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Lecture - CASA - Jefferson Lab

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Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

Energy Recovered Linacs,<br />

Short Pulses of X-rays X-rays,<br />

and Non-linear Thomson Scattering<br />

G. A. Krafft<br />

<strong>Jefferson</strong> <strong>Lab</strong><br />

ODU Colloquium<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

15 February 2005


Outline<br />

• Recirculating linacs defined and described<br />

• Review of recirculating SRF linacs<br />

• Energy recovered linacs<br />

• Energy recovered linacs as light sources<br />

• Ancient history: lasers and electrons<br />

• Dipole emission from a free electron<br />

• Thomson scattering<br />

• Motion of an electron in a plane wave<br />

1. Equations of motion<br />

2. Exact solution for classical electron in a plane wave<br />

• Applications to scattered spectrum<br />

1. General solution for small a<br />

2. Finite a effects<br />

33. Ponderomotive broadening<br />

4. Sum Rules<br />

• Conclusions<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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15 February 2005


Schematic Representation of Accelerator Types<br />

Linac<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

Recirculating<br />

Linac<br />

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RF Installation<br />

Beam injector and dump<br />

Beamline<br />

Ring<br />

15 February 2005


Why Recirculate?<br />

. Performance upgrade of a previously installed linac<br />

- Stanford Superconducting Accelerator and MIT Bates doubled their<br />

energy this way<br />

. Cheaper design to get a given performance<br />

- Microtrons, by many passes, reuse expensive RF many times to get<br />

energy up. Penalty is that the average current has to be reduced<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

proportional to 1/number passes, for the same installed RF.<br />

- <strong>Jefferson</strong> <strong>Lab</strong> CEBAF type machines: add passes until the<br />

“decremental” gain in RF system and operating costs pays for<br />

additional recirculating loop<br />

- <strong>Jefferson</strong> <strong>Lab</strong> FEL and other Energy Recovered Linacs (ERLs) save<br />

the cost of higher average power RF equipment (and much higher<br />

operating costs) at higher CW operating currents by “reusing” beam<br />

energy through beam recirculation.<br />

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15 February 2005


Beam Energy Recovery<br />

r r<br />

dγeE⋅v = 2<br />

dt mc<br />

Recirculation path length in standard configuration recirculated linac. For energy<br />

recovery choose h iit to be b (n ( + 1/2)λ 1/2)λ. Th Then<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

dγ<br />

tot<br />

dt<br />

=<br />

0<br />

ODU Colloquium<br />

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15 February 2005


Beam Energy Recovery<br />

Recirculation path length in herring herring-bone bone configuration recirculated linac. For<br />

energy recovery choose it to be nλ. Note additional complication: path length has to<br />

be an integer at each and every different accelerating cavity location in the linac.<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

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15 February 2005


Comparison between Linacs and Storage Rings<br />

. Advantage Linacs<br />

EEmittance itt dominated d i t d by b source emittance itt and d emittance itt growth th down d linac li<br />

Beam polarization “easily” produced at the source, switched, and preserved<br />

Total transit time is quite short<br />

BBeam iis easily il extracted. t t d Utilizing Utili i source control, t l flexible fl ibl bunch b h patterns tt possible ibl<br />

Long undulaters are a natural addition<br />

Bunch durations can be SMALL (10-100 fsec)<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

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15 February 2005


Comparison Linacs and Storage Rings<br />

. Advantage Storage Rings<br />

Up to now now, the stored average current is much larger<br />

Very efficient use of accelerating voltage<br />

Technology well developed and mature<br />

. Disadvantage of Storage Rings<br />

Technology well developed and mature<br />

Th There’s ’ nothing thi you can ddo about b t synchrotron h t radiation di ti damping d i and d the th<br />

emittance and bunch length it generates<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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15 February 2005


