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ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

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Page 1: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

ELI Nuclear Physics WorkshopMagurele

Feb. 1. 2010Gérard Mourou

Page 2: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

ELI Integrated Infrastructure

CZ Prague

HO Szeged

RO Bucarest

Page 3: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou
Page 4: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

The ELI’s Ultimate Scientific Goal:“ Study of the structure of matter from Atom

to Vacuum “

Page 5: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Photonuclear Physics:Photonuclear Physics:Exploring Nuclei with LaserExploring Nuclei with Laser

Page 6: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou
Page 7: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou
Page 8: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Rel

ativ

istic

Ultr

a R

elat

ivis

tic

Rel

ativ

istic

Com

pres

sion

EQ=mpc2

Ultra-relativistic intensity isdefined with respect to the proton EQ=mpc2, intensity~1024W/cm2

NL Optics

QCD ~1035W/cm2

Page 9: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

ELI Cardinal Features

• Ultra High intensity• Relativistic and ultrarelativistic regime• Ultrashort Pulse of high energy radiations and

particles because(Power-Pulse Duration Conjecture)

• Pristine synchronization between beams within a fraction of the period

Page 10: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

• Unique laser properties:

- ultrahigh fields

- ultrashort pulses

• Novel techniques:

- production of brilliant photon beams

Page 11: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Peak Power -Pulse Duration Conjecture

1) To get high peak power you must decrease the pulse duration.

2) To get short pulses you must increase the intensity

Page 12: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Q-Switch, DyeI=kW/cm2

Modelocking, DyeI=MW/cm2

Mode-Locking KLMI=GW/cm2

MPII>1013W/cm2

Laser Pulse Duration vs. Intensity

Relativistic and Ultra R Atto, zepto….?

Page 13: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

RelativisticRelativistic Optics Optics

r F =q

r E +

r v c

∧r B

⎛ ⎝ ⎜

⎞ ⎠ ⎟

⎝ ⎜

⎠ ⎟

a)Classical optics v<<ca)Classical optics v<<c , , b) Relativistic optics v~cb) Relativistic optics v~c

x~ax~aoo

z~az~aoo22

aa00<<1, a<<1, a00>>a>>a002 2 aa00>>1, a>>1, a00<<a<<a0022

a0 =eA0

mc2=

eE0λmc2

Page 14: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Relativistic Rectification(Wake-Field Tajima, Dawson) sE

r+ -

1) pushes the electrons.

2) The charge separation generates an electrostatic longitudinal field. (Tajima and Dawson: Wake Fields or Snow Plough)

3) The electrostatic field

r F Bz

=qr v c

∧r B

⎛ ⎝ ⎜

⎞ ⎠ ⎟

r v ∧

r B

Es=cγmoωp

e= 4πγmoc

2ne

Es≈EL

Page 15: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou
Page 16: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Front and back acceleration mechanisms

Peak energy scales as : EM ~ (IL×)1/2

Page 17: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

C

Vp ~0

Vp ~C

C

Non relativistic ions

Relativistic ions >1024 Photons

Photons

Ep ~ I1/2

Ep ~ I

The Ultra relativistic:Relativistic Ions

Page 18: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

High Energy Radiation

Betatron oscillation X-ray laser

Harmonic generation Thomson/Compton Scattering

Radiation reaction

Page 19: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Attosecond pulse generation by Relativistic Compression

ε =1−ω 2

p

γ 0ω2

where γ 0 = 1+ a0

2

Page 20: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Scalable Isolated Attosecond Pulses

Amplitude, a

1D PIC simulations in boosted frame

Duration,

t (as) 2D: a=3, 200as

tas)=600/a0

I=1022W/cm2 (Hercules)

l=1019W/cm2 (3

laser)

optimal ratio: a0/n0=2, or exponential gradient due to wcr=w0a-1/2

n0= n/ncr

Page 21: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Attosecond Electron Bunches

N. Naumova, I. Sokolov, J. Nees, A. Maksimchuk, V. Yanovsky, and G. Mourou, Attosecond Electron Bunches, Phys. Rev. Lett. 93, 195003 (2004).

Attosecond pulse train

Attosecond bunch train

25÷30 MeV

a0=10, t=15fs, f/1, n0=25ncr

Page 22: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

D. Habs

Page 23: ELI Nuclear Physics Workshop Magurele Feb. 1. 2010 Gérard Mourou

Expectations

• Romania must do its share. It must become the world premier facility in Laser-Based Nuclear Physics.

• Must become a recognized pan-european Infrastructure, with collaboration from the ELI Partners (Cz, Hu, De, Fr, UK, …..) and beyond.