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Special Topic: Laser Acceleration Eric R. Colby Advanced Accelerator Research Department, SLAC Given at the 2009 Winter USPAS

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Page 1: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Special Topic:

Laser Acceleration

Eric R. Colby

Advanced Accelerator Research Department, SLAC

Given at the 2009 Winter USPAS

Page 2: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Outline

•The Lawson-Woodward theorem

•One route to understanding the Lawson-Woodward theorem

•Far-field antenna radiation pattern synthesis

•Lawson’s argument for why open accelerator structures won’t work

•The reciprocity theorems

•Application to an Example

•Linear Accelerator Examples: a0<<1

•“Non-linear” accelerator examples: a0>1

Page 3: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Lawson-Woodward Theorem

Colloquial version: A nonvanishing synchronous longitudinal field component can only occur in vacuum

for TEM modes in the near field.

Colloquial Version, Narrowly Applied to Accelerators: Boundaries must be present for net energy

exchange to occur in first order for v c beams traveling straight trajectories in vacuum.

Original version: J. D. Lawson, P. M. Woodward: EM fields in the neighborhood of a boundary (cf.

aperture) may be represented by a combination of propagating and evanescent plane waves. Furthermore,

the far field pattern is simply the Fourier transform of the aperture distribution. Propagating plane waves

have vph≥c and strictly transverse polarization, hence no accelerating field. Evanescent plane waves have

E‖/E⊥∝1/g0 as g∞, hence have decreasing accelerating field with increasing particle energy.

Schemes which do not violate Lawson-Woodward:

•IFEL (particles do not travel in straight lines) *Inverse Smith-Purcell (boundary within lg)

•Ponderomotive Acceleration (Second-order process) *Inverse Cerenkov (gas present to slow vph)

•Non-linear Compton Scattering (Multi-order process)

•LEAP (finite interaction length)

Page 4: Special Topic: Laser Acceleration - USPAS | U.S. Particle

One Route to L-W

1. Derive an eigenfunction expansion suitable for expressing EM fields above an

arbitrary boundary (first handled in the context of antenna design)

2. Identify general characteristics of the eigenfunctions

1. Do they represent propagating or bound modes?

2. Is there a non-vanishing field component in the direction of propagation?

3. Is it synchronous?

3. Based on these general characteristics, deduce what situations cannot lead to

particle acceleration for vc particles.

Page 5: Special Topic: Laser Acceleration - USPAS | U.S. Particle

One Route to L-W

The far-field antenna pattern synthesis problem:

Q: For a given far-field power distribution P(q), what configuration of aperture

currents is required to produce it?

Aperture (22.5 m DIA)

Pave Paws Phased-Array Radar

Installation, Beale AFB (1792 dipoles,

340 W/dipole, 2.2o main lobe width)

50l aperture

l~45 cm (~650 MHz)

Page 6: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Woodward’s PrescriptionP. M. Woodward, “A Method of Calculating the Field over a Plane Aperture Required to

Produce a Given Polar Diagram”, J.I.E.E., 93 (IIIA), 1554, (1947).

One can approximately synthesize any desired

infinite far-field pattern by vectorially adding

the patterns from the 2n+1 linearly independent

(Fourier) harmonics of the radiation aperture.

Furthermore, one can synthesize any radiation

pattern in the finite far-field to still greater

precision by adding evanescent solutions.

+c.c. (omitted for clarity)

5l

5l

log|S| far-field

n=5

Page 7: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Propagating vs. Evanescent

k=0 q=0o

k=p/l q=+30o

k=2p/l q=+90o

Propagating (pure vacuum mode)

Evanescent (REQUIRES nearby charges)

k=3p/l q=0o

k=4p/l q=0o

k=5p/l q=0o

Source spacing: l/p2

log|S| far-field Real(Ex(x)) log|S| far-field

Page 8: Special Topic: Laser Acceleration - USPAS | U.S. Particle

What’s the Connection?

q

l

p

sin

~

)2exp()()~,0(0

=

= y

y

djpyHZ y

Note: |sin q|≤1 propagating plane-waves

|sin q|>1 evanescent waves

y

x

z

-

Page 9: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Rayleigh-Helmholtz Reciprocity Theorem

(one of many)

Colloquial version: Mutual inductance is reciprocal when no nonlinear media are present. (paraphrase

of J. D. Kraus, Antennas, 2nd Ed., McGraw-Hill, New York, p.410-11, (1950), with nonlinear media clause coming from J. R. Carson,

“Reciprocal Theorems in Radio Communication”, Proc. IRE, 17(6), p.952ff, (1929).)

