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1 Integrity Service Excellence Ultrashort Pulse (USP) Laser – Matter Interactions 5 MAR 2013 Dr. Riq Parra Program Officer AFOSR/RTB Air Force Research Laboratory DISTRIBUTION A: Approved for public release; distribution is unlimited

Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Dr. Riq Parra presents an overview of his program, Ultrashort Pulse (USP) Laser -- Matter Interactions, at the AFOSR 2013 Spring Review. At this review, Program Officers from AFOSR Technical Divisions will present briefings that highlight basic research programs beneficial to the Air Force.

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Page 1: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

1

Integrity Service Excellence

Ultrashort Pulse (USP) Laser – Matter

Interactions

5 MAR 2013

Dr. Riq Parra

Program Officer

AFOSR/RTB

Air Force Research Laboratory

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Page 2: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

2

500 700 900

nm

25 nm

300 nm

0.002 nm

BANDWITH

Modelocked femtosecond lasers

Light Emitting Diode

Ti:Sapphire modelocked fs laser

Sunlight

He-Ne cw laser

Wik

iped

ia

Wik

iped

ia

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time

time

time

time

Pulses!

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2013 AFOSR SPRING REVIEW 3001O PORTFOLIO OVERVIEW

• 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.

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Page 4: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Applications of USP Lasers

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 • Optical waveform synthesis • High precision spectroscopy • Frequency/time transfer • High-capacity 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

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Page 5: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Outline

– Microresonator-based optical frequency combs

– High peak power, ultrashort pulse laser processing of materials

– Extreme ultraviolet (EUV) comb spectroscopy

– High harmonic interferometry

– Relativistic optics

DISTRIBUTION A: Approved for public release; distribution is unlimited Photo credits: DOI: 10.1038/nature05524, www.attoworld.de, E. Chowdhury (OSU)

Page 6: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Outline

– Microresonator-based optical frequency combs

– High peak power, ultrashort pulse laser processing of materials

– Extreme ultraviolet (EUV) comb spectroscopy

– High harmonic interferometry

– Relativistic optics

DISTRIBUTION A: Approved for public release; distribution is unlimited Photo credits: DOI: 10.1038/nature05524, www.attoworld.de, E. Chowdhury (OSU)

Page 7: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Optical frequency combs: Frequency & time domains

Source: Kippenberg et al., Science (2011); Diddams. DISTRIBUTION A: Approved for public release; distribution is unlimited

2∆φ

τr.t = 1/fr

t

E(t) ∆φ

Frequency domain

Time domain

Page 8: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Metrological applications of optical frequency combs

Source: Newbury, Nature Photonics (2011) DISTRIBUTION A: Approved for public release; distribution is unlimited

Page 9: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Sou

rce:

Bra

je, P

hysi

cs 3

, 75

(201

0)

Combs in monolithic microresonators

High-Q mm crystalline resonators

top left doi: 10.1038/nphoton.2012.127 right doi: 10.1103/physreva.84.053833 bottom left doi: 10.1103/physrevlett.101.093902

CaF

2

Fused-quartz

MgF

2

Silica toroids

doi:1

0.10

38/n

atur

e064

01

Silicon nitride microrings

doi: 10.1038/nphoton.2009.259

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Parametric

Source: Kippenberg et al., Science (2011)

Conventional

Presenter
Presentation Notes
Different approach to comb generation, in which equally spaced frequency markers are produced by the interaction between a continuous-wave pump laser of a known frequency with the modes of a monolithic ultra-high-Q microresonator13 via the Kerr nonlinearity.
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Octave spanning bandwidths

Source: Del’Haye, Phys. Rev. Lett. 107, 063901 (2011), Okawachi, Opt. Lett. 36, 3398 (2011) DISTRIBUTION A: Approved for public release; distribution is unlimited

Page 11: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Why microresonators?

