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Nonstoichiometric Laser Materials;
           Designer Wavelengths in
          Neodymium Doped Garnets

                              Brian M. Walsh
                             Norman P. Barnes
                            NASA Langley Research Center
                              Hampton, VA 23681 USA

International Conference on Luminescence - Lyon, France (July 7 - 11, 2008)

 National Aeronautics and                   ICL08
 Space Administration               Lyon, France (July 2008)
Prelude

“Lanthanum has only one oxidation state, the +3 state. With
 few exceptions, this tells the whole boring story about the
 other 14 lanthanides.”

G.C. Pimentel & R.D. Sprately,
quot;Understanding Chemistryquot;,
Holden-Day, 1971, p. 862




                  So much for ‘Understanding Chemistry’…
                  Let’s do some physics!

National Aeronautics and                 ICL08
Space Administration             Lyon, France (July 2008)
NASA - Laser Material Research
Activity                           Input                              Results
  Quantum                    X-ray data, refractive           Energy levels, transition
  Mechanics                  Index, crystal symmetry          probabilities, ET parameters

                           Materials meeting requirements

                             Small spectroscopic              Cross sections, lifetimes,
Spectroscopy                 Samples - inexpensive            energy levels, ET parameters


                              Best Materials Only


                             Laser quality samples               Laser demonstration,
Laser research
                             (rods, discs, fibers                 modeling


National Aeronautics and                   ICL08
Space Administration               Lyon, France (July 2008)
Remote Sensing Applications
       4X                          DIAL: CO2
                                   Backscatter Lidar: Aerosols/Clouds


            2 Micrometer
                laser           Coherent Winds:
                              Lower Troposphere & clouds



                                                  3X
                                                Noncoherent Winds:
                                                  Mid/Upper Atmosphere

            1 Micrometer
                                      2X                  Altimetry:
                laser                                  Surface Mapping
                                                        Oceanography


                                      2X                   OPO
                                                                         DIAL: Ozone
                                                                         Backscatter Lidar: Aerosols/Clouds
            0.94 Micrometer
                  laser
                              DIAL: H20


National Aeronautics and                              ICL08
Space Administration                          Lyon, France (July 2008)
What is a Nonstoichiometric Material?

    Stoichiometry - Derived from the Greek words stoikheion, meaning element
                    and metron, meaning measure.

     In Chemistry it is related to :
              Conservation of Mass
              Law of Definite Proportions
              Law of Multiple Proportions

     Stoichiometric Material - The elements composing the crystal appear as
                               ratios of integers. Example: YAG (Y3Al5O12)

     Nonstoichiometric materials are crystals composed of elements that can’t be
     represented by a ratio of whole numbers. Correct valence state, site symmetry
     and atomic size constraints are important considerations.


National Aeronautics and                ICL08
Space Administration            Lyon, France (July 2008)
Compositional Tuning



  YAG
    -to-
  YGG
                       YAG                                      YGAG

                The arrangement of atoms in a crystal structure depends on:
                the ion charge, bonding type between atoms, and atom size.
National Aeronautics and                  ICL08
Space Administration              Lyon, France (July 2008)
The Garnet Structure
                                        {Dodecahedral}
   {A3+}3[B3+]2 (C3+)3O12



             Oxygen

             Rare Earth

             Al, Ga, Fe

                            [Octahedral]                  (Tetrahedral)
Rare Earth: Y, Sc, La, Ce, Pr, Nd, Pm, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu

                                              Lanthanides
 National Aeronautics and              ICL08
 Space Administration          Lyon, France (July 2008)
Compositional Tuning Approach
• Stoichiometric Materials
     – Garnet = {A3+}3[B3+]2 (C3+)3O12
     – YAG = Y3Al2Al3O12
• Nonstoichiometric Materials
     – Compositional tuned garnets
     – YGAG = Y3GaxAl(5-x)O12 (0 < x < 2)
     – charge neutrality (correct valence)
     – atomic size (coordination number)
• Crystal dependence
     – LN3+ ion site symmetry (Group theory)
     – lattice constant variation (Crystal field)
     – chemistry&crystals (Pauling’s Rules)


 National Aeronautics and                  ICL08
 Space Administration              Lyon, France (July 2008)
Chemistry and Crystallography
    • The nature of crystals
           - Chemistry dictates bonding character (ionic and covalent)
           - Crystallography dictates geometry and structure
    • The important role of charge
           - Pauling’s theory of electronegativity (effective charges)
           - Influences bond lengths (Pauling’s Rules) J. Am. Chem. Soc. 1929
    • Size constraints - cations and anions
           - As cation size decreases, coordination number (CN) decreases
           - 1.000 = Rc/Ra (CN =12) Cubic
           - 1.000 > Rc/Ra > 0.732 (CN =8) Cubic
           - 0.732 > Rc/Ra > 0.414 (CN = 6) Octahedral
           - 0.414 > Rc/Ra > 0.225 (CN =4) Tetrahedral
           - Generally true, but many exceptions exist.

