

Radiation pressure (Pa)

,659Hz/MV

Electric field (V/m)

Magnetic field (A/m)

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Tuning stiffness

• Tuning stiffness, ks, parametric analysis.

• Counteracting effects of deformation inthe pole and tuning regions.

Results – RFD cavity

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Electric field (V/m)

Magnetic field (A/m)

Page 26: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Outline

Introduction

Numerical model

Results

Overall results

Tunability

Pressure sensitivity

Lorentz force detuning

Conclusions

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Page 27: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Conclusions

Tunability, pressure sensitivity and Lorentz force detuning of SRFCrab cavities were numerically evaluated using COMSOL.

The numerical predictions of the DQW cavity tunability matched verywell the experimental results.

Pressure sensitivity and Lorentz force detuning values were usedduring the design stage of the RFD cavity body.

Parametric study on the tuning stiffness is used for the design of thetuning system.

COMSOL is a very powerful tool for the RF-Structural evaluation ofcrab cavities during the validation and design stages.

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Page 28: Numerical evaluation of the tuning, pressure sensitivity and ... pleite...logo area Numerical evaluation of the tuning, pressure sensitivity and Lorentz force detuning of RF superconducting

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Thank you for your attention!