Power Multiplication Factor<br />

. An advantage of energy recovered recirculation is nicely quantified by the<br />

notion of a power p multiplication p factor:<br />

k = P /<br />

b,<br />

ave<br />

where P rf is the RF power needed to accelerate the beam<br />

. By the first law of thermodynamics (energy conservation!) k < 1<br />

in any linac not recirculated. Beam recirculation with beam deceleration<br />

somewhere is necessary to achieve k > 1<br />

. If energy IS very efficiently recycled from the accelerating to the decelerating<br />

beam<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

k<br />

>><br />

P<br />

1<br />

rf<br />

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15 February 2005


High Multiplication Factor Linacs<br />

Normal Conducting g Recirculators k


Comparison Accelerator Types<br />

Parameter High Energy<br />

Electron Linac<br />

High k Recirculated<br />

Superconducting Linac<br />

Accelerating Gradient[MV/m] >50 10 10-20 20 NA<br />

Duty Factor


Another Reason to Recirculate!<br />

. A renewed general interest in beam recirculation has arisen due to the<br />

success in <strong>Jefferson</strong> <strong>Lab</strong>’s high average current Free Electron Lasers (FELs),<br />

and the broader realization that it may y be possible p to achieve beam parameters p<br />

“Unachievable” in linacs without recirculation.<br />

ERL synchrotron source: Beam power is (100 mA)(5 GeV)=500 MW.<br />

Realistically Realistically, even the federal govt. govt will be unable to provide a third of a<br />

nuclear plant to run a synchrotron source. Use the high multiplication<br />

factor possible in energy recovered designs to reduce the power load.<br />

Pulse lengths of order 100 fsec or smaller may in be possible in a ERL<br />

source; “impossible” at a storage ring ring. Better emittance too. too<br />

The limits, in particular the average current carrying capacity of possible<br />

designs, g , are not yet y determined and may y be far in excess of what the FELs can<br />

do!<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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15 February 2005


Challenges for Beam Recirculation<br />

. Additional Linac Instability<br />

- Multipass Beam Breakup (BBU)<br />

- Observed first at Illinois Superconducting Racetrack Microtron<br />

- Limits the average current at a given installation<br />

- Made better by y damping p g non-fundamental electromagnetic g High g Order<br />

Modes (HOMs) in the cavities<br />

- Best we can tell at CEBAF, threshold current is around 20 mA, several<br />

mA in the FEL<br />

- Changes based on beam recirculation optics<br />

. Turn around optics tends to be a bit different than in storage rings or more<br />

conventional linacs. Longitudinal beam dynamics gets coupled strongly to the<br />

transverse ta svesedy dynamics. a cs.<br />

. HOM cooling will perhaps limit the average current in such devices.<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

15 February 2005


Challenges for Beam Recirculation<br />

. High average current sources to provide beam<br />

- Right now, now looks like s good way to get there is with DC photocathode<br />

sources as we have in the <strong>Jefferson</strong> <strong>Lab</strong> FEL.<br />

- Need higher fields in the acceleration gap in the gun.<br />

- Need better vacuum performance in the beam creation region to increase<br />

the photocathode lifetimes.<br />

- Goal is to get the photocathode decay times above the present storage ring<br />

Toushek lifetimes<br />

. Beam dumping of the recirculated beam can be a challenge.<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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15 February 2005


Recirculating SRF Linacs<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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15 February 2005


The CEBAF at <strong>Jefferson</strong> <strong>Lab</strong><br />

Most radical innovations (had not been done before on the scale of CEBAF):<br />

• choice of Superconducting Radio Frequency (SRF) technology<br />

• use of multipass beam recirculation<br />

Until LEP II came into operation, CEBAF was the world’s largest implementation of<br />

SRF technology.<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

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15 February 2005


CEBAF Accelerator Layout*<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

*C. W. Leemann, D. R. Douglas, G. A. Krafft, “The Continuous Electron<br />

Beam Accelerator Facility: CEBAF at the <strong>Jefferson</strong> <strong>Lab</strong>oratory”, Annual<br />

Reviews of Nuclear and Particle Science, 51, 413-50 (2001) has a long<br />

reference list on the CEBAF accelerator. Many references on Energy<br />

Recovered Linacs may be found in a recent ICFA Beam Dynamics<br />

Newsletter, l #26, #26 Dec. 2001: 2001 http://icfa- h //i f<br />

usa/archive/newsletter/icfa_bd_nl_26.pdf<br />

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15 February 2005


CEBAF Beam Parameters<br />

Beam energy 6 GeV<br />

Beam current A 100 µA, B 10-200 nA, C 100 µA<br />

Normalized rms emittance 1 mm mrad<br />

RRepetition i i rate 500 MH MHz/Hall /H ll<br />

Charge per bunch < 0.2 pC<br />

Extracted energy spread


Short Bunches in CEBAF<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

Wang, Krafft, and Sinclair, Phys. Rev. E, 2283 (1998)<br />

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15 February 2005


Short Bunch Configuration<br />

bunch<br />

leengthh<br />

(fs)<br />

250<br />

200<br />

150<br />

100<br />

50<br />

0<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

0 50 100 150<br />

Beam current (µA)<br />

KKazimi, i i Sinclair, Si l i and dKrafft, K fft PProc. 2000 LINAC Conf., C f 125 (2000)<br />

