parra - ultrashort pulse (usp) laser matter interactions - spring review 2012

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1 DISTRIBUTION A: Approved for public release; distribution is unlimited. 15 February 2012 Integrity Service Excellence Riq Parra Program Manager AFOSR/RSE Air Force Research Laboratory Ultrashort Pulse (USP) Laser-Matter Interactions 08 MAR 2012

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Dr. Riq Parra presents an overview of his program - Ultrashort Pulse (USP) Laser Matter Interactions - at the AFOSR 2012 Spring Review.

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Page 1: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

1 DISTRIBUTION A: Approved for public release; distribution is unlimited. 15 February 2012

Integrity Service Excellence

Riq Parra

Program Manager

AFOSR/RSE

Air Force Research Laboratory

Ultrashort Pulse (USP)

Laser-Matter

Interactions

08 MAR 2012

Page 2: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

2 DISTRIBUTION A: Approved for public release; distribution is unlimited.

USP Laser Matter Interactions

Page 3: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

3 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Characteristics of short pulse lasers

• The program aims to understand and control light sources exhibiting

extreme bandwidth, peak power and temporal characteristics.

• Portfolio sub-areas: optical frequency combs, high-field science,

attosecond physics.

Peak

Power

Pulsewidth Bandwidth

Page 4: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

4 DISTRIBUTION A: Approved for public release; distribution is unlimited.

USP

Lasers

Secondary Radiation Sources generation of particle & photons

• High power THz generation

• Extreme ultraviolet

lithography

• Biological soft x-ray

microscopy

• Non-destructive evaluation

• Medical imaging/therapy

Metrology stabilized, ultra-wide bandwidth

• Ultra-stable freq sources

• Arb waveform generation

• High precision spectroscopy

• Frequency/time transfer

• Ultra-wideband comms

• Coherent LIDAR

• Optical clocks

• Calibration

Material Science ultrashort, high peak power

• Surgery

• Chemical analysis (LIBS)

• Surface property

modification

• Non-equilibrium ablation

• Micromachining

• Ultrafast photochemistry

• Attochemistry

Propagation in media self-channeling

• Remote sensing

• Remote tagging

• Directed energy

• Electronic warfare

• Countermeasures

• Advanced sonar

Particle Acceleration ultrahigh electric field gradients

• Table-top GeV electron

accelerators

• MeV ion sources for

imaging

• Isotope production

• Hadron tumor therapy

• Proton-based fast

ignition

Applications of USP Lasers

Page 5: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

5 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Modelocked femtosecond lasers

Source: Diddams, JOSA B (2010)

Thorlabs

Page 6: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

6 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Mode-locked lasers as broadband phase-

coherent optical sources (optical

frequency combs)

Page 7: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

7 DISTRIBUTION A: Approved for public release; distribution is unlimited.

PI: James Gord, AFRL/RZ

Advancing Ultrafast Lasers for High-

Bandwidth 4D Metrology

• Ultrashort pulses for propulsion measurements

• Ultrafast laser–based spectroscopic techniques for investigating the physics

and chemistry of reacting flows.

• Generate top-quality data for

• advanced concept development and model validation (R&D)

• propulsion-system performance assessment (T&E)

• weapon-system active combustion control (ACC)

• Measure everything, everywhere, all the time…

Pratt & Whitney F119

Page 8: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

8 DISTRIBUTION A: Approved for public release; distribution is unlimited.

PI: James Gord, AFRL/RZ

Spectrally Resolved Femtosecond

CARS 1D Line Imaging

Key fs-CARS advantages

• >3 OOM faster data acquisition

• 1D line vs. point measurements

• Free from collisional broadening

• Nonresonant-background control

• Strong coherences

• Improved accuracy, precision

• Species-selective [n] and T

• Multiple-species excitation

16-shot avg.

Single-shot

Single-shot, one-dimensional thermometry in flames

Page 9: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

9 DISTRIBUTION A: Approved for public release; distribution is unlimited.

An optical frequency comb

Source: Diddams, JOSA B (2010)

Repetition rate

phase-locked to a

microwave reference.

fo measured via the

heterodyne between

the second harmonic

of the IR & VIS comb

components.

Page 10: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

10 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Metrological applications

of optical frequency combs

Source: Newbury, Nature Photonics (2011)

Page 11: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

11 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Microresonator frequency combs

Source: Kippenberg et al., Science (2011)

CaF2 SiN rings Silica toroids

FY2012 Basic Research Initiative (BAA-AFOSR-2012-02)

Page 12: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

12 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Mode-locked lasers as high peak power

sources (high field science)

Page 13: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

13 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Progress in peak intensity

• Over the last two decades, a 6 order of magnitude increase in achieved

focused intensities in table-top systems.

Source: CUOS website

2x1022

Phenomena Relevance

Thomson scattering Gamma rays source

Laser wakefield

acceleration

Compact e-

accelerators

Particle and x-ray

emission from solids

Proton & x-ray

sources

High harmonic

generation

Coherent EUV

sources

Filamentation Propagation of

EM pulses

Laser ablation

of solids

Laser machining

& patterning

Page 14: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

14 DISTRIBUTION A: Approved for public release; distribution is unlimited.

High intensity lasers are reducing from

national lab to university scale systems

Attributes LLNL Petawatt (1998) Thales Alpha 10 (2012)

Power per pulse 660 J 40 J

Pulse width 440 fs 25 fs

Focused intensity 7 x 1020 (W/cm2) n/a

Peak power 1.5 PW 1.3 PW

Size Building 14 x 19 ft2

Rep rate few shots/day 1 Hz

Gain material Nd:glass Ti:Sapphire

Commercial product!

SIZE Thales

Alpha 10

brochure

Thales Alpha 10

Page 15: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

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Laser micromachining & patterning

• Ultrashort laser pulses open up novel

possibilities and mechanisms for laser-solid

interactions.

• Demonstrated femtosecond laser processing

and surface texturing techniques to engineer

surface structures & properties (e.g. darkened &

colored metals, super wicking surfaces).

• Studied nanostructure-covered laser-induced

periodic surface structures (NC-LIPSS) &

nanostructure-covered large scale waves (NC-

LSW).

Colorizing metals using femtosecond lasers

Super wicking surfaces: Array of parallel

microgrooves generates strong capillary force.

PI: Chunlei Guo, U of Rochester

NC-LIPSS NC-LSW

Page 16: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

16 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Propagation of high-intensity USPL pulses

• Propagation of localized high-intensity laser pulses is of

interest for remote sensing, imaging, communications and

remote interactions.

• Such propagation in air leads to self-channeling (i.e.

filaments) and plasma formation.

• AFRL/RDLA Filamentation Team is engaged in an

experimental, theoretical and computational effort to:

• Develop computational models for long-distance fs propagation

as an extended free space waveguide.

• Study filament propagation for long distances (2, 5 & 7 km test

sites available).

• Characterize fs-laser filament physics necessary for

coupling/confining external EM-Fields.

• Understand filamentation induced electrical shorting.

PI: William P Roach, AFRL/RD

9-inch filament bundle propagation

through kV-level E-Field

Range

High-performance

GPU computing

enclave

Page 17: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

17 DISTRIBUTION A: Approved for public release; distribution is unlimited.

PI: Pavel Polynkin, Arizona

Optical breakdown of air triggered by

femtosecond laser filaments

• Generation and 200x enhancement of dense

plasma channels at range via dual-pulse

femtosecond-nanosecond laser excitation.

• Control of femtosecond laser filamentation

through laser beam engineering. Extended bottle-

like plasma-channel distributions using vortex

beams and high order Bessel beams.

100 laser shots

fs pulse only

Single shot

fs + ns pulses

Bottle-like filament

patterns produced by

vortex beams in water

Page 18: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

18 DISTRIBUTION A: Approved for public release; distribution is unlimited.

High Harmonic Generation (HHG)

Microscopic single-

atom physics of HHG

Macroscopic phase-matched

harmonic emission

Source: Popmintchev et al., Nat Photonics (2010),

Popmintchev et al., CLEO postdeadline (2011)

Co Ni Cu Fe C O N B

lLASER=3.9 mm

0.8mm

2mm

WATER WINDOW

Page 19: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

19 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Direct Frequency Comb Spectroscopy

in the Extreme Ultraviolet

• Generating frequency combs in the extreme

ultraviolet (XUV) via high harmonic generation

(HHG) in a femtosecond enhancement cavity.

• Demonstrated generation of >200 µW per

harmonic down to 50 nm.

• Ultrahigh precision spectroscopy below the

100 nm spectral region:

• Direct frequency comb spectroscopy of Argon

transition at 82 nm with resolved 10 MHz

linewidth (atomic thermal motion limited).

10 MHz Ar @ 82 nm

PI: Jun Ye, U of Colorado

119 nm 97 nm 82 nm 47 nm 71 nm

Page 20: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

20 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Diocles 100 TW laser system

• Nd:YAG pumped Ti:Sapphire

• 3.5 J in < 30 fs, 100 TW @ 10 Hz

Spot size (FWHM) = 16 microns

Enclosed energy > 75-80 %

Focal spot

PI: Donald Umstadter, U of Nebraska

Page 21: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

21 DISTRIBUTION A: Approved for public release; distribution is unlimited.

• Scattering from a 300 MeV electron beam

can Doppler shift a 1-eV energy laser

photon to 1.5 MeV energy.

• Demonstrated > 710 MeV electron beams

with no detectable low-energy

background.

• Proof-of-principle experiments are

underway.

Laser-driven x-rays generation

(0.1 – 10 MeV) PI: Donald Umstadter, U of Nebraska

Super

Sonic

Nozzle

E-Beam

Scattering

Laser Pulse

Experimental geometry

for generating x-rays via

Thomson scattering

> 710 MeV

electrons

Energy tunability from 0.1 – 0.8 GeV.

Monoenergetic: ΔE/E ~ 10 %

Low angular divergence: 1-5 mrad

Page 22: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

22 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Repetitive petawatt-class laser

• Completed upgrade to 0.7 PW

@ 0.1 Hz.

10-cm Ti:Sapphire power amplifier

25-J Nd:glass pump lasers

New gratings for pulse compressor

PW Specifications

Wavelength 805 nm

Pulse duration < 30 fs

Rep rate 0.1 Hz

Pulse energy 20 J

Peak power 0.7 PW

Strehl ratio 0.95

Max intensity (f/2) 1x1023 W cm-2

PI: Donald Umstadter, U of Nebraska

Page 23: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

23 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Mode-locked lasers as sources of

ultrashort EM pulses (attosecond physics)

Page 24: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

24 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Generation of single attosecond

photon pulses

Source: Corkum, Nature Physics (2007),

Goulielmakis, Science (2008)

Streaking spectrogram Retrieved intensity profile

ww

w.a

tto

wo

rld.d

e

Page 25: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

25 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Attosecond pulses provide a new set

of metrology tools

Source: Krausz, RMP (2009)

Page 26: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

26 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Sub-cycle optical pulses for isolated

attosecond pulse generation

• Coherent wavelength multiplexing of high

energy pulses, spanning two octaves, into

a non-sinusoidal waveform with sub-cycle

features.

• Shortest high-field transient lasts 0.8 cycles of the carrier frequency.

• Unique, scalable approach to higher

energies and rep rates for high average

power sources of isolated attosecond

pulses.

PI: Franz Kaertner, MIT High-energy optical

waveform synthesizer

Computed isolated attosecond pulse Synthesized waveform

0.8 cycles Waveform supports

directly isolated soft

X-ray pulse with

150 as duration (with

no gating).

Page 27: Parra - Ultrashort Pulse (USP) Laser Matter Interactions - Spring Review 2012

27 DISTRIBUTION A: Approved for public release; distribution is unlimited.

Optical frequency combs ultra-wide bandwidths

• Spectral coverage to exceed an

octave with high power/comb.

• Coherence across EUV-LWIR.

• Novel resonator designs (e.g.

micro-resonator based).

• Ultra-broadband pulse shaping.

• …

Attosecond science ultrashort pulsewidths

• Efficient, high-flux generation.

• Pump-probe methods.

• Probe atoms/molecules &

condensed matter systems.

• Attosecond pulse propagation.

• Novel attosecond experiments.

• Fundamental interpretations of

attosecond measurements.

• …

Summary and outlook

The program aims to understand

and control light sources exhibiting

extreme temporal, bandwidth and

peak power characteristics.

High-field laser physics high peak powers

• Laser-solid interactions.

• Fs propagation in media.

• Sources of secondary photons.

• Compact particle accelerators.

• High peak power laser

architectures.

• High repetition rates.

• New wavelengths of operation.

• …