National Aeronautics and                  ICL08
Space Administration              Lyon, France (July 2008)
Ionic and Covalent Bonds
                Ionic

• Atoms (cations and anions)
  are charged particles and
  electrostatic forces hold
  structure together.

• Bond strength - ionic charge

            Covalent
• Atoms satisfy charge balance
  by sharing electrons with
  adjacent orbitals in hybrid
  or molecular orbitals.

• Bond strength - orbital overlap

 National Aeronautics and                   ICL08
 Space Administration               Lyon, France (July 2008)
Compositional Tuning Experiments


                           • Wavelength tuning
                           • Cross section ratios
                           • Inhomogeneous broadening
                           • Laser performance
                              -




National Aeronautics and                  ICL08
Space Administration              Lyon, France (July 2008)
Compositional Tuning - YGAG
        Measurement of Nd 4F3/2 → 4I9/2 transition wavelengths
                           6
                           5                                                  R2-Z1 A
                                                                              R2-Z1 B
   Gallium concentration




                                                                              R1-Z1
                           4                                                  R2-Z2
                                                                              R2-Z3
                           3                                                  R1-Z2
                                                                              R1-Z3
                           2                                                  R2-Z4
                                                                              R1-Z4 A
                                                                              R1-Z4 B
                           1                                                  R2-Z5
                                                                              R1-Z5 A
                           0                                                  R1-Z5 B

                           -1
                                860     870    880   890       900   910     920        930   940   950   960
                                                                Wavelength (nm)
                                      • Wavelength tuning is linear with Gallium concentration (x)
                                      • Wavelength can be predicted according to:
                                                 λYGAG = 1/5[(5-x)λYAG+xλYGG]
National Aeronautics and                                           ICL08
Space Administration                                       Lyon, France (July 2008)
Compositional Tuning - Mixed




National Aeronautics and           ICL08
Space Administration       Lyon, France (July 2008)
Spectral Lineshapes
Lorentzian:       (Homogeneous width)
                                                                Line shape parameter
                                                                        1 !L                    Gaussian
           1       $L                                           SV =                            Voigt
! (quot; ) =                                                               ln 2 ! G
           # (quot; % quot; 0 ) 2 + $ L
                              2                                                                 Lorentzian




Gaussian:       (Inhomogeneous width)


            1     ln 2 %( ln 2 )(quot; %quot; 0 )2   #G
                                              2
! (quot; ) =              e
           #G      $


Voigt:     (Convolution - Lorentzian&Gaussian)                                           Voigt width:
                               *
                                                     e% t
                                                            2



                               +S
                                                                                                               1/2
         SV 1          ln 2                                                              ! L # ! L2        &
! (quot; ) =                                                                       dt   !V quot;    +%      + ! G2 (
         #G $           $                2
                                             + &(quot; % quot; 0 ) ln 2 % t (
                                                                           2
                                                                                          2 $ 4            '
                               %*    V         '                    )
National Aeronautics and                                  ICL08
Space Administration                              Lyon, France (July 2008)
Inhomogeneous Broadening - YGAG
            B.M. Walsh, N.P. Barnes, et al.,
            J. Opt. Soc Am. B., 15, 2794 (1998)


                           YGAG
                     Y3GaxAl(5-x)O12




         YAG                           YGG
       Y3Al5O12                      Y3Ga5O12

National Aeronautics and                        ICL08
Space Administration                    Lyon, France (July 2008)
Inhomogeneous Broadening - YAG/YSAG

                               Nd:YAG                                                                        Nd:(YAG)0.18(YSAG)0.82
                               R1→ Z5 line (Voigt shape = 1.74)                                              R1→ Z5 line (Voigt shape = 0.37)
                               More Lorentzian than Gaussian                                                 More Gaussian than Lorentzian


                               4.0                                                                           4.0
cross section (x10 -20 cm 2)




                                                                              cross section (x10 -20 cm 2)
                               3.5 !EL =8.09 cm
                                                -1
                                                                                                             3.5                     !E L= 7.73 cm -1
                               3.0 !E G=3.85 cm -1                                                           3.0                     !E G= 17.28 cm -1
                               2.5                                                                           2.5
                                    !EV=10.02 cm -1                                                                                  !E V= 21.58 cm -1
                               2.0                                                                           2.0
                               1.5                                                                           1.5
                               1.0                                                                           1.0
                               0.5                                                                           0.5
                               0.0                                                                           0.0
                                  940   942     944    946     948   950                                        940   942    944     946     948     950
                                              Wavelength(nm)                                                                Wavelength(nm)