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15 February 2005


dp/p data: 2-Week Sample Record<br />

EEnergy Spread S d less l than th 50 ppm in i Hall H ll C, C 100 ppm in i Hall H ll A<br />

Primary Hall (Hall C)<br />

Energy drift<br />

Energy spread<br />

X Position => relative energy Drift<br />

rms X width => Energy Spread<br />

12 1.2<br />

08 0.8<br />

04 0.4<br />

23-Mar 27-Mar 31-Mar<br />

0<br />

4-Apr<br />

Date<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

mm<br />

X andd<br />

sigma X in<br />

1E-4<br />

12 1.2<br />

08 0.8<br />

04 0.4<br />

0<br />

ODU Colloquium<br />

Secondary Hall (Hall A)<br />

Energy drift<br />

Energy spread<br />

23-Mar 27-Mar 31-Mar 4-Apr<br />

Time<br />

Courtesy: Jean-Claude Jean Claude Denard<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

15 February 2005


Energy Recovered Linacs<br />

The concept of energy recovery first appears in literature by<br />

Maury Tigner, as a suggestion for alternate HEP colliders*<br />

There have been several energy recovery experiments to date, the<br />

first one in a superconducting linac at the Stanford SCA/FEL**<br />

Same-cell energy recovery with cw beam current up to 10 mA and<br />

energy up to 150 MeV has been demonstrated at the <strong>Jefferson</strong> <strong>Lab</strong><br />

10 kW FEL FEL. Energy recovery is used routinely for the operation of<br />

the FEL as a user facility<br />

* M Maury Tigner, Ti Nuovo N Cimento Ci t 37 (1965)<br />

** T.I. Smith, et al., “Development of the SCA/FEL for use in Biomedical and<br />

Materials Science Experiments,” NIMA 259 (1987)<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

15 February 2005


The SCA/FEL Energy Recovery Experiment<br />

Same-cell energy recovery was first demonstrated in an SRF linac at the<br />

SCA/FEL in July 1986<br />

Beam was injected at 5 MeV into a ~50 MeV linac<br />

The first recirculation system (SCR, 1982) was unsuccessful in obtaining the<br />

peak current required for lasing and was replaced by a doubly achromatic<br />

single-turn recirculation line.<br />

All energy was recovered. d FEL was not t in i place. l<br />

T. I. Smith, et al., NIM A259, 1 (1987)<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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15 February 2005


The CEBAF Injector Energy Recovery Experiment<br />

N. R. Sereno, “Experimental Studies of Multipass Beam Breakup and Energy<br />

Recovery using the CEBAF Injector Linac,” Ph.D. Thesis, University of<br />

Illi Illinois i (1994)<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

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15 February 2005


Instability Mechanism<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

Courtesy: N. Sereno, Ph.D. Thesis (1994)<br />

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15 February 2005


Threshold Current*<br />

Growth Rate<br />

where<br />

( ω λ t r ) ω λ<br />

κ sin<br />

Im ( ωω<br />

) ≈ −<br />

−<br />

2t<br />

2Q<br />

κ =<br />

2 ( Q)<br />

k eT I t / 2<br />

R λ<br />

/ λ 12 0 0<br />

If the average current exceeds the threshold current<br />

I<br />

th<br />

=<br />

1<br />

e<br />

0<br />

2<br />

( R / Q ) Q k T sin ( ω t )<br />

λ<br />

λ<br />

2ω<br />

have instability (exponentially growing cavity amplitude!)<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