Colloquial Version, Narrowly Applied to Accelerators: If a structure accelerates beam, it will make

the beam radiate, and the narrowband coupling impedance for each process will be the same.

Rigorous, general version: Given imposed quasistationary drive fields Eo’ and Eo

’’ on two objects

and a bounding surface S containing both objects within volume V, and e,m, and s are all scalar and

constant: (from S. Ballantine, Proc. IRE, 17(6), p.929ff, (1929).)

Original version: “Let there be two circuits of insulated wire A and B and in their neighborhood any

combination of wire circuits or solid conductors in communication with condensers. A periodic

electromotive force in the circuit A will give rise to the same current in B as would be excited in A if

the electromotive force operated in B.” Lord J. W. S. Rayleigh, Theory of Sound, v. II, Dover: New York, p. 145, (1894).

HC

dSn

HEHEcdvCo

ECo

E

c

=

p

p

4

]''''''[4

]''''''[

Page 10: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Many Variants…

0)'''''')(4/(

0)''''''(

0)''''''(

0''''''''''''

)'''()'''(4

''''''

))(4/(

0]''''''[4

]''''''[

4

=

=

=

==

=

=

==

dvEo

EEo

Ei

dvo

JEo

JE

dvJo

EJo

E

Co

ECo

ECECE

HEHEc

Co

ECo

E

oEEiHC

dSn

HEHEcdvCo

ECo

E

c

pes

p

pes

p

p

No radiation from beyond surface S

Most general local form

Impressed fields, no impressed

charges, Ballantine form

Impressed currents, no impressed

fields

No other radiation beyond surface S

pesl

e

m

m

pl

4/

0

0

/

4

i

E

H

cHiE

EHE co

=

=

=

=

=

Page 11: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Specific Example:

Crossed-Gaussian Accelerator

Page 12: Special Topic: Laser Acceleration - USPAS | U.S. Particle

z

Interferometric Acceleration

The laser beams are polarized in the XZ plane, and are out of phase by p

Terminating

BoundaryTerminating

Boundary

E1

E2

E1z

E2z

E1x

E2

x

x

E1x + E2x = 0

|E1z + E2z| > 0

no transverse deflection

nonzero electric field in the

direction of propagation

Interaction Length : ~1000 l ~0.1 ZR

Slit

Width

~10 l

Slit

Width

~10 l

Electron beam

Waist size:

wo~100 l

Crossing

angle: q

Page 13: Special Topic: Laser Acceleration - USPAS | U.S. Particle

))cos()(sin(exp

)cos(exp

1

21

21

21

101

21

21

1

01

2

1

1

tZ

z

tw

r

kw

xE

z

tw

r

w

wE

x

R

o

E

E

=

=

Ez1

Ex1E1

oRRt ZzwZrztkz f = )/(tan)/( 1

12

1

2

111

P. Sprangle, E. Esarey, J. Krall, A. Ting, Opt. Comm., 124, p.69ff, (1996).

Z1 Z2

(paraxial approximation to first order in 1/wok ~ 10-3)

Page 14: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Crossed Gaussian Illumination

Entrance slit

q q

Electron Beam

Real(Ex) log(S) far-field

Page 15: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Analytic Field Calculations: Paraxial

Approximation vs. Physical Optics

Analytic theory (Sprangle/Esarey/Krall 1996) ,

numerical integration of crossed TEM00 modes,

and a brute-force vector diffraction calculation

of fields

Page 16: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Accelerator vs. RadiatorReal(Ex) Real(Er)

Crossed-Beam Accelerator CTR Radiator, viewed narrowband

Crossed Gaussian beams, w0=64m, 10m x 10m x l/30 bunch, 104 particles

q=11.5 mr

EkYH

c

RK

c

zj

c

ejE

c

RK

c

zj

R

yx

c

eE

iiN

i o

z

iiN

i i

ii

o

yx

=

=

=

=

=

=

ˆ

)()exp(2

4

)()exp(2},{

4

0

10

1222

1

10

122},{

4

4

g

pgpe

g

pgpe

Far-field CTR

From Slit

Abs(Ex)

Page 17: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Sprangle-Esarey-Krall vs.

