Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the...

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CERN Accelerator School, Divonne 2009 Erk Jensen, CERN BE-RF

Transcript of Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the...

Page 1: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

Erk Jensen, CERN BE-RF

Page 2: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009 2RF II24 February, 2009

Page 3: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

RR/b

Cavity

Generator

IG

Z

P

C=Q/(Rw0)

Vgap

Beam

IB

L=R/(Qw0)LC

b: coupling factor

R: Shunt impedance : R-upon-Q

Simplification: single mode

We have used this before when explaining the “fast feedback”

3RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 4RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

Example: KEK photon factory 500 MHz

- R as good as it gets -

this cavity optimized

pillbox

R/Q: 111 W 107.5 W

Q: 44270 41630

R: 4.9 MW 4.47 MW

Nose cones increase transit time factor, round outer shape minimizes losses.

nose cone

5RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

0 5 10 15 20

t f0

-1

0

1

Voltage induced by a single charge q:

RR/b

Cavity

Beam

C=Q/(Rw0)

V (induced)IB

L=R/(Qw0)LCEnergy deposited by a

single charge q:

Impedance seen by the beam

6RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

Vgap

gap voltage

Ploss

Power lost in the cavity walls

W

Energy stored inside the cavity

7RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

The beam current “loads” the generator, in the equivalent circuit this appears as a resistance in parallel to the shunt impedance.

If the generator is matched to the unloaded cavity, beam loading will cause the accelerating voltage to decrease.

The power absorbed by the beam is , the

power loss .

For high efficiency, beam loading shall be high.

The RF to beam efficiency is .

8RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

Resonance frequency

Transit time factor

field varies while particle is traversing the gap

Shunt impedance

gap voltage – power relation

Q factor

R/Qindependent of losses – only geometry!

loss factor

Linac definitionCircuit definition

9RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

IB

R3, Q3,w3R2, Q2,w2R1, Q1,w1

......

external dampers

n1 n3n2

10RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

without dampers

with dampers

11RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

electric field (@ 0º) magnetic field (@ 90º)

(only 1/8 shown)(TM110)

12RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

For particles moving virtually at v=c, the integrated transverse force (kick) can be determined from the transverse variation of the integrated longitudinal force!

W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged

Particles in Radio-Frequency Fields”, RSI 27, 1957]

Pure TE modes: No net transverse force !

Transverse modes are characterized by

• the transverse impedance in w-domain

• the transverse loss factor (kick factor) in t-domain !

13RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

inductive (loop) coupling, low self-inductance

14RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

Example shown:80 MHz cavity PS for LHC.

Color-coded:

15RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 16RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 17RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

PEP II cavity476 MHz, single cell,

1 MV gap with 150 kW, strong HOM damping,

LEP normal-conducting Cu RF cavities,350 MHz. 5 cell standing wave + spherical cavity for energy storage, 3 MV

18RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

example for capacitive coupling

cavity

coupling C

19RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 20RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

• The R/Q of a single gap cavity is limited to some 100 W.

Now consider to distribute the available power to n

identical cavities: each will receive P/n, thus produce an

accelerating voltage of .

The total accelerating voltage thus increased,

equivalent to a total equivalent shunt impedance of .

1 2 3 n

P/n P/nP/n P/n

21RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

• Instead of distributing the power from the amplifier, one might as well couple the cavities, such that the power automatically distributes, or have a cavity with many gaps (e.g. drift tube linac).

• Coupled cavity accelerating structure (side coupled)

• The phase relation between gaps is important!

22RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

A 3 GHz Side Coupled Structure to accelerate protons out of cyclotrons from 62 MeV to 200 MeV

Medical application:treatment of tumours.

Prototype of Module 1built at CERN (2000)

Collaboration CERN/INFN/Tera Foundation

23RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

This Picture made it to the title page of CERN Courier vol. 41 No. 1 (Jan./Feb. 2001)

24RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 25RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

synchronous

2p

w L/c

speed of light line,

w = b /c

p

p/2

pp/2 b L0

0

p/2

p

2p/3

26RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

1 cm

30 GHz structure (CLIC)

11.4 GHz structure (NLC)

27RF II24 February, 2009

Page 28: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

Dimensions in mm

28RF II24 February, 2009

Page 29: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

¼ geometry shown

Input coupler

Output coupler

Travelling wave structure(CTF3 drive beam, 3 GHz)

shown: Re {Poynting vector} (power density)

29RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 30RF II24 February, 2009

Page 31: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

-4.00

-2.00

0.000E+00

2.00

4.00

0.000E+00 0.500 1.00 1.50 2.00 2.50

FRAME: 1 01/06/00 - 17:06:38 VERSION[V4.024] SICA32.DRD

SI: A+3,10,4, B-5,CELL-6,15

A: 1.700E+01 MM, B: 3.703E+01 MM.

FOR REF., E.J., JUNE 2000

X COMPONENT OF WAKE POTENTIAL IN V [INDIRECT CALC.]