λ<br />

λ<br />

12<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

λ<br />

λ<br />

r<br />

*Krafft, Bisognano, and Laubach, unpublished (1988)<br />

ODU Colloquium<br />

15 February 2005


The <strong>Jefferson</strong> <strong>Lab</strong> IR FEL<br />

Wiggler assembly<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

Neil, G. R., et. al, Physical Review Letters, 84, 622 (2000)<br />

ODU Colloquium<br />

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15 February 2005


FEL Accelerator Parameters<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

PParameter t DDesigned i d MMeasuredd Kinetic Energy 48 MeV 48.0 MeV<br />

Average current 5mA 5 mA 48mA 4.8 mA<br />

Bunch charge 60 pC Up to 135<br />

pC<br />

Bunch length<br />

(rms)<br />


ENERGY RECOVERY WORKS<br />

GGradient di modulator d l drive d i signal i l in i a linac li cavity i measured d without i h energy recovery<br />

(signal level around 2 V) and with energy recovery (signal level around 0).<br />

Volttage<br />

(V)<br />

2.5<br />

2<br />

1.5<br />

1<br />

0.5<br />

0<br />

-0.5<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

GASK<br />

-1.00E-04 0.00E+00 1.00E-04 2.00E-04 3.00E-04 4.00E-04 5.00E-04<br />

Time (s)<br />

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Courtesy: Lia Merminga<br />

15 February 2005


Thomson Source Scattering Geometry<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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15 February 2005


60 sec FEL Short-pulse X-ray Spectrum<br />

Countts<br />

2000<br />

1500<br />

1000<br />

500<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

0<br />

Ee- = 36.7 MeV<br />

λ λL =5181µm<br />

= 5.181 µm<br />

IR = 250 Watts, cw<br />

Live run time = 60 sec.<br />

EX-ray = 5.12 keV<br />

FWHM = 0.319 keV<br />

Lasing<br />

FEL X-ray Spectra<br />

Boyce, Krafft, et al.<br />

Sept. 30, 1999<br />

Preliminary<br />

Not Lasing<br />

0 200 400 600 800 1000<br />

Ch Channel l number b<br />

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15 February 2005


IR FEL Upgrade<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

Power(kW)<br />

ODU Colloquium<br />

5<br />

4<br />

3<br />

2<br />

1<br />

Power(kW)<br />

Gain<br />

0<br />

0<br />

0.2 0.3 0.4 0.5 0.6 0.7<br />

Wavelength(µm)<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

5<br />

4<br />

3<br />

2<br />

1<br />

15 February 2005<br />

Gain


IR FEL 10 kW Upgrade Parameters<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

Parameter Design Value<br />

Kinetic Energy<br />

Average g Current<br />

Bunch Charge<br />

Bunch Length<br />

Transverse Emittance<br />

Longitudinal Emittance<br />

Repetition Rate<br />

ODU Colloquium<br />

160 MeV<br />

10 mA<br />

135 pC<br />


ERL Phase II X-ray X ray SR Source Conceptual Layout<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

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CHESS / LEPP<br />

15 February 2005


ERL Phase II Sample Parameters<br />

CHESS / LEPP<br />

Parameter Value Unit<br />

Beam Energy 5-7 GeV<br />

Average Current 100 / 10 mA<br />

Fundamental frequency 1.3 GHz<br />

Charge per bunch 77 / 8 pC<br />

Injection Energy 10 MeV<br />

NNormalized li d emittance i 2 / 02* 0.2* µm<br />

Energy spread 0.02-0.3 * %<br />

BBunch h llength th iin ID IDs 012* 0.1-2* ps<br />

Total radiated power 400 kW<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

* rms values<br />

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15 February 2005


Brilliance Scaling and Optimization<br />

. For 8 keV photons, 25 m undulator, and 1 micron normalized emittance, X-ray<br />

source brilliance<br />

B<br />

I<br />

2<br />

ε<br />

∝ = 2<br />

ε th<br />

fQ<br />

+ AQ<br />

. For any power law dependence on charge-per-bunch, Q, the optimum is<br />

p<br />

AQ th<br />

2<br />

≈ ε / p<br />

p<br />

( −1)<br />

. If the “space charge” generated emittance exceeds the thermal emittance εth<br />

