Optics, Lasers, and Remote Sensing Department 1128 Microlasers and Nonlinear Optics R. Schmitt, D....
-
Upload
tamsin-casey -
Category
Documents
-
view
215 -
download
0
Transcript of Optics, Lasers, and Remote Sensing Department 1128 Microlasers and Nonlinear Optics R. Schmitt, D....
Optics, Lasers, and Remote Sensing Department 1128
Microlasers and Nonlinear Optics
R. Schmitt, D. Armstrong, A. Smith, B. Do, and Greg Hebner
Sandia National LaboratoriesLaser, Remote Sensing, Plasma Physics and Complex Systems
Department 1128
Sandia is a multiprogram laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the United States Department of Energy’s National Nuclear Security Administration under contract DE-AC04-94AL85000.
Optics, Lasers, and Remote Sensing Department 1128
Emerging and enabling technologies require investment
• Long history of atomic and molecular physics– Spectroscopy, optical surface diagnostics
• Fiber lasers– Emerging compact high power sources.
• Frequency extension, nonlinear optics– Generate wavelength(s) matched to the mission
requirements.– Recent advances in nonlinear optics understanding are
enabling new system designs.
• Exploiting the THz region of the EM spectra– New source and detector technology is opening up the THz
spectral region.– High chemical specificity, unique and not widely published
spectral signatures, low probability of intercept, broad area imaging using SAR like processing.
• Compact, robust sources– Micro lasers, high power in a small size.– Solid-state and semiconductor laser systems
• UV solid state lasers are relatively well developed at 400 nm with 290 nm sources on the horizon. Wavelengths are a good fit to some remote sensing opportunities.
0.6 THz image
1.5 1 0.5 0 0.5 1 1.51.5
1
0.5
0
0.5
1
1.5
Optics, Lasers, and Remote Sensing Department 1128
Basic design for passively Q-switched microlaser
• fiber-coupled diode laser pump (electrical isolation)• passively Q-switched (electrical isolation)• Cr:Nd:GSGG active material (rad hard)• Cr4+:YAG Q-switch (rad hard)• simple cavity with mirror coatings directly on crystal faces• crystals bonded together to form rugged, monolithic laser• thermal lensing and gain guiding stabilize flat-flat cavity
Cr:Nd:GSGG Cr4+:YAG 1.06 moutput pulse
lens808-nm pump light
Fiber
Optics, Lasers, and Remote Sensing Department 1128
The Cr:Nd:GSGG microlaser produces ~1.6-ns-wide pulses
• Eout = 57 μJ / pulse
• ~1.6 ns (FWHM) pulse width
• raw beam Imean ~ 150 MW/cm2
• after-pulse is common– ~15 - 25% total energy in
second pulse typical
– affected by details of pump focus, pump beam quality
• linearly polarized (>100:1)-5 0 5 10 15 200
50
100
150
time (ns)
Inte
nsity
(M
W/c
m2 )
1.6 ns FWHM
near field beam intensity (MW/cm2)
output energy is scalable from μJ to 100’s of μJ
Optics, Lasers, and Remote Sensing Department 1128
The Cr:Nd:GSGG microlaser produces excellent beam quality
• The near-field beam diameter (1/e2) is 150 μm (h) x 144 μm (v).
• The far-field divergence (1/e2 full angle) is 10.2 mRad (h) x 10.6 mRad (v).
• M2 ≈ 1.05 (fitted second moment beam diameter to propagation equation)
• Eout = 57 μJ / pulse Fpeak = 0.67 J / cm2 Imax ~ 300 MW/cm2 (raw beam)
near-field image
distance (mm)
dis
tan
ce (
mm
)
0.8 0.9 1
0.7
0.8
0.9
far field image
divergence (mRad)
div
erg
ence
(m
Ra
d)
2 4 6 8 10 12
2
4
6
8
0.1
0.2
0.3
0.4
0.5
0.6
80 100 120 140 160 180 200 220 240
seco
nd
mo
me
nt d
iam
ete
r (m
m)
distance (mm)
scan through focus
Optics, Lasers, and Remote Sensing Department 1128
laser 1 2
3
Waveguides written directly into bulk material can be used for optical interconnects
• Bulk optical waveguide elements provide functional “circuits” while fibers provides the “wires”.
• Waveguide structures are a building block for buried optical computing.
• All optical interconnects are a significant safety improvement.
– Alignment and materials are very robust but if broken, can be time consuming to repair.
• Waveguides in bulk material fail based upon well understood material properties (heat, water).
Phase contrast image of a waveguide written in borosilicate glass
Ring coupling structures have been manufactured using femtosecond laser machining.
Near field mode profile of a laser written waveguide is near Gaussian.
Writing custom optical elements directly into bulk glass
Optics, Lasers, and Remote Sensing Department 1128
Tunable high pulse energy UV: A difficult problemTunable high pulse energy UV: A difficult problem
• Typical method: SFG using Nd:YAG-pumped ns OPO signal + Nd:YAG 2
– 803 nm + 532 nm 320 nm
• Many problems to overcome:– High-energy ns OPO beam quality is poor
– Nanosecond OPO’s start late and back-convert– Q-switched Nd:YAG beam quality is poor
100/ cavitysignal2pump LD F
Signal
Depletedpump
F 200
Critical direction
OPO signal far-field fluence
SPIE 5887-3
Optics, Lasers, and Remote Sensing Department 1128
Image rotating nonplanar ring “RISTRA” OPOImage rotating nonplanar ring “RISTRA” OPO
“RISTRA” cavity: Rotated Image Singly-Resonant Twisted RectAngle JOSA B 19, 1801–1814 (2002)
“RISTRA” cavity: Rotated Image Singly-Resonant Twisted RectAngle JOSA B 19, 1801–1814 (2002)
/2
Pump in
/2
Pump out
OPO: xz-cut KTP, = 58.4803(e) + 1576(o) 532(o)
10 × 10 × 15 mm3
SFG crystal Type-II BBO, = 48.2
803(e) + 532(o) 320(e)
Pulsed “self seed”
beam
UV out
Signal out
Mechanically robust. Long-term stability
No mirror adjustments
Mechanically robust. Long-term stability
No mirror adjustments
1.975"
SPIE 5887-3
Optics, Lasers, and Remote Sensing Department 1128
Near- and far-field = 803 nm signal fluence profilesNear- and far-field = 803 nm signal fluence profiles
Fresnel # D2 / L > 450 for Signal = 803 nm Fresnel # D2 / L > 450 for Signal = 803 nm
Far field: Lens with effective f/# 77Far field: Lens with effective f/# 77Near field: Image of OPO output couplerNear field: Image of OPO output coupler
SPIE 5887-3
Optics, Lasers, and Remote Sensing Department 1128
Pump depletion for seeded and unseeded oscillationPump depletion for seeded and unseeded oscillation
Self-seeded oscillation in two-crystal RISTRA~85% pump depletion
Self-seeded oscillation in two-crystal RISTRA~85% pump depletion
Free-running oscillation in two-crystal RISTRA ~37% pump depletion
Free-running oscillation in two-crystal RISTRA ~37% pump depletion
SPIE 5887-3
Optics, Lasers, and Remote Sensing Department 1128
Are flat-top beam profiles important?Are flat-top beam profiles important?
2nd-order Gaussian pump0th-order Gaussian seed
~52% pump depletion
2nd-order Gaussian pump0th-order Gaussian seed
~52% pump depletion
Flat-top pump 100 mJ flat-top seed 10 mJ
Pump depletion = 93%
Flat-top pump 100 mJ flat-top seed 10 mJ
Pump depletion = 93%
Flat-top pump 100 mJGaussian seed 10 mJPump depletion = 92%
Flat-top pump 100 mJGaussian seed 10 mJPump depletion = 92%
Flat-top pumpFlat-top seed
~ 85 % pump depletion
Flat-top pumpFlat-top seed
~ 85 % pump depletion
SPIE 5887-3
Optics, Lasers, and Remote Sensing Department 1128
Maximum extra-cavity UV energy ~ 190 mJMaximum extra-cavity UV energy ~ 190 mJ
Detector: Scientech 380101 absorberCalibration: 1 mJ/mV @ 10 HzTransmission loss: ~5%Efficiency: 1064 nm to 320 nm > 21%
Detector: Scientech 380101 absorberCalibration: 1 mJ/mV @ 10 HzTransmission loss: ~5%Efficiency: 1064 nm to 320 nm > 21%
Scientech 380101
Depleted SFG Pulses67 % depletion of 80350 % depletion of 532UV energy ~ 180 mJ
Depleted SFG Pulses67 % depletion of 80350 % depletion of 532UV energy ~ 180 mJ
SPIE 5887-3
Optics, Lasers, and Remote Sensing Department 1128
End