OP-:4024

#1DGRAPH

ORDINATE: WAKETCOMPONENT: X

FIXED COORDINATES:DIM...........MESHLINE X 11 Y 1

ABSCISSA: GEOMWAKE[BASE OF WAKET]

REFERENCE COORDINATE: SVARY..........MESHLINEFROM 0 TO 2994

3 GHz SICA structure: Transverse wake suppression

s [m]

transverse wake for 3 cells.

offset 10 mm, 2.5 mms

W [V/pC]t

31RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

“T18” reached 105 MV/m!“HDS” – novel fabrication technique

32RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 33RF II24 February, 2009

Page 34: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

Different from DC, at RF the resistance is not exactly zero, but just very small. It is

The maximum accelerating gradient is normally limited by the maximum possible surface magnetic field (the “superheating field”, 180 mT for Nb, 400 mT for Nb3Tn).

Maximum acc. gradients are however obtained for Nb (ILC, ≈ 40 MV/m).

1.3 GHz

34RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

10.2 MV/ per cavity

35RF II24 February, 2009

Page 36: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

25 -35 MV/m

36RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 37RF II24 February, 2009

Page 38: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009 38RF II24 February, 2009

Page 39: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

All this was replaced by the RFQ …

39RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 40RF II24 February, 2009

Page 41: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

Minimum Energy of a DTL: 500 keV (low duty) - 5 MeV (high duty)At low energy / high current we need strong focalisationMagnetic focusing (proportional to b) is inefficient at low energy. Solution (Kapchinski, 70’s, first realised at LANL):

Electric quadrupole focusing + bunching + acceleration

41RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

The electrode modulation creates a longitudinal field component that creates the“bunches” and accelerates the beam.

42RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 43RF II24 February, 2009

Page 44: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009 44RF II24 February, 2009

Page 45: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

Typical ranges (commercially available)

0.1

1

10

100

1000

10000

10 100 1000 10000f [MHz]

CW

/Ave

rag

e p

ow

er

[kW

]

Transistors

solid state (x32)

grid tubes

klystrons

IOT CCTWTs

45RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

MRF151G

46RF II24 February, 2009

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CERN Accelerator School, Divonne 2009http://accelconf.web.cern.ch/AccelConf/e04/PAPERS/THPKF031.PDF

147 modules

DU1029UK

47RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

RS 1084 CJ (ex Siemens, now Thales),

< 30 MHz, 75 kW

YL1520 (ex Philips, now Richardson),

< 260 MHz, 25 kW

4CX250B

(Eimac/CPI),

< 500 MHz, 600 W

(Anode removed)

48RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

CERN Linac3: 100 MHz, 350 kW

CERN PS: 13-20 MHz, 30 kW

50 kW Driver: TH345, Final: RS 2054 SK

Driver: solid state 400 W, Final: RS 1084 CJSC

49RF II24 February, 2009

Page 50: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

RF in RF out

CathodeCollector

z

t

velocity

modulationdrift

density

modulation

-V0

50RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

CERN CTF3 (LIL):

3 GHz, 45 MW,

4.5 ms, 50 Hz, h 45 %

CERN LHC:

400 MHz, 300 kW,

CW, h 62 %

51RF II24 February, 2009

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CERN Accelerator School, Divonne 2009 52RF II24 February, 2009

Page 53: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

0 2000 4000 6000 80000

2

4

6

0 2000 4000 6000 80000

2

4

6

0 2000 4000 6000 80000

180

360

“SLED” outputpulse

Input phaseInput pulse

SLED: SLAC Energy Doubler LIPS: LEP Injector Power Saver

1 2

34

53RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

2.57961

0

Ci 1

6.94444 103.0 C

i 0

0 2000 4000 6000 80000

1

2

3

2.32804

0

Ci 1

6.94444 103.0 C

i 0

0 2000 4000 6000 80000

1

2

3179.999848

0

Ci 1

180

p

.

65004500 Ci 0

5000 60000

100

200

179.999848

0

Ci 1

180

p

.

C1i 1

180

p

.

65004500 Ci 0

5000 60000

100

2002.37117

0

Ci 1

6.94444 103.0 C

i 0

0 2000 4000 6000 80000

1

2

3

5.27181

0

Ci 1

6.94444 103.0 C

i 0

0 2000 4000 6000 80000

2

4

6

Standard “SLED”Pulse

RF phasemodulation

Flat pulse

Distorted pulseFlat pulse RF phasemodulation

-10 kHz

Old

New

54RF II24 February, 2009

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CERN Accelerator School, Divonne 2009

BOC „Barrel Open Cavity“

55RF II24 February, 2009

Page 56: Erk Jensen, CERN BE-RF · W.K.H. Panofsky, W.A. Wenzel: “Some Considerations Concerning the Transverse Deflection of Charged Particles in Radio-Frequency Fields”, RSI 27, 1957]

CERN Accelerator School, Divonne 2009

Electric field, logarithmic scale

2.99848 GHz,S11: -12.9 dB

Magnetic field

56RF II24 February, 2009