Monoenergetic Proton Beams from Laser Driven...

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Monoenergetic Proton Beams from Laser Driven Shocks Dan Haberberger Neptune Laboratory, Department of Electrical Engineering, UCLA In collaboration with: Sergei Tochitsky, Chao Gong, Warren Mori, Chan Joshi Neptune Laboratory, Department of Electrical Engineering, UCLA Frederico Fiuza, Luis Silva, Ricardo Fonseca Instituto Superior Technico, Lisbon, Portugal

Transcript of Monoenergetic Proton Beams from Laser Driven...

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Monoenergetic Proton Beams from Laser Driven

Shocks

Dan Haberberger Neptune Laboratory, Department of Electrical Engineering, UCLA

In collaboration with: Sergei Tochitsky, Chao Gong, Warren Mori, Chan Joshi

Neptune Laboratory, Department of Electrical Engineering, UCLA

Frederico Fiuza, Luis Silva, Ricardo Fonseca

Instituto Superior Technico, Lisbon, Portugal

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Outline

AAC (Jun 2012) Neptune Laboratory

• Applications of Laser Driven Ion Acceleration (LDIA) : Hadron cancer therapy • Localized energy deposition : Bragg Peak • Therapy centers : conventional accelerators vs. lasers • Ion source requirements

• Collisionless Shock Wave Acceleration (SWA) of protons • 1D OSIRIS Simulations • Laser driven case

• UCLA proton acceleration experiment : CO2 laser and a H2 gas jet target • Results : Spectra, emittance • Interferometry : Plasma density profile

• 2D OSIRIS simulations • Modeling the experiment • Scaling to higher power lasers • Using 1µm laser systems

• Conclusion

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Laser Driven Ion Beam Applications

Probing of strong electric fields in dense plasma on the picosecond timescale

– ~1μm resolution, 5-20MeV

– Borghesi, Phys. Plasmas (2002) • 50μm Ta wire • Imaging with 6-7MeV protons

-15ps -5ps 5ps

VULCAN Laser, 20J, 1019W/cm2

Hadron Cancer Therapy – 250MeV, 109-1010 protons/s – ΔE/E ≤ 5%

Fast Ignition – 15-23MeV – <20ps – Eff = 10%

Picosecond injectors for conventional accelerators – 1-10MeV, <.004 mm.mrad, <10-4 eV.s [Cowan, Phys. Rev. Lett. (2004)]

AAC (Jun 2012) Neptune Laboratory

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Energy Deposition : Ions vs. Photons

AAC (Jun 2012) Neptune Laboratory

Bragg Peak for ions results in localized energy deposition

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Multi-beam Localization

Radiation dose relative to peak (100%)

Simulations of Irradiating the Human Skull

GSI Helmholtz Centre for Heavy Ion Research in Darmstadt http://www.weltderphysik.de/gebiet/leben/tumortherapie/warum-schwerionen/

AAC (Jun 2012) Neptune Laboratory

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Problem : Cost and Size

Heidelberg Ion-Beam Therapy Center, Commissioned in 2009

Cost : ~200 Million USD • Accelerator ring (20m) • Transport magnets • Complicated Gantry • Radiation shielding

Only a few in operation along with ~30 small facilites • 10’s of thousands of people

treated • Need more than an order of

magnitude more therapy centers

20 meters

http://www.klinikum.uni-heidelberg.de/Welcome.113005.0.html?&L=1 AAC (Jun 2012) Neptune Laboratory

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Solution : Laser Based Accelerators

Goal Cost : 10-20 million USD Table top laser system (developing) Transportation : Mirrors Only has focusing magnet Gantry : small, protons generated in direction of patient

M. Murakami, et al., AIP Conf. Proc. 1024 (2008) 275, doi:10.1063/1.2958203

AAC (Jun 2012) Neptune Laboratory

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Proton Beam Requirements

Radiation Beam Requirements

2 Gray in 1 liter tumor in a few minutes -Translates to 1010 protons per second

Proton energies in range of 250 MeV

Energy Spread of ~5%

Focusability, Energy Accuracy, Energy Variability, Dose Accuracy, etc.

Lasers can accelerate up to 1012 protons in a single shot Worlds most powerful lasers have produced 75 MeV protons

Vast majority of beams have continuous energy spread

Future Work

Laser Driven Ion Acceleration (LDIA)

AAC (Jun 2012) Neptune Laboratory

Dose

Energy

Energy Spread

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What is a Shock Wave?

Subsonic Sonic Supersonic

A disturbance that travels at supersonic speeds through a medium

• At supersonic speeds, pressure will build at the front of a disturbance forming a shock

• Characterized by a rapid change in pressure (density and/or temperature) of the medium

In a plasma, a shock wave is characterized by a propagating electric field at speeds useful for ion acceleration (Vsh > 0.01c)

AAC (Jun 2012) Neptune Laboratory

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1D OSIRIS Simulations

Plasma 1 ne1

Te

Cold Ions

Plasma 2 ne2 Te

Cold Ions

In Plasmas, the driver is a potential or electric field

Plasma 1 ne1 = ne2

Te1

Cold Ions

Plasma 2 ne1 = ne2

Te1

Cold Ions

Expansion Shocks Driven Shocks

Ambipolar electric field of Plasma 1 is driven into

Plasma 2

Initial drift causes overlap; overlap causes local density

increase and again ambipolar electric field is driven into the

plasma

←Vd /2 Vd /2→

AAC (Jun 2012) Neptune Laboratory

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1D Sims : Driven Shocks (Te = 511 keV Cs = 0.0233c).

Wave train response

Proton trapping begins

Proton reflection begins

Strong damping of wave

No interaction

Reflection Condition eɸ > 1/2mv2

AAC (Jun 2012) Neptune Laboratory

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Shock formation in laser driven plasmas

• Linearly polarized laser incident upon an overcritical target creates and heats the plasma

• Ponderomotive force creates density spike and imparts a velocity drift on surface plasma

High-intensity laser pulse E

Shock

acceleration

Sheath Field

(TNSA)

Beam quality destroyed

by TNSA fields

F. Fiuza | Prague, April 20 | SPIE 2011

Denavit PRL 1992, Silva PRL 2004

AAC (Jun 2012) Neptune Laboratory

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• Gas jets can be operated at or above 1019 cm-3 (ncr for 10µm)

• Long scale length plasma on the back side of the gas jet inhibits strong TNSA fields preserving proton spectrum

• High repetition rate source • Clean source of ions (H2, He, N2,

O2, Ar, etc…) • Low plasma densities allows for

probing of plasma dynamics using visible wavelengths

Gas jet target advantages for Shock Wave Acceleration (SWA)

CO2 Laser Interacting with a Gas Jet Target

Gas plume

hybrid PIC Extended Plasma Steepened

Plasma E TNSA ~ 1/L

AAC (Jun 2012) Neptune Laboratory

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CO2 Laser Pulse Temporal Structure

Pressure = 8atm Line Separation = 55GHz

Line Center : 10.6µm

400 450 500 550 6000

1

2

3

4MARS Shot # 14300

Peak P

ow

er

(TW

)

Time (ps)300 400 500 600

0

0.5

1

1.5

2

2.5

MARS Shot # 14405

Peak P

ow

er

(TW

)

Time (ps)

~70ps ~110ps

D. Haberberger et al., Opt. Exp. 18, 17865 (2010) AAC (Jun 2012) Neptune Laboratory

Experimentally Measured Temporal Profile

Calculated CO2 Gain Spectrum

E = 50 J Ppeak = 4TW

Pulse Separation = 1/55GHz = 18.5ps 7-10 pulses long

18.5ps

~70ps

3ps

27 27.5 28 28.50

0.2

0.4

0.6

0.8

1

No

rma

lized

Am

plit

ude

Frequency (THz)

Frequency Spectrum

CO2 Gain Spectrum at 8atm

3ps Input Pulse Spectrum

Overlapped Spectrums

0 50 100 150 2000

0.2

0.4

0.6

0.8

1

Time (ps)

Amplified PulseTemporal Structure

18ps = 1/55GHz

3ps

1.2THz

55GHz

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0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 5.5 660

