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Full-scale particle simulations of high-energy density science experiments W.B.Mori , W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou, V.K.Decyk, C. Joshi (UCLA) L.O.Silva, R.A.Fonseca (IST Portugal) C.Ren (U. Rochester) T. Katsouleas (USC)
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Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Dec 22, 2015

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Page 1: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Full-scale particle simulations of high-energy density science experiments

W.B.Mori , W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou, V.K.Decyk, C. Joshi (UCLA)

L.O.Silva, R.A.Fonseca (IST Portugal)C.Ren (U. Rochester) T. Katsouleas (USC)

Page 2: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Directed high-energy density

• Pressure=Energy/Volume– Pressure=Power/Area/c

• PetaWatt with 10m spot– 3x1010 J/cm3

– 300 GBar

• Electric field in laser:– TeV/cm

• At SLAC:– N=2x1010 e- or e+

r=1m, z =60m

– E=50GeV

• Pressure:– 15x1010J/cm3

– 1.5TBar

• Electric field of beam:– 1.6TeV/cm

Lasers Particle beams

Page 3: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Radiation pressure and space forces of intense lasers and beams expel plasma electrons

Page 4: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Particle Accelerators Why Plasmas?

• Limited by peak power and breakdown

• 20-100 MeV/m

• No breakdown limit

• 10-100 GeV/m

Conventional Accelerators Plasma

a0 ≡eA

mc 2= 8.5x1010 I(W /cm2)λ μm

Why lasers?

Radiation pressure can excite longitudinal wakes

Page 5: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Laser Wake Field Accelerator(LWFA, SMLWFA, PBWA)

A single short-pulse of photons

Plasma Wake Field Accelerator(PWFA)

A high energy electron bunch

Concepts For Plasma Based Accelerators*

Drive beam Trailing beam

1. Wake excitation2. Evolution of driver and wake3. Loading the wake with particles

*Tajima and Dawson PRL 1979

Page 6: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Plasma Accelerator Progress and the “Accelerator Moore’s Law”

LOA,RAL

LBL ,RALOsaka

Slide 2

Courtesy of Tom Katsouleas

Page 7: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

The blowout and bubble regimesRosenzwieg et al. 1990 Puhkov and Meyer-te-vehn 2002

Ion column provides ideal accelerating and focusing forces

Page 8: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Typical simulation parameters:

~109 particles~105 time steps

Full scale 3D particle-in-cell modeling is now possible:OSIRIS

Other codes:VLPL, Vorpal, TurboWAVE, Z3 etc., but no all the same!

Page 9: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Progress in computer hardware

The “Dawson” cluster at UCLA: <$1,000,000

$50,000,000

Page 10: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Progress in lasers

Courtesy of G.Mourou

Page 11: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Progress in hardware and software

• Era Memory particles speed max energy (full PIC)

•80’s 16MByte 105-106 5s/part-step 100 MeV (2D)

•Today ~6TByte/3 ~109 1x10-3s/part-step 1-10GeV (3D(e.g., NERSC) (~7.5 Tflops/3)

•Local ~500GByte ~109 2x10-3 s/part-step 1-10GeV (3D)Clusters (2.3Tflops) 1 TeV (3D)(e.g., DAWSON)

•Future 25-1000TByte >1011 5x10-5s/part-step 500 GeV (3D)

150Tflops - 10Pflops?

The simulations of Tajima and Dawsonwould take ~1 second on my laptop!

Page 12: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Beam-driven wake* Fully ExplicitΔz ≤ .05 /cωp

Δy, Δx ≤ .05 /cωp

Δt ≤ .02 /cωp

# grids in z ≥350

# grids in x , y ≥150# s teps ≥2 x 10 5

Npa rticles ~.25 x 1 08 (3D)~1 x 10 6 (2D)

Pa rticles x s teps ~.5 x 1013 (3D) - ≥ 10,000 h rs~1 x 10 11 (2D) - ≥ 75 h rs

*Lase r-driven GeV st age re quires on the o rder of (ωo/ωp)2=1000 x longer , however , the the res olution ca n usua lly be re laxed.

Computational challenges for modeling plasma-based acceleration

(1 GeV Stage)

Page 13: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Full-scale modeling: Challenges and expectations

• As a laser propagates through the plasma it encounters ~1013-1014

electrons

• There are ~106-109 self-trapped electrons

• Need to model accuracy of 1 part in O(106)

• Don’t know exact plasma profile.

• Don’t know laser intensity or spot size.