Inverse Transition Radiation:

Near-Field

LEAP

CTR at

800nm

Er

ExEx

Page 18: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Inverse Transition Radiation:

Far-Field

Er

Ex

Propagate

12,500 l

1 cm=6.4 zR

Page 19: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Vector Diffraction CodeA Matlab implementation of Huygen’s Principle in l.i.h. media

1ˆ1

4)(

22ˆˆ111ˆˆ1

4)(

1ˆ1

4)(

22ˆˆ111ˆˆ1

4)(

2222

2222

=

=

=

=

RjkRR

eRG

kRj

RkRR

kRj

RkRR

R

eYjkRG

RjkRR

eRG

kRj

RkRR

kRj

RkRR

R

ejkZRG

jkR

EM

jkR

oHM

jkR

EM

jkR

EJ

p

p

p

p

=2

2

2

)'()')('()')('(

)')('()'()')('(

)')('()')('()'(1ˆˆ

zzyyzzxxzz

zzyyyyxxyy

zzxxyyxxxx

RRR

|Ey|

3. Propagate to field points

1. Construct or load incident fields

L. Diaz, T. Milligan, Antenna Engineering Using Physical Optics, Artech House, London, (1996).

EnnYJ

HnnZM

eq

eq

=

=

ˆˆ

ˆˆ

1=

=

ZY

Ze

m

Source

Patch

Array

Field

Patch

Array

|Ey| arg(Ey)

2. From incident fields, calculate

surface currents on initial, discrete

surface

=

=

')'()(')'()()(

')'()(')'()()(

dSrJRGdSrMRGrH

dSrMRGdSrJRGrE

HJHM

EMEJ

Page 20: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Fundamental Physics Considerations I

• Lawson-Woodward Theorem requires that one or more of:

– Boundaries*

– Gases

– Periodic transverse motion of accelerated particles

be present for linear acceleration (∝E ) to take place

• *Furthermore, since free-space modes are strictly TEM, efficient acceleration requires a structure that either strongly diffracts the TEM mode, or guides a TM-like mode boundaries must be very close to the beam (r/gl<1)

• Accelerating fields must not degrade transverse emittances fields must be rotationally symmetric

Page 21: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Fundamental Physics Considerations II

• Good coupling impedance strong fundamental-mode wakefield

• Stability against regenerative beam breakup minimal higher order mode wakefields

• Higher stored energy (Q) in structure Tighter dimensional tolerances

• Larger acceptance larger aperture

Page 22: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Basic Technical Considerations I• For efficiency, accelerators should be designed at

wavelengths to use the most efficient lasers

– Yb:KGd(WO4)2, Yb:KY(WO4)2 l ~ 1.0 mm

– Erbium Fiber l ~ 1.5 mm

– Cr++:ZnSe l ~ 2.2-2.8 mm

• For economy of fabrication, accelerators should be designed at wavelengths were materials are low loss and amenable to lithographic or fiber drawing processes:

– a-SiO2 l ~ 0.2-2.5 mm

– c-Si l > 1.5 mm

Page 23: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Basic Technical Considerations II

• Structure materials should have

– High damage threshold resistance to breakdown

– High radiation resistance resistance to high-radiation accelerator environment

– Excellent optical linearity, even under large applied electric fields minimal intensity-dependent dephasing

– Good thermal conductivity, low thermal expansion thermally stable under changing operating conditions

– Amenability to fabrication Lithography or fiber drawing

Page 24: Special Topic: Laser Acceleration - USPAS | U.S. Particle

T. Plettner, “Proof-of-Principle Experiment for Crossed Laser beam Electron Acceleration in a

Dielectric Loaded Vacuum Structure”, Ph.D. Thesis, Stanford Univ., 2002.

Short-Pulse Laser Damage of Dielectrics

•t1/2 dependence for t>10 ps

•No t dependence for t<5 ps

•“Laser Conditioning” raises threshold ~10%

•Some materials perform worse under vacuum

SiO2SiO + O

1.7 GV/m

1.2 GV/m

Fields for

st=1 ps

Page 25: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Examples of

Laser Accelerators

Page 26: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Second Example:

Photonic Band Gap Structures

X. (Eddie) Lin, “Photonic Band Gap Fiber Accelerator”, Phys. Rev. ST-AB, 4, 051301, (2001).

•Can be designed to support a single, confined, synchronous mode

•All other modes at all other frequencies radiate strongly

DIA=1.4l

Zc=19.5W

g=0.581.305l

er=2.13

(Silica)

P

EZc

2

22

acc l=

Page 27: Special Topic: Laser Acceleration - USPAS | U.S. Particle

2D Photonic Band Gap Structures

Ben Cowan, ARDB, SLAC

guide

pad

e-beam

a=0.36l

0

0.2

0.4

0.6

0.8

1

TE Band Structure of Crystal

a/2

pc

Position around Brillouin Zone Edge

2D TE Band Gap

er=12.1

(Silicon)

w=1.08ld=0.09

This geometry is designed for the

lithographic process.

Page 28: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Impedance and Gradient Optimization

Ben Cowan, ARDB, SLAC

1 1.2 1.4 1.6 1.8 2 2.2 2.4 2.60

50

100

150

200

250

300

w/l

Zc [

W]

PC Waveguide Shunt Impedance for SOL Modes

55.3

~

l

wZc

0 0.05 0.1 0.15 0.2 0.250.03

0.04

0.05

0.06

0.07

0.08

0.09

d/a

Ezm

ax /E

p

Maximum Accelerating Gradient for 25 mm Segment

w = 3.0aw = 4.0aw = 5.0aw = 6.0a

0 0.05 0.1 0.15 0.2 0.250.1

0.15

0.2

0.25

0.3

0.35

0.4

0.45

d /a

f D

Damage Factor vs. Pad and Guide Widths

w = 3.0aw = 4.0aw = 5.0aw = 6.0a

Eaccel/Epeak

d/a

d/a

Assuming 1ps laser pulse

w/a

Page 29: Special Topic: Laser Acceleration - USPAS | U.S. Particle

2D Fiber Structures

Mehdi Javanmard, ARDB, SLAC This geometry is designed for the fiber

drawing process.

-1 -0.8 -0.6 -0.4 -0.2 0-60

-50

-40

-30

-20

-10

0

log10

(r/R)

Azi

mut

hal m

ode

ampl

itude

(dB

)

R = 0.52a

m = 0m = 1m = 2m = 3m = 4m = 6m = 12

-1 -0.8 -0.6 -0.4 -0.2 0-60

-50

-40

-30

-20

-10

0

log10

(r/R)

R = 1.34a

m = 0m = 1m = 2m = 5m = 6m = 12

-1 -0.8 -0.6 -0.4 -0.2 0-60

-50

-40

-30

-20

-10

0

log10

(r/R)

R = 2.1a

m = 0m = 2m = 4m = 6m = 11m = 12

Zc=1.5WZc=22W Zc=5W

Log10(r/R) Log10(r/R) Log10(r/R)

Azi

mu

thal

Mod

e A

mp

litu

de

[dB

]

Azi

mu

thal

Mo

de

Am

pli

tud

e [d

B]

Azi

mu

thal

Mod

e A

mp

litu

de

[dB

]

Page 30: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Fabricated Examples

P. Russell, “Holey fiber concept spawns optical-

fiber rennaissance”, Laser Focus World, Sept.

2002, p. 77-82.

a b

c d

PCF structures vary according to application: (a) highly nonlinear

fiber; (b) endlessly single-mode fiber; (c) polarization maintaining

fiber; (d) high NA fiber. From René Engel Kristiansen (Crystal

Fibre A/S), “Guiding Light with Holey Fibers,” OE Magazine June

2002, p. 25.

Page 31: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Hollow Fiber Bragg Accelerator

Rint

Rn

en

Rn

n

2

n

2

Rn

n

2

n

2

# Concentric layers (e1,e2)

# Each layer

# vph = c

/ 4 1l e

int 00.3R l=

int 00.8R l=Levi Schächter, The Technion

Page 32: Special Topic: Laser Acceleration - USPAS | U.S. Particle

STELLA (Staged Electron Laser Acceleration) experiment at the BNL ATF(STI Optronics/Brookhaven/Stanford/U. Washington)

CO2 laser beam

ELECTRONSPECTROMETER

IFELACCELERATOR

IFEL

BUNCHER

46 MeV 0.5 nC

2 mm mrad 3.5 ps

0.6 GW, 180 ps

Steeringcoil

BPM

BPM

BPM

BPM

Focusing

quadrupoles

Steering

coil

Focusing

quadrupoles

W. Kimura, I. Ben-Zvi, in proc. of Adv. Accel. Conc. Conf., Santa Fe, NM, 2000.

The Inverse Free Electron Laser

Energy

Energy

EnergyIncoming BeamOptically Modulated

Beam

Optically

Accelerated Beam

Page 33: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Multicell Linear Acceleration Experiments

Inverse Cerenkov Acceleration in Waveguide

(Unfolded Fabry-Perot Interferometer)

A. Melissinos, R. Tikhoplav (U. Rochester, Fermilab)

TEM01* mode

l=1.0 mm (Nd:YAG)

0.2

ATM

He

Status: Structure has been fabricated with 80% power

transmission measured. Nd:YAG drive laser is under

construction at Fermilab now.Y-C. Huang, et al, Nat’l Tsinghua University.

Images from ATF User’s Meeting, January 31, 2002.

Expected gain: 250 keV over 24cm.

ZnSe

Lenses

Multiple ITR AcceleratorsY.-C. Huang, NTHU, Taiwan

(at Brookhaven)

Page 34: Special Topic: Laser Acceleration - USPAS | U.S. Particle

crossed

laser beams

electron

beam

Fused silica prisms

and flats

High Reflectance

Dielectric coated

surfaces

Accelerator cell

slit

Computed Field Intensity, |Et|2

The LEAP Accelerator Cell

~1 cm

Stanford University (Appl Phys. & HEPL) / SLAC

“Laser Electron Acceleration Project”

Page 35: Special Topic: Laser Acceleration - USPAS | U.S. Particle

The LEAP Accelerator Cell

Electron Beam

1 cm

Page 36: Special Topic: Laser Acceleration - USPAS | U.S. Particle

High Field Coupling Mechanisms

ao>1

No near-field structure required, but

beam deflection often plays a vital role

Page 37: Special Topic: Laser Acceleration - USPAS | U.S. Particle

High Field Acceleration MechanismsCombined Ponderomotive and Nonlinear

Compton Scattering

P. X. Wang, Y. K. Ho, et al, J. Appl.

Phys. 91 (2) p. 856, (2002).

Ponderomotive Acceleration

(CEA-Lemeil-Valenton)

G. Malka, E. Lefebvre, J. Miquel, Phys.

Rev. Lett. 78, 3314 (1997).

a=3, q=39o

a=3, q=46o

a=2, q=46o

ao~300

Page 38: Special Topic: Laser Acceleration - USPAS | U.S. Particle

High Field Acceleration Mechanisms

G. Stupakov, M. Zolotorev, Phys Rev Lett 86 5274

(2001).

Ponderomotive Scattering with

Deflection field to aid beam extraction

Y. Salamin, C. Keitel, Phys Rev Lett 88

095005 (2002).

Ponderomotive Acceleration and Focussing

a0~5

Bs

ao~68

Page 39: Special Topic: Laser Acceleration - USPAS | U.S. Particle

The High Peak Power T3 Laser

100 TW (1.9J) at JAERI Kansai.

Upgrading to 1 PW system.

(ao~1030)

National Ignition Facility (LLNL)

Nd:glass 600 TW (1.8 MJ)Laser MegaJoule (CEA-Limeil)

Nd:glass 600 TW (1.8 MJ)

Lasers at 1 PW and beyond

Under Construction

1 shot/8 hours!

The Vulcan 100 TW (2600 J)

Nd:glass system at RAL.

Upgrading to 1 PW system.

(ao~1030)

(ao~241300 [0.1 ps])(ao~241300 [0.1 ps])

The GEKKO XII 1 PW (400 J)

Nd:glass system at ILE Osaka.

(ao~30)

Page 40: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Key Issues for Low Field Acceleration

•What improvement in material damage threshold is possible?

•Are there better materials?

•Do improved surface smoothness or material purity help?

•What coupling impedance is possible?

•What structure geometries can be fabricated?

•What geometric accuracy is possible?

•What electrical efficiency is possible?

•Can alignment and vibration tolerances be met?

Page 41: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Key Issues for High Field Acceleration

• Can better laser media be manufactured?

•Broad(er) bandwidth

•Higher damage and saturation fluences

•Better thermal conductivity

•Amenable to diode-pumping

• How small a focal spot is possible?

•What surface accuracy is possible for very large optics?

•What beam quality is possible for what charge?

Page 42: Special Topic: Laser Acceleration - USPAS | U.S. Particle

Final Thought

“One of the authors (W.W.H.), in his study of cavity resonators, was

motivated by a desire to find a cheap method of obtaining high

energy electrons. This cavity acceleration work was put aside, largely

because of the change in standard of success caused by the advent of

Kerst’s betatron. . .

. . .By the end of the war many people

were interested [in linear acceleration], possible reasons being: (a)

wide-spread knowledge of cavity properties and technique, (b) the

enormous pulsed powers made available by radar developments.”

- E. L. Ginzton, W. W. Hansen, W. R. Kennedy, “A Linear Electron Accelerator”, Rev. Sci.

Inst., 19(2), p. 89, February 1948.