                   National Aeronautics and                              ICL08
                   Space Administration                          Lyon, France (July 2008)
Voigt Fitting Parameters
                   Material               !       quot;EL      quot;EG      quot;EV      Voigt      #R       $Z        %r
                                                                                             1        5
                                        (nm)     (cm-1)   (cm-1)   (cm-1)    shape
                                                                                      (x10-20cm2)
                  YSGG                  937.75   8.33     13.15    21.02    0.6666      1.7073            5.57
               YAG1/2YSGG1/2            942.59   6.76     28.50    32.89    0.1975      1.5050            6.01
               YAG3/5YSGG2/5            943.43   7.63     27.61    31.65    0.2303      1.4177            6.25
               YAG2/3YSGG1/3            944.24   8.35     26.03    28.83    0.2671      1.5780            6.30
               YAG3/4YSGG1/4            944.84   6.76     25.56    26.66    0.3432      1.4026            6.50
                  YAG                   945.87   8.09     3.85     10.02    1.7400      3.7670            7.36
                  GGG                   937.30   10.19    3.94     11.94    2.1491      1.7500            7.66
               YSAG2/3GGG1/3            940.96   7.83     28.24    32.42    0.2310      1.4761            6.08
                  YSAG                  943.63   8.15     15.52    20.13    0.43744     2.5825            4.64
                 YSAG                   943.63   8.15     15.52    20.13    0.43744     2.5825            4.64
              YAG0.18YSAG0.82           943.93   7.73     17.28    21.58    0.3721      2.3277            5.07
                  YAG                   945.87   8.09     3.85     10.02    1.7400      3.7670            7.36
                 GSAG                     -        -        -        -         -           -                -
              YAG0.45GSAG0.55           944.23   7.37     22.45    26.43    0.2733      1.9673            4.44
              YAG0.3GSAG0.050           944.51   7.59     22.55    26.66    0.2803      1.8017            4.75
                  YAG                   945.87   8.09     3.85     10.02    1.7400      3.7670            7.36
         YAG0.03(YSAG0.98GGG0.02)0.97   943.66   8.68     17.17    22.06    0.4208      2.1152            4.75
         YAG0.20(YSAG0.98GGG0.02)0.80   944.16   7.97     19.26    23.65    0.3447      2.0205            4.96
         YAG0.30(YSAG0.90GGG0.10)0.70   944.10   8.12     22.23    26.76    0.3043      1.8765            5.04
         YAG0.40(YSAG0.90GGG0.10)0.60   944.81   8.36     22.19    26.65    0.3138      1.7903            5.27


National Aeronautics and                             ICL08
Space Administration                         Lyon, France (July 2008)
YAG / YSAG Garnets
           Emission cross sections                                  Wavelength tuning
    Favorable cross section ratio is beneficial
    in limiting the deleterious effects of ASE                    YAG
    for Q-switched laser operation                               Y3Al5O12




                                                                    YAG/YSAG
                                                                 (YAG)0.18(YSAG)0.82




                                                                   YSAG
                                                                 Y3Sc2Al3O12




                           Wavelength (nm)                                     Wavelength (nm)

National Aeronautics and                             ICL08
Space Administration                         Lyon, France (July 2008)
YGAG Material Assessment

              • Continuous compositional tuning available
                     - YAG (x = 0) through YGG (x = 5)
                     - tuning is linear with Ga concentration (x)
              • Emission cross section (gain issues)
                     - Some lines are split (A and B sites)
                     - Lines are inhomogeneously broadening
                     - 1.06 to 0.94 µm cross section ratio > 20
              • Laser performance issues
                     - Slope efficiency (< 0.1%)
                     - Optical quality problems
                     - ASE (amplified spontaneous emission) problems


National Aeronautics and                      ICL08
Space Administration                  Lyon, France (July 2008)
YAGxYSAG(1-x) Material Assessment

         • Continuous compositional tuning available
                - YAG (x = 1) to YSAG (x = 0)
                - Tuning is linear with x
         • Emission cross section (gain issues)
                - No line splitting observed
                - Lines are inhomogeneously broadened
                - 1.06 to 0.94 µm cross section ratio ~ 5
         • Laser performance issues
                - Slope efficiencies > 0.2%
                - Optical quality good
                - ASE (amplified spontaneous emission) somewhat mitigated.


