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Rutherford Appleton Laboratory Three mechanisms interact to cause ion acceleration in PW laser interactions • Relativistic electrons expelled by the ponderomotive pressure of light wave. To overcome the attractive electric field of the ions, E e > E c . The Coloumb energy E c is approximately E c 2 2 ne 2 l s R • Later the ions move due to Coloumb repulsion. E i 4 2 ne 2 R 2 R laser l s •Inductive electric field caused by the rapid change in the B field that accelerates ions and decelerates electrons. The energy gained by this process is E i 8 e 2 n R 2

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laser. R. l s. Three mechanisms interact to cause ion acceleration in PW laser interactions. Rutherford Appleton Laboratory. - PowerPoint PPT Presentation

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Page 1: Rutherford Appleton Laboratory

Rutherford Appleton Laboratory

Three mechanisms interact to cause ion acceleration in PW laser interactions

• Relativistic electrons expelled by the ponderomotive pressure of light wave. To overcome the attractive electric field of the ions, Ee > Ec . The Coloumb energy Ec is approximately

Ec 2 2 ne2lsR

• Later the ions move due to Coloumb repulsion.

Ei 4 2 ne2R2

Rlaser

ls

•Inductive electric field caused by the rapid change in the B field that accelerates ions and decelerates electrons. The energy gained by this process is •

Ei 8 e2n R2

Page 2: Rutherford Appleton Laboratory

Rutherford Appleton Laboratory

Sophisticated 3D simulations performed by Prof. S.Bulanov and co-workers has revealed that for linear polarisation case

the ion energy is px = 0.61mic

Conclusion: at intensities 31021 Wcm-2, ~1012 protons are accelerated with energies of several hundred MeV

3D computer simulations of ion acceleration process

Page 3: Rutherford Appleton Laboratory

Rutherford Appleton Laboratory

0.1

10

1000

105

107

109

1013 1015 1017 1019 1021 1023 1025 1027

Tan et al.CR39 resultsCR39 (Dec.98)Recent CR39 resultsLivermore

Ion

ener

gy (

keV

/nuc

leon

)

I2 Wcm-2µm2

Maximum ion energy vs I

PIC simulationS.V.Bulanov et alJETP Lett 71, 407 (2000)

a02 I2

PIC simulationT.Zh.Esirkepov et alJETP Lett 70, 82 (1999)

a0 I2

Prospects for GeV proton acceleration using PW lasers

Page 4: Rutherford Appleton Laboratory

Rutherford Appleton Laboratory

GeVlacm

cmnE x

e 20318

3

)(10

)(

The energy gain over the interaction length in a plasma wakefield is

When I2 >> 1018 Wcm-2m2, the radiation pressure is so large nearly all electrons are expelled from the photon wave-envelope, generating a “snow-

plough” in which the electron momentum gain is

202

0

20

4

1a

cmn

E

cn

Ep

e

c

ex

cm

eEa

00

00

provided the laser pulse fully interacts with the plasma (i.e. not diffracted)

Accelerating gradients 200 TeV/cm at 1026 Wcm2

Wakefield acceleration

e

cmEc

00

Page 5: Rutherford Appleton Laboratory

Nd:glass

20 fs seed laser stretched to 400 ps

1000ps

527 nm

3400 J

SHG

LBO1.5 cm

KDP3.8 cm

4452 J

41 %

LBO1.4 cm

KDP1.1 cm

KDP 0.8 cm

3400 J3400 J44 % 46 % 0.2 mJ 4 J

00.20.40.60.8

11.21.41.6

-600 -200 200 600

time (ps)

inte

nsi

ty (

a.u

.) signal out

depleted pump

Output signal and pump intensity profiles

100 PW

Intensity profile after compression

-80 -60 -40 -20 0 20 40 60 80

time (fs)

inte

nsi

ty

FWHM = 22 fs

(0.3 J/cm2)

Rutherford Appleton Laboratory

Ideas for EW lasers (Dr I.N.Ross)

Page 6: Rutherford Appleton Laboratory

Rutherford Appleton Laboratory

Future Upgrade OptionsGiven Some Technology DevelopmentGiven Some Technology Development

SHG Pump Dielectric Gratings 1μm Output 50cm KDP

F/1 Focusing0.3 EW 1025 W/cm2

THG Pump Dielectric Gratings0.5μm Output 50cm KDP

F/1 Focusing 0.6 EW 1026 W/cm2

Multi OPCPA >1 EW >1026 W/cm2

Page 7: Rutherford Appleton Laboratory

Rutherford Appleton Laboratory

• The VULCAN PW upgrade is nearly completion - first experiments to university users scheduled November 2002 - laser wakefield accelerator studies

• >100 MeV protons and >1GeV heavy ions expected

• Future upgrades to multi-PW levels are being actively pursued

• The CLF is investigating new designs for average and peak power lasers required for accelerator and fusion applications

Summary