0.2

0.4

0.6

0.8

1

Distance (mm)

dE

/dx (

Norm

aliz

ed U

nits)

Energy Deposition of Protons in CR-39 vs. Distance

1mm CR-39

CR-39 Proton Detection

CR-39 1mm

Detection: 11-15 MeV

CR-39 1mm

Detection: 16-19 MeV

CR-39 1mm

Detection: 20-22 MeV

CR-39 1mm

Detection: 23-25 MeV

150mm 100x100mm Imaging Proton

Spectrometer

Protons 10μm Laser Pulse

CR-39 1mm

Detection: <1-10 MeV

1 MeV 27 MeV

AAC (Jun 2012) Neptune Laboratory

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CO2 Laser Produced Proton Spectra

1mm CR-39

Energy spreads measured to

be FWHM ΔE/E ̴ 1%

Feb 22th

CR-39 #179

Jan 25th

CR-39 #92

Jan 25th

CR-39 #99 Haberberger, Tochitsky, Fiuza, Gong, Fonseca, Silva, Mori, Joshi, Nature Phys., 8, 95-99 (2012)

Noise Floor

AAC (Jun 2012) Neptune Laboratory

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Emittance Estimation

Source Size : d = 120µm Beam Size (RMS) : σx ̴ 5.7mm σy ̴ 2.2mm Divergence : θx ̴ 37mrad θy ̴ 14mrad Emittance : εx = d.θx = 4.6mm.mrad εy = d.θy = 1.7mm.mrad

H2 Gas Jet

CR-39 150mm

Laser

Protons

50

mm

50mm

σy

σx 11/30/10 22MeV

AAC (Jun 2012) Neptune Laboratory

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Plasma Density Profile

-600 -400 -200 0 200 4000

1

2

3

4

X-Distance (m)

Pla

sm

a D

en

sit

y

(10

19cm

-3)

Y-D

ista

nce (

m)

-600

-300

0

300

600

Laser

Laser Observations 1. Strong profile

modification on the front side of the plasma : hole boring

2. Sharp rise (10λ) to overcritical plasma where laser pulse is stopped

3. Long (1/e 30λ) exponential plasma tail

AAC (Jun 2012) Neptune Laboratory

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2D OSIRIS Simulations : Input Deck

linear ramp

exponential ramp (plasma expansion)

18 ps

Initial Plasma Profile

Laser ao = 2.5 Δτ = 3ps

Laser ao = 2.5 Δτ = 3ps

AAC (Jun 2012) Neptune Laboratory

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2D OSIRIS Simulations : Results Time = 17ps Time = 52ps Time = 122ps

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2D Simulations : Energy Scaling

UCLA

AAC (Jun 2012)

-K. Zeil et. al., New J. Phy 12, 045015 (2010)

𝐸𝑝 ∝ 𝑎𝑜3 2

-F. F

iuza

, Ph

ys. R

ev. L

ett.

, Su

bm

itte

d

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Proposed Shock Wave Acceleration at 1µm

Gas plume

hybrid PIC Extended Plasma

E TNSA ~ 1/L

AAC (Jun 2012) Neptune Laboratory

10µm Laser – Gas Jet Target 1µm Laser – Exploded Foil Target

High Power Drive Pulse

Low Power Pre-heater

Foil target of thickness Δx

Ion beam

Δx and Δt • Peak density for Drive Pulse is 5-

15ncr = 5-15 x 1021 cm-3 • Extended plasma profile (1/e - 30λ)

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Conclusions Laser-driven, electrostatic, collisionless shocks in overdense plasmas

produce monoenergetic protons at high energies • Protons accelerated to 15-22 MeV (at IL ~ 4x1016 W/cm2) • Energy spreads as low as 1% (FWHM) • Emittances as low as 2x4 mm·mrad • Interferometry uncovers unique plasma profile • Plasma simulations elucidate shock wave acceleration of

protons through the backside of the plasma

AAC (Jun 2012) Neptune Laboratory

Step towards achieving 200-300 MeV protons needed for cancer therapy

• Simulations show scaling to ~300 MeV with a laser ao = 15

• Proposed method of exploding foil target for 1µm laser systems