Source: Kippenberg et al., Science (2011) DISTRIBUTION A: Approved for public release; distribution is unlimited

Page 12: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Comb generation dynamics

DISTRIBUTION A: Approved for public release; distribution is unlimited Graphics adapted from Herr, arXiv:1111.3071v1, 2011

Page 13: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Comb generation dynamics

DISTRIBUTION A: Approved for public release; distribution is unlimited Graphics adapted from Herr, arXiv:1111.3071v1, 2011

Page 14: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Comb generation dynamics

DISTRIBUTION A: Approved for public release; distribution is unlimited Graphics adapted from Herr, arXiv:1111.3071v1, 2011

Page 15: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Comb generation dynamics

DISTRIBUTION A: Approved for public release; distribution is unlimited Graphics adapted from Herr, arXiv:1111.3071v1, 2011

Page 16: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Comb generation dynamics

DISTRIBUTION A: Approved for public release; distribution is unlimited Graphics adapted from Herr, arXiv:1111.3071v1, 2011

Page 17: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Comb generation dynamics

DISTRIBUTION A: Approved for public release; distribution is unlimited Graphics adapted from Herr, arXiv:1111.3071v1, 2011

Page 18: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Comb generation dynamics

DISTRIBUTION A: Approved for public release; distribution is unlimited Graphics adapted from Herr, arXiv:1111.3071v1, 2011

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(FY12 BRI) Microresonator-based optical frequency combs

• Initiative aimed at exploring the fundamental physics of microresonator comb generation.

• Six efforts exploring:

– Spatio-temporal field mapping and control

– Silicon-carbide microdisks

– Silicon nitride resonators

– Mid-IR microresonators

– Time domain characterization

– Dispersion tailoring via slotted waveguides

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Page 20: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Temporal and Spectral Comb Generation Dynamics

Optical spectrum

RF spectrum Temporal output

Source: http://arxiv.org/abs/1211.1096v3

PI: Alex Gaeta, Cornell

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Presenter
Presentation Notes
As the comb grows further, you see the RF noise continue to increase.
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Temporal and Spectral Comb Generation Dynamics

Source: http://arxiv.org/abs/1211.1096v3

PI: Alex Gaeta, Cornell Optical spectrum

RF spectrum Temporal output

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Presenter
Presentation Notes
Now at this point we see some very interesting behavior…. (next slide)
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Temporal and Spectral Comb Generation Dynamics

Transition to modelocking? Source: http://arxiv.org/abs/1211.1096v3

PI: Alex Gaeta, Cornell Optical spectrum

RF spectrum Temporal output

DISTRIBUTION A: Approved for public release; distribution is unlimited

Presenter
Presentation Notes
And as the pump is further tuned into resonance, the spectrum equalizes and an ultrafast pulse train is formed while maintaining a low-noise state.
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99-GHz repetition rate

160-fs pulses

Ultrashort Pulses at 99 GHz

Source: http://arxiv.org/abs/1211.1096v3

PI: Alex Gaeta, Cornell

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Page 24: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Outline

– Microresonator-based optical frequency combs

– High peak power, ultrashort pulse laser processing of materials

– Extreme ultraviolet (EUV) comb spectroscopy

– High harmonic interferometry

– Relativistic optics

DISTRIBUTION A: Approved for public release; distribution is unlimited Photo credits: DOI: 10.1038/nature05524, www.attoworld.de, E. Chowdhury (OSU)

Page 25: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Long laser pulse Ultrashort pulses

Long laser pulse damages adjacent structures Ultrashort pulses no collateral damage

Source: C. Momma, A. Tunnermann et al., Opt. Commun. 129, 134 (1996) DISTRIBUTION A: Approved for public release; distribution is unlimited

Presenter
Presentation Notes
It has been shown that the quality of ablated holes and patterns produced with femtosecond pulses is much better than the quality of structures produced with nanosecond or even picosecond laser pulses,1–4 and that submicron features can be produced on metal and semiconductor surfaces. It is well known that metals are very problematic materials for microstructuring with lasers owing to their high thermal conductivities and low melting temperatures. With conventional laser systems delivering pulses longer than 1 ns, the ablation of metals is always accompanied by the formation of large heat-affected zones and a throw out of the molten material. This limits the achievable precision and the quality of the produced structures. The fs pulses are shorter than all major relaxation times. Such pulses excite only electrons, leaving the lattice cold for the time required for the transfer of the absorbed laser energy from the heated electrons to the lattice. For this reason, any laser-induced phase transformations occur in non-equilibrium conditions, making properties of the material drastically different from their equilibrium counterparts. [Gamaly]
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Timescales of electron and lattice processes in laser-excited solids

Time-dependent processes in materials

Source: Sundaram, Nat Mater 1, 217 (2002), Mao, Applied Physics A 79, 1695 (2004).

10 – 100 fs

Multi- photon

Tunneling

Avalanche

Excitation mechanisms

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Page 27: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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High peak power, ultrashort pulse laser processing of materials

• 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 & colorized metals, hydrophilic & hydrophobic surfaces).

Colorized metals

PI: Chunlei Guo, U of Rochester

Hydrophilic Hydrophobic

DISTRIBUTION A: Approved for public release; distribution is unlimited

Presenter
Presentation Notes
Ablation of solids by high fluence, ultrashort laser pulses makes ablated materials undergo different, extreme phase changes. The mechanism of the laser-material interaction in this regime critically depends on photon-electron-phonon dynamics, plasma formation and its interaction with the incident laser beam, solid target and surrounding media such as air.
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(FY13 BRI) High peak power, ultrashort pulse laser processing of materials

• Initiative aimed at developing a fundamental understanding of intense field laser ablation/damage in the femtosecond regime.

• Three multi-PI efforts exploring: – Dynamics of ionization – Fundamental dynamics of laser ablation – Defect states in multi-pulse interaction – Effect of structures on laser damage – First principle-based models, non-

adiabatic quantum MD, classical MD – Vary λ = 400 nm – 4 µm, τ = 5 – 1000 fs – Complex beam shapes (Bessel, Airy,

vortex, SSTF beams) – Novel laser-matter interaction geometries

(confined microexplosions, SSTF excitation, few-cycle pulses)

SSTF focus

Gratings

Classical MD

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Page 29: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Outline

– Microresonator-based optical frequency combs

– High peak power, ultrashort pulse laser processing of materials

– Extreme ultraviolet (EUV) comb spectroscopy

– High harmonic interferometry

– Relativistic optics

DISTRIBUTION A: Approved for public release; distribution is unlimited Photo credits: DOI: 10.1038/nature05524, www.attoworld.de, E. Chowdhury (OSU)

Page 30: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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High Harmonic Generation (HHG)

Microscopic single-atom physics of HHG

Macroscopic phase-matched harmonic emission

Source: Popmintchev, Nat Photonics 4, 822 (2010), Popmintchev, Science 336, 1287 (2012) DISTRIBUTION A: Approved for public release; distribution is unlimited

2D electron wavepacket quantum simulation

Source: Luis Plaja, U Salamanca

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Direct Frequency Comb Spectroscopy in the Extreme Ultraviolet

PI: Jun Ye, U of Colorado

Source: Cingoz, Nature 482, 68 (2012)

Towards dual comb EUV spectroscopy

COMB 1

COMB 2

Beat notes!

119 nm 97 nm 82 nm 47 nm 71 nm

DISTRIBUTION A: Approved for public release; distribution is unlimited

Unpublished

Page 32: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Outline

– Microresonator-based optical frequency combs

– High peak power, ultrashort pulse laser processing of materials

– Extreme ultraviolet (EUV) comb spectroscopy

– High harmonic interferometry

– Relativistic optics

DISTRIBUTION A: Approved for public release; distribution is unlimited Photo credits: DOI: 10.1038/nature05524, www.attoworld.de, E. Chowdhury (OSU)

Page 33: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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High Harmonic Interferometry to follow chemical reactions

PI: Paul Corkum, NRC

Source: Worner, Nature 466, 604 (2010).

Br2

Br + Br

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Presenter
Presentation Notes
HHG can be used to observe a chemical reaction in real time. In this case we use an interferometric technique using high harmonic spectroscopy based on electron wavepacket recollision. The dynamics are mapped into the HHG radiation and may be possible to extract. The simple photodissociation of Molecular bromide (Br2) serves as the example. The interference of HHG recombining to the excited state or ground state allows for the extraction of the harmonic amplitude and phase of the excited level relative to the ground state. There’s a wealth of information in these plots. You can further extract the bond length as a function of time (because of quantum interference).
Page 34: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Conical intersections drive the chemistry of complex molecules

Source: Paul Corkum

PI: Paul Corkum, NRC

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Page 35: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Conical Intersection Dynamics in NO2

Source: Wörner, Science 334, 208 (2011)

PI: Paul Corkum, NRC

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Page 36: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Electronic dynamics near a conical intersection

Source: Wörner, Science 334, 208 (2011)

PI: Paul Corkum, NRC

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Page 37: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Outline

– Microresonator-based optical frequency combs

– High peak power, ultrashort pulse laser processing of materials

– Extreme ultraviolet (EUV) comb spectroscopy

– High harmonic interferometry

– Relativistic optics

DISTRIBUTION A: Approved for public release; distribution is unlimited Photo credits: DOI: 10.1038/nature05524, www.attoworld.de, E. Chowdhury (OSU)

Page 38: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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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

Relativistic ions Nonlinearity of vacuum GeV e acceleration e+e- production Nuclear reactions Relativistic plasmas Hard x-ray generation Tunnel ionization High temperature plasma formation Bright x-ray generation Nonperturbative atomic physics High order nonlinear optics Perturbative atomic physics Nonlinear Optics

DISTRIBUTION A: Approved for public release; distribution is unlimited

Presenter
Presentation Notes
Over their 50-year history, lasers have gone from producing powers of a few hundred watts to greater than a petawatt, or a quadrillion watts. Several key technological jumps have allowed researchers to compress laser beams into infinitesimally short pulses, which amplifies their peak power. “The key to understanding the underlying physics in these interactions is to realize that ordinary matter – whether solid, liquid or gas – will be rapidly ionized when subjected to high intensity irradiation. The electrons released are then immediately caught in the laser field, and oscillate with a characteristic energy (right hand column) which then dictates the subsequent interaction physics.” (Gibbon, 2005)
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Petawatt class university lasers

University of Texas, 1.1 PW University of Nebraska, 0.7 PW

University of Michigan, 0.3 PW Ohio State University, 0.5 PW

July 16, 2012 First Light

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Page 40: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Laser-driven x-ray sources

• Understanding laser-generated electron beam characteristics is the key to advancing x-ray sources.

• PIC simulations of high intensity short pulse laser interacting with structured targets yields an enhancement in the number and energy of hot electron.

• Monte Carlo simulations using the electron beam source from PIC show enhancement of x-ray production.

DISTRIBUTION A: Approved for public release; distribution is unlimited

PI: Kramer Akli, OSU

Hot electron generation

Enhanced x-ray production

Picture: Courtesy of Kwei-‐Yu Chu and Lawrence Livermore National Laboratory

Page 41: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Laser-driven x-rays generation (0.1 – 10 MeV)

• 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.

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

DISTRIBUTION A: Approved for public release; distribution is unlimited

Presenter
Presentation Notes
Thomson scattering of laser light from a relativistic electron beam is a promising route to the development of a compact mono-energetic x-ray source.
Page 42: Parra - Ultrashort Pulse (USP) Laser -- Matter Interactions - Spring Review 2013

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Laser-driven x-rays generation (0.1 – 10 MeV)

0.5 inch thick steel plate

PI: Donald Umstadter, U of Nebraska

DISTRIBUTION A: Approved for public release; distribution is unlimited

Presenter
Presentation Notes
Thomson scattering of laser light from a relativistic electron beam is a promising route to the development of a compact mono-energetic x-ray source.
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Brighter, more energetic and tunable than conventional synchrotrons

UNL 2012

Hartemann, F. V. et al. High-energy scaling of Compton scattering light sources. Physical Review Special Topics - Accelerators and Beams 8, 100702 (2005).

PI: Donald Umstadter, U of Nebraska

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(FY14 BRI) Laser-matter interactions in the relativistic optics regime

• Laser-driven electron acceleration – Laser Wakefield Acceleration: Electrons

are accelerated to gigaelectronvolt (GeV) energies over centimeters distances

– Direct Light Acceleration

• Ion acceleration – Protons and ions are accelerated to

megaelectronvolt (MeV) energies by a mechanism known as ‘target normal sheath acceleration’ (TNSA)

• X-ray radiation sources – keV to MeV x-rays via non‐linear Thomson

Scattering – Kα monochromatic emission – Bremsstrahlung broadband radiation

• Neutron sources

– Protons incident on a secondary target (e.g. Lithium) can produce MeV neutrons

• QED physics DISTRIBUTION A: Approved for public release; distribution is unlimited

Electron density distribution and generation of quasi-monoenergetic electron bunches observed in PIC simulations.

Target Sheath Normal Acceleration: Laser acceleration of protons from the back side of a microstructured target.

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Summary and outlook

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. • …

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. • …

DISTRIBUTION A: Approved for public release; distribution is unlimited