• Don’t know laser transverse, longitudinal, or frequency profile (not a diffraction limited Gaussian beam).

Challenges: What is excellent agreement?

Page 14: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Convergence of advances in

laser technology and

computer simulation

Page 15: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

•Simulation Parameters–Laser:

• a0 = 1.1• W0=15.6 25 m• ωl/ωp = 10

–Particles• 2x1x1 particles/cell• 500 million total

–Plasma length• L=.2cm• 50,000 timesteps

Full scale 3D LWFA simulation using OSIRIS:6TW, 50fs

2340 cells56.18 m

512 cells100 m

512 cells100 m

State-of- the- art ultrashort laser pulse

0 = 800 nm, Δt = 50 fs

I = 2.5x1018 W/cm-2, W =12.5 m

Laser propagation

Plasma Backgroundne = 2x1019 cm-3

Simulation ran for 6400 hours on DAWSON

(~4 Rayleigh lengths)

Simulation ran for 6400 hours on DAWSON

(~4 Rayleigh lengths)

Page 16: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Simulations: no fitting parameters!Nature papers, agreement with experiment

• In experiments, the # of electrons in the spike is 1.4 108.

• In our 3D simulations, we estimate of 2.4 108 electrons in the bunch.

3D Simulations for: Nature V431, 541 (S.P.D Mangles et al)

-2 1011

0

2 1011

4 1011

6 1011

8 1011

1 1012

1.2 1012

1.4 1012

-50 0 50 100 150 200

Imperial Data #( /((dE/E) Ω)3 D OSIRIS

( )Energy MeV

Page 17: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Movie of Imperial RunPlasma density and laser envelope

QuickTime™ and aMPEG-4 Video decompressor

are needed to see this picture.

Page 18: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

3D PIC simulations:Tweak parameters

Parameters: E=1 J, 30 fs, 18 µm waist, 6×1018 cm-3

Scenario:• self-focusing (intensity increases by 10)• longitudinal compressionExcite highly nonlinear wakefield with cavitation: bubble formation

• trapping at the X point• electrons dephase and self-bunch• monoenergetic electrons are behind the laser field

Propagation: 2 mm

PIC

Experiment

Page 19: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

•Simulation Parameters–Laser:

• a0 = 4• W0=24.4 5 m• ωl/ωp = 33

–Particles• 2x1x1 particles/cell• 500 million total

–Plasma length• L=.7cm• 300,000 timesteps

Full scale 3D LWFA simulation using OSIRISPredict the future: 200TW, 40fs

4000 cells101.9 m

256 cells80.9 m

256 cells80.9 m

State-of- the- art ultrashort laser pulse

0 = 800 nm, Δt = 30 fs

I = 3.4x1019 W/cm-2, W =19.5 m

Laser propagation

Plasma Backgroundne = 1.5x1018 cm-3

Simulation ran for 75,000 hours on DAWSON

(~5 Rayleigh lengths)

Simulation ran for 75,000 hours on DAWSON

(~5 Rayleigh lengths)

Page 20: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

OSIRIS 200 TW simulation: Run on DAWSON Cluster

A 1.3 GeV beam!

The trapped particles form a beam. • Normalized emittance:The

divergence of the beam is about 10mrad.

• Energy spread:

Beam loading

Page 21: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Physical pictureEvolution of the nonlinear structure

• The blowout radius remains nearly constant as long as the laser intensity doesn’t vary much. Small oscillations due to the slow laser envelope evolution have been observed.

• Beam loading eventually shuts down the self injection.

• The laser energy is depleted as the accelerating bunch dephases. The laser can be chosen long enough so that the pump depletion length is longer than the dephasing length.

QuickTime™ and aMPEG-4 Video decompressor

are needed to see this picture.

Page 22: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

2-D plasma slab

Beam (3-D):

Laser or particles

Wake (3-D)

1. initialize beam

2. solve ∇⊥2ϕ =ρ, ∇⊥

2ψ =ρe ⇒ Fp,ψ

3. pushplasma, storeψ

4. stepslabandrepeat2.

5. useψ togiantstepbeam

QuickPIC loop:

Page 23: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Solved by 2D field solver

(1c2

∂2

∂t2 −∇2)A =4πc

j

(1c2

∂2

∂t2 −∇2)φ =4πρ

−∇⊥2A =

4πc

j

−∇⊥2φ =4πρ

plasma e− :

dPe

d(ξ /c)=

qe

1− vez /c(E +

1

cve × B)

dXe

d(ξ /c)=

ve

1− vez /c

⎨ ⎪ ⎪

⎩ ⎪ ⎪

beam e− :

dPb

d(s /c)= qb (E +

1

cvb × B)

dXb

d(s /c)= vb

⎨ ⎪ ⎪

⎩ ⎪ ⎪

Let :

s = z,ξ = ct − z

Assume :

(1) ∂s << ∂ξ

(quasi − static

approximation)

(2) vb ≈ c€

plasma e− :

dPe

dt=qe (E +

1

cve × B)

dXe

dt= ve

⎨ ⎪

⎩ ⎪

beam e− :

dPb

dt= qb (E +

1

cvb × B)

dXb

dt= vb

⎨ ⎪

⎩ ⎪

Maxell’s equations in Lorentz gauge Particle pusher(relativistic)

Full PIC(no approximation)

Let : Ψ = φ − A//

QuickPIC

QuickPIC: Basic concepts

−∇⊥2 φ = 4πρ

−∇⊥2 Ψ = 4π (ρ −

j//

c)

Page 24: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

QuickPIC: Code structure

Page 25: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

-3

-2

-1

0

1

2

-5 0 5 10

OSIRISQuickPIC

ξ( /cωp)

-3

-2

-1

0

1

2

3

-8 -6 -4 -2 0 2 4 6 8

OsirisQuickPIC (l=2)QuickPIC (l=4)

ξ ( /cωp)

-0.1

-0.05

0

0.05

0.1

-10 -5 0 5 10

Osiris

QuickPIC (l=2)

ξ ( /cωp)

-1

-0.5

0

0.5

1

-6 -4 -2 0 2 4 6

Osiris QuickPIC (l=2)

ξ ( /cωp)

e- driver e+ driver

e- driver with ionization laser driver

QuickPIC Benchmark: Full PIC vs. Quasi-static PIC

Benchmark for different drivers

Excellent agreement with full PIC code. More than 100 times time-savings. Successfully modeled current experiments. Explore possible designs for future experiments. Guide development on theory.

100+ CPU savings with “no” loss in accuracy

Page 26: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

A Plasma Afterburner (Energy Doubler) Could be Demonstrated at SLAC

Afterburners

3 km

30 m

S. Lee et al., Phys. Rev. STAB, 2001

0-50GeV in 3 km50-100GeV in 10 m!

Page 27: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Excellent agreement between simulation and experiment of a 28.5 GeV positron beam which has passed through a 1.4 m PWFA

OSIRIS Simulation Prediction:Experimental Measurement:

Peak Energy Loss64 MeV

65±10 MeV

Peak Energy Gain78 MeV

79±15 MeV

5x108 e+ in 1 ps bin at +4 ps

Head Tail Head Tail

OSIRIS E162 Experiment

Page 28: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Full-scale simulationof E-164xx is possible using a new code QuickPIC

• Identical parameters to experiment including self-ionization: Agreement is excellent!

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

0

+2

+4

-4

-2

0 +5-5X (mm)

Rel

ativ

e E

nerg

y (G

eV)

Page 29: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Full-scale simulationof E-164xx is possible using a new code QuickPIC

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

QuickTime™ and aYUV420 codec decompressor

are needed to see this picture.

Page 30: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

5000 instead of 5,000,000 node hours

• We use parameters consistent with the International Linear Collider “design”

•We have modeled the beam propagating through ~25 meters of plasma.

QuickTime™ and aMPEG-4 Video decompressor

are needed to see this picture.

Full-scale simulation of a 1TeV afterburner possible using QuickPIC

Page 31: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

I see a day where particle simulations

will use 1 trillion particles

I see a day where theworld is fueled

by fusion energy.

I see a day when high energy

acceleratorswill fit on a

tabletop.

Page 32: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

πρφ

π

4)1

(

4)

1(

22

2

2

22

2

2

=∇−∂

=∇−∂

tc

ctcjA

−∇⊥2 A =

cj

−∇⊥2 φ = 4πρ

−∇⊥2ψ = 4π (ρ − jz /c)

∂(ρ − j /c)

∂ξ+∇⊥⋅ j⊥ = 0

Maxwell equations in Lorentz gaugeReduced Maxwell equations

φ,A = ϕ (ct − z = ξ ,x⊥),A(ξ ,x⊥)

Quasi-static approx.

ψ =φ−Az

We define

Wakefield equations:“2D-electro and magneto-statics

Antonsen and Mora 1997

Whittum 1997

Huang et al., 2005 (QuickPIC)

Page 33: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

(1c2

∂2

∂t2 −∇2)A =4πc

j

(1c2

∂2

∂t2 −∇2)φ =4πρ

−∇⊥2A =

4πc

j

−∇⊥2φ =4πρ

quasi - static : ∂s ≈ 0

Maxwell equations in Lorentz gauge Reduced Maxwell equations

])([:

:

//⊥⊥

⊥ ×+−

=

⎥⎦

⎤⎢⎣

⎡ ×+−=

BV

EP

BV

EP

cVcq

dd

electronsplasmaFor

ccq

ds

delectronsbeamFor

e

e

ee

bbb

ξ

Initialize beam

Call 2D routine

Deposition

3D loop end

Push beam particles

3D loop begin

Initialize plasma

Field Solver

Deposition

2D loop begin

2D loop end

Push plasma particles Iteration

s =z, ξ =ct−z

2∂∂s

−ik0 +∂∂ξ

⎝⎜

⎠⎟a−∇⊥

2a=k02χ pa=−k0

2 ωp2

ω02γp

a

Quasi-static Model including a laser driver

Laser envelope equation:

Page 34: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Pipelining: scaling quasi-static PIC to 10,000+ processors

beam

solve plasma response

update beam

Initial plasma slab

Without pipelining: Beam is not advanced until entire plasma response is determined

solve plasma response

update beam

solve plasma response

update beam

solve plasma response

update beam

solve plasma response

update beam

Initial plasma slab

beam

1 2 3 4

1 2 3 4

With pipelining: Each section is updated when its input is ready, the plasma slab flows in the pipeline.

Page 35: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

LWFA - Accelerating Field

512 cells40.95 m

•Isosurface values:

•Blue : -0.9

•Cyan: -0.6

•Green: -0.3

•Red: +0.3

•Yellow: +0.6

•Electric Field in normalized units me c ωp e-1

•Isosurface values:

•Blue : -0.9

•Cyan: -0.6

•Green: -0.3

•Red: +0.3

•Yellow: +0.6

•Electric Field in normalized units me c ωp e-1

Page 36: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

SimulationsThe 200 TW run: Dephasing ~ Pump depletion

LT ≈1.0cm

Ldp ≈1.3cm

ΔE ≈1.5GeV

Laser plasma Given a we pick the density and we evaluate from our formulas:

After 5 Zr / 7.5 mm

Total charge = 1.1 nC

0

0.5

1

1.5

2

2.5

800 1200 1600 2000

f(E)

Energy (MeV)

f(E) (a.u.)

w0 = 20μm

τ =30 fs

a0 = 4

=0.8μm

P = 200TW

np =1.5 ×1018cm−3

P

Pc

≈10

Page 37: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Physical picture of an “optimal” regimeGeometry - fields

• The ponderomotive force of the laser pushes the electrons out of the laser’s way.

• The particles return on axis after the laser has passed.

• The region immediately behind the pulse is void of electrons but full of ions.

• The result is a sphere (bubble) moving with the speed of (laser) light, supporting huge accelerating fields.

• The ponderomotive force of the laser pushes the electrons out of the laser’s way.

• The particles return on axis after the laser has passed.

• The region immediately behind the pulse is void of electrons but full of ions.

• The result is a sphere (bubble) moving with the speed of (laser) light, supporting huge accelerating fields.

Page 38: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

Physical pictureEvolution of the nonlinear structure

• The front of the laser pulse interacts with the plasma and loses energy. As a result the front etches back.

• The shape and size of the accelerating structure slightly change.

• Electrons are self-injected in the plasma bubble due to the accelerating and focusing fields.

• The trapped electrons make the bubble elongate.

• The front of the laser pulse interacts with the plasma and loses energy. As a result the front etches back.

• The shape and size of the accelerating structure slightly change.

• Electrons are self-injected in the plasma bubble due to the accelerating and focusing fields.

• The trapped electrons make the bubble elongate.

Page 39: Full-scale particle simulations of high- energy density science experiments W.B.Mori, W.Lu, M.Tzoufras, B.Winjum, J.Fahlen,F.S.Tsung, C.Huang,J.Tonge M.Zhou,

PIC Simulations of beam loading in blowout regime:Used the new code QuickPIC

(UCLA,USC,U.Maryland)

Wedge shape w/ beam load beam length = 6 c/ωp, nb/np= 8.4, Ndrive = 3x1010, Ntrailing = 0.5x1010

Bi-Gaussian shapez= 1.2 c/ωp, nb/np= 26