from whatever source, you’ve already lost the game!<br />

. BEST BRILLIANCE AT LOW CHARGES, , once a given g design g and bunch<br />

length is chosen!<br />

. Unfortunately, best flux at high charge<br />

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)<br />

2<br />

/mr 2<br />

(ph/s/0.1%/mm 2<br />

Average<br />

Brilliance (<br />

10 23<br />

10 22<br />

10 21<br />

10 19<br />

ERL X-ray X ray Source Average Brilliance and Flux<br />

ERL 25 25m 00.015nm 015 10 10m A<br />

0.15nm 100mA<br />

LCLS SASE<br />

Sp8 25m<br />

APS 4.8m<br />

Sp8 5m<br />

20 ESRF U35<br />

10<br />

10 18<br />

10 17<br />

10 16<br />

10 15<br />

10 14<br />

13<br />

10 13<br />

APS 2.4m<br />

LCLS spont.<br />

CHESS 24p wiggler<br />

CHESS 49p wiggler<br />

10 100<br />

Photon Energy (keV)<br />

Avverage<br />

Flux (phhotons/s/0.1%)<br />

10 16<br />

10 15<br />

10<br />

10 14<br />

ESRF U35<br />

Sp8 25m<br />

ERL 25m<br />

0.015nm 10mA<br />

APS 2.4m<br />

LCLS SASE<br />

APS 44.8m 8m<br />

CHESS / LEPP LEPP<br />

ERL 25m 0.15nm 100mA<br />

Sp8 5m<br />

3 4 5 6 7 8 910 20 30 40 50<br />

Photon Energy (keV)<br />

Courtesy: y Qun Shen, CHESS Technical Memo 01-002, Cornell Universityy<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

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15 February 2005


)<br />

0.1%/mm 2<br />

/mr 2<br />

Peak Brilliance B (ph/s/0<br />

10 27<br />

10<br />

10 26<br />

10 25<br />

ERL Peak Brilliance and Ultra Ultra-Short Short Pulses<br />

0.15nm 100mA 4.7ps<br />

ERL 25m 0.015nm<br />

10mA 0.3ps<br />

0.15nm<br />

24<br />

10<br />

100mA 0 3ps<br />

24 100mA 0.3ps<br />

10 23<br />

10 22<br />

Sp8 25m<br />

ESRF U35<br />

Sp8 5m<br />

10 21 APS 2.4m<br />

10 20<br />

10 19<br />

10 18<br />

10 17<br />

10 16<br />

10<br />

10 15<br />

CHESS 49-pole G/A-wiggler<br />

τ=153ps, f=17.6MHz (9x5)<br />

CHESS 24-pole F-wiggler<br />

10 100<br />

Photon Energy (keV)<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

)<br />

mm 2<br />

/mr 2<br />

Peak Brilliaance<br />

@ 8 keVV<br />

(ph/s/0.1%/m<br />

10 27<br />

10<br />

10 26<br />

10 25<br />

10 24<br />

10 23<br />

10 22<br />

10 21<br />

10 20<br />

10 19<br />

10<br />

10 18<br />

10 17<br />

10 16<br />

ODU Colloquium<br />

3rd SR<br />

APS upg<br />

Sp8-25m<br />

ESRF<br />

APS<br />

2nd SR<br />

CHESS<br />

49p<br />

24p<br />

CHESS / LEPP<br />

ERL<br />

0.015nm 0.01A<br />

0.15nm 0.1A<br />

0.15nm 0.1A<br />

4.7ps p<br />

1.5nm 0.1A<br />

ALS fs BLs<br />

ALS sect.6<br />

undulator<br />

ALS 5.3.1<br />

1000 100 10 1 0.1<br />

X-ray Pulse Duration τ (ps)<br />

Courtesy: Q. Shen, I. Bazarov<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

15 February 2005


Phase I ERL<br />

Beam Energy 100 MeV<br />

Injection Energy 5 MeV<br />

Beam current 100 mA<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

CHESS / LEPP<br />

Charge per bunch 77 pC<br />

Emittance, norm. 2* µm<br />

Sh Shortest t t bunch b h length l th 100* fs f<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

* rms values<br />

15 February 2005


Superconducting RF Technology<br />

99-cell ll 11.3 3 GH GHz cavity it<br />

Superconducting RF cavities (Q ~ 10 10 @ 20 MV/m)<br />

Thomas <strong>Jefferson</strong> National Accelerator Facility<br />

ODU Colloquium<br />

Operated by the Southeastern Universities Research Association for the U. S. Department of Energy<br />

CHESS / LEPP<br />

15 February 2005

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