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1 International Max Planck Research School on Advanced Photonics Lectures on Relativistic Laser Plasma Interaction J. Meyer-ter-Vehn, Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007 1. Lecture: Overview, Electron in strong laser field, 2. Lecture: Basic plasma equations, self- focusing, direct laser acceleration 3. Lecture: Laser Wake Field Acceleration (LWFA) 4. Lecture: Bubble acceleration 5. Lecture: High harmonics and attosecond pulses from
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J. Meyer-ter-Vehn, Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

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International Max Planck Research School on Advanced Photonics Lectures on Relativistic Laser Plasma Interaction. J. Meyer-ter-Vehn, Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007. Lecture: Overview, Electron in strong laser field, - PowerPoint PPT Presentation
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Page 1: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

1

International Max Planck Research School on Advanced Photonics

Lectures onRelativistic Laser Plasma Interaction

J. Meyer-ter-Vehn, Max-Planck-Institute for Quantum Optics, Garching, Germany

April 16 – 21, 2007

1. Lecture: Overview, Electron in strong laser field,

2. Lecture: Basic plasma equations, self-focusing, direct laser acceleration

3. Lecture: Laser Wake Field Acceleration (LWFA)

4. Lecture: Bubble acceleration

5. Lecture: High harmonics and attosecond pulses from relativistic mirrors

Page 2: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

2

Relativistic Laser Electron Interaction and Particle Acceleration

J. Meyer-ter-Vehn, MPQ Garching

a = eA/mc2

1025

1015

1020

200019851960

1018

I (W/cm2)

2015

GeV electrons

GeV protons

CPA

a = 1

non-relativistic: a < 1

laserelectron

a > 1relativistic:

beam generation

Page 3: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

3

Relativistic plasma channels and electron beams at MPQ

C. Gahn et al. Phys. Rev. Lett. 83, 4772 (1999)

gas jet laser

6×1019W/cm2

observed channel

electron spectrum plasma 1- 4 × 1020 cm-3

Page 4: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

4

Laser-induced nuclear and particle physics

107 positrons/shot

Page 5: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

5

Neutrons From Deuterium Targets

Page 6: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

6

GraphikIOQ Jena

2004Ewald

Schwörer

Page 7: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

7

Relativistic protons: 5 GeV at 1023 W/cm2

D. Habs, G. Pretzler, A. Pukhov, J. Meyer-ter-Vehn, Prog. Part. Nucl. Physics 46, 375 (2001)

Experiments:Multi-10 MeV

ion beams from thin foils

observed

1 kJ , 15 fs laser pulsefocussed on 10 m spot

of 1022/cm3 plasma

Simulations:

Page 8: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

8

Inertial Confinement Fusion (ICF)

J. Meyer-ter-VehnMax-Planck-Institute for Quantum Optics,

Garching

IPP Summer University, Garching 2006

few mmimploded core

100 m

few mg DT

Page 9: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

9

D2 burn fast-ignited from DT seedAtzeni, Ciampi, Nucl. Fus. 37, 1665 (1997)

bulk fuel

DT seed (0.1 mg T)

beam heated region

20 mg D2

15 ps

25 ps

55 ps

35 ps

5 ps

45 ps

1000 g/cc

5 kJ

yield 1.3 GJ

D2 burn produces more tritium than in seed:

breeding ratio: 1.37

Simulation

Page 10: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

10

Nature Physics 2, 456 (2006)

L=3.3 cm, =312 mLaser

1.5 J, 38 TW, 40 fs, a = 1.5

Plasma filled capillary

Density: 4x1018/cm3

Divergence(rms): 2.0 mradEnergy spread (rms): 2.5%Charge: > 30.0 pC

1 GeV electrons

Page 11: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

11

Design considerations for table-top, laser-based VUV and X-ray free electron lasers

F. Grüner, S. Becker, U. Schramm, T. Eichner, M. Fuchs, R. Weingartner, D. Habs, J. Meyer-ter-Vehn, M. Geissler, M. Ferrario, L. Serafini,

B. van der Geer, H. Backe, W. Lauth, S. Reiche

http://arxiv.org/abs/physics/0612125 (Dec 2006)See also from DESY: Arxiv:physics/0612077 (8 Dec 2006)

Page 12: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

12

-5/2

B. Dromey, M. Zepf et al., Nature Physics 2, 698 (2006)

Observation of high harmonics from plasma surfacesacting as relativistic mirrors

Page 13: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

13

Plane Laser Wave

0/ Re{( / ) }iE A c t i c A e

0Re{ }iB A ik A e

4( / )S c E B

2

08( / )AI kS for LP

for CP

2 , ,

(1 cos )

2 , .

2 2

0 0

22

08 2

A Ak

I c

for lin. (circ.) polarization1 (2)

00 yAA e

00 ( )y zAA e ie

lin. pol. (LP): circ. pol. (CP):

( )0( , ) Re{ }i k r tA r t A e

k r t

/ 2 /k c

Page 14: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

14

Relativistic Intensity Threshold

/ ( / )m dv dt e E v c B eE

02

ReeAv eE

c imc mc

forcos

cos

LP

fs or CPin

y

y z

e

e e

20 0 0valid for , relativistic regim< e< : 1 1a eA mc a

(non-relativistic v/c << 1)

2 2 18 2 20 0 0 022

W 1.37 10 μm

cmI P a a

2 3

0 511 kV 17 kA = 8.67 GWmc mc

Pe e

Average intensity:

Power unit:

Page 15: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

15

1. Problem: Normalized light amplitude a0 = eA0/mc2

Show that the time averaged light intensity I0 is related to the normalized lightamplitude a0 by

where l is the wavelength, equals 1 (2) for linear (circular) polarization,and P0 is the natural power unit

2 3

0 511 kV 17 kA = 8.67 GWmc mc

Pe e

2 2 18 2 20 0 0 022

W 1.37 10 μm

cmI P a a

Confirm that the laser fields are

12L 03 10 V/m E a

8L 010 gauss B a

Use that, in cgs units, the elementary charge is e = 4.8 1010 statC and 1 gauss = 1 statC/cm2.

Page 16: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

16

Special relativity

Relativistic Lagrange function:

L = - mc2 v2/c2)1/2 - q + (q/c) v•A

Galilei:

t´= t x´= x - vt

Lorentz:

t´= (t - vx/c2) x´= x - vt )

v2/c2) -1/2

mechanics electrodynamics

Einstein (1905): Also laws of mechanicshave to follow Lorentz invariance

A = Ld

L = L = -mc2 - (q/c) pA

Page 17: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

17

2. Problem: Relativistic equation of motion

The Lagrange function of a relativistic electron is (c velocity of light, e and m electron charge and rest mass, f and A electric and magnetic potential)

Use Euler-Lagrange equation

to derive equation of motion

with electric field , magnetic field , and

electron momentum

2 2 2( , , ) 1 /e

L r v t mc v c v A ec

0d L L

dt v r

( / )/ e cdp dt eE v B

/E A c t

B A

2, / , and 1/ 1 .p mc v c

Page 18: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

18

Symmetries and Invariants for planar propagating wave

symmetry: invariant: ( / ) const , / 0 / e cL r L v p A

symmetry:

invariant: const

,

( ) / /

/ /

E

x

x

L x ct dH dt L t c L x c dp dt

p c

2 2 2 ( / )( , ) 1 / ( ) e cL v x ct mc v c v A x ct

1/

0d L L

dt v r

( /c)/ eL v m v A p

Relativistic Electron Lagrangian

2 2 2 2kin 2E ( 1) /2 /xmc p c p m mc a

For electron initially at rest:

(relativistically exact !)

Page 19: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

19

Relativistic side calculation

2 2 2 2

2 2

2 2 2

2

2

( )( ) ( )

( )

( ) ( )2

x

x

x

x

E mc p c

mc

p c

mc

p c

m ccc pp

2 /2xp c p m

Page 20: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

20

Relativistic electrons from laser focus observedC,L.Moore, J.P.Knauer, D.D.Meyerhofer, Phys. Rev. Lett. 74, 2439 (1995)

2 2kinE ( 1) /2xmc p c p m

2

2 kin2

kin

2 E 2tan

1/x

p m

p E c

p

xp

>>1 electrons emergein laser direction

(follows from L(x-ct) symmetry)

Page 21: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

21

Relativistic equations of motion

ˆ / 0, , y zp p mc a a a

2 2 2kin kin

ˆ ˆ ˆE E / 1 /2 /2xmc p p a

2( ) /a eA mc

( ) ( )/t t x t c

2 211 1

2 2

d d d dx d a a d d

dt dt d c dt d d d

ˆ ( )y y y

dyp a

c dt

2ˆ ( ) / 2x x

dxp a

c dt

ˆ ( )z z z

dzp a

c dt

( )y

dyca

d

( )z

dzca

d

2 ( )/2dx

c ad

Page 22: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

22

Relativistic electron trajectories: linear polarization

0 cosdy

cad

0( ) ( / )siny t ca

220 cos

2

cadx

d

2

0 12

4 2( ) sin

cax t

20a

0a

Figure-8 motion in drifting frame (=kc)

20

0

2( ) ( /8)sin

sinD

ky a

k x x a

x

Page 23: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

23

Relativistic electron trajectories: circular polarization

)0 0 0ˆ ˆ( ) Re{ ( ) } ( 0, cos , sin )i

y za a e ie e a a

2 2 2 20 const( ) + y za a a a 2

0 const1 /2 a

20( ) ( /2 ) x t a ct

2

0

2

0

/2

1 /2( )/ 1 /

a

at x t c t t

20ˆ /2x x

dxp a

c dt

0 ( / )sin tdz

ac dt

0 ( / )cos tdy

ac dt

0 ( / )( ) ( / )sin ty t ca

0 ( / )( ) ( / ) cos tz t ca

x

Page 24: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

24

0Re ( ) ( , , ) exp( )y za e ie a r z t ikz i t

2 20 0 0 0 0( , , ) , / / a a r z t a t a a z ka

22

022

2

10 2 ( , ) 0ik a

c tra

3. Problem: Derive envelope equation

Consider circularly polarized light beam

Confirm that the squared amplitude depends only on the slowly varyingenvelope function a0(r,z,t), but not on the rapidly oscillating phase function

Derive under these conditions the envelope equation for propagation invacuum (use comoving coordinate=z-ct, neglect second derivatives):

Page 25: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

25

0

1 2 ( , ) 0r ik a r z

r r r z

4. Problem: Verify Gaussian focus solution

Show that the Gaussian envelope ansatz2

0 0 ( , ) exp( ( ) ( )( / ) )a r z P z Q z r r

2 2 2 20

2/[ (1 / )]

0 2 22 20

/ ( , ) exp arctan

1 /1 /

Rr r z LR

R RR

z Le z ra r z i i

L r z Lz L

inserted into the envelope equation

leads to

Where is the Rayleigh length giving the length of the focal region.

2 20 0/ 2 /RL kr r

Page 26: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

26

New physics described in these lectures

At relativistic intensities, I2 > 1018 W/cm2 m2, laser light accelerates electrons to velocity of light in laser direction and generates very bright, collimated beams.

The laser light converts cold target matter (gas jets, solid foils) almost instantaneously into plasma and drives huge currents. The relativisticinteraction leads to selffocused magnetized plasma channels and directlaser acceleration of electrons (DLA).

In underdense plasma, the laser pulse excites wakefields with hugeelectric fields in which electrons are accelerated (LWFA). For ultra-shortpulses (<50 fs), wakefields occur as single bubbles which self-trap electronsand generate ultra-bright mono-energetic MeV-to-GeV electron beams.

At overdense plasma surfaces, the electron fluid acts as a relativistic mirror,generating high laser harmonics in the reflected light. This opens a new route to intense attosecond light pulses.

Page 27: J. Meyer-ter-Vehn,  Max-Planck-Institute for Quantum Optics, Garching, Germany April 16 – 21, 2007

27

ICF target implosion