National Aeronautics and                   ICL08
Space Administration               Lyon, France (July 2008)
Laser Schematic
                                                      • Flashlamp pumped oscillator
     Nd operating on the                              • 5 x 55 mm laser rods
     R1 → Z5 transition.                              • Acousto-optic Q-switch
                                                      • Flashlamp pumped Amplifier


   0.94 µm resonator                         A-O
                                                                   HR 0.94
                                           Q-Switch
                                                                   HT 1.06



                           Laser       Oscillator
                            rod
                                                         Energy              Amplifier
                                                         meter
                                         PFN                                   PFN

                                                                                         Energy
                                                                                         meter
                               Laser           Output    Pickoff               Laser
    HR 0.94
                                rod            mirror                           rod
    HT 1.06


National Aeronautics and                       ICL08
Space Administration                   Lyon, France (July 2008)
Laser Performance
                               140.0
                                            Slope efficiency ~ 0.5%                   Slope efficiency ~ 0.2%
                                            Threshold ~ 26 J                         Threshold = 41 J
                               120.0        λL = 0.946 µm                            λL = 0.944 µm


                               100.0
           Laser energy (mJ)




                                80.0

                                60.0

                                40.0
                                                                                         Nd:GYAG (NM)
                                                                                         Nd:GYAG (QS)
                                20.0                                                     Nd:YAG/YSAG (NM)
                                                                                         Nd:YAG/YSAG (QS)

                                 0.0
                                       20        30      40      50       60     70        80      90         100
                                                                 Electrical energy (J)

National Aeronautics and                                          ICL08
Space Administration                                      Lyon, France (July 2008)
Summary

                   • Chemistry and crystallography
                           - Chemistry describes bonding
                           - Crystallography describes geometry
                   • Spectroscopy of materials
                           - Wavelength, cross section ratio, linewidth
                           - YAG/YSAG is material of choice.
                   • Laser demonstration
                           - Compositional tuning to 944 nm
                           - Over 100 mJ Q-switched energy




National Aeronautics and                       ICL08
Space Administration                   Lyon, France (July 2008)
NASA Langley                 Brian M. Walsh
                           Research Center              Laser Remote Sensing Branch
National Aeronautics and                    ICL08
Space Administration                                    Email: brian.m.walsh@nasa.gov
                                    Lyon, France (July 2008)
                                                        Phone: 757 864-7112

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Nonstoichiometric Laser Materials;

  • 1. Nonstoichiometric Laser Materials; Designer Wavelengths in Neodymium Doped Garnets Brian M. Walsh Norman P. Barnes NASA Langley Research Center Hampton, VA 23681 USA International Conference on Luminescence - Lyon, France (July 7 - 11, 2008) National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 2. Prelude “Lanthanum has only one oxidation state, the +3 state. With few exceptions, this tells the whole boring story about the other 14 lanthanides.” G.C. Pimentel & R.D. Sprately, quot;Understanding Chemistryquot;, Holden-Day, 1971, p. 862 So much for ‘Understanding Chemistry’… Let’s do some physics! National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 3. NASA - Laser Material Research Activity Input Results Quantum X-ray data, refractive Energy levels, transition Mechanics Index, crystal symmetry probabilities, ET parameters Materials meeting requirements Small spectroscopic Cross sections, lifetimes, Spectroscopy Samples - inexpensive energy levels, ET parameters Best Materials Only Laser quality samples Laser demonstration, Laser research (rods, discs, fibers modeling National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 4. Remote Sensing Applications 4X DIAL: CO2 Backscatter Lidar: Aerosols/Clouds 2 Micrometer laser Coherent Winds: Lower Troposphere & clouds 3X Noncoherent Winds: Mid/Upper Atmosphere 1 Micrometer 2X Altimetry: laser Surface Mapping Oceanography 2X OPO DIAL: Ozone Backscatter Lidar: Aerosols/Clouds 0.94 Micrometer laser DIAL: H20 National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 5. What is a Nonstoichiometric Material? Stoichiometry - Derived from the Greek words stoikheion, meaning element and metron, meaning measure. In Chemistry it is related to : Conservation of Mass Law of Definite Proportions Law of Multiple Proportions Stoichiometric Material - The elements composing the crystal appear as ratios of integers. Example: YAG (Y3Al5O12) Nonstoichiometric materials are crystals composed of elements that can’t be represented by a ratio of whole numbers. Correct valence state, site symmetry and atomic size constraints are important considerations. National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 6. Compositional Tuning YAG -to- YGG YAG YGAG The arrangement of atoms in a crystal structure depends on: the ion charge, bonding type between atoms, and atom size. National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 7. The Garnet Structure {Dodecahedral} {A3+}3[B3+]2 (C3+)3O12 Oxygen Rare Earth Al, Ga, Fe [Octahedral] (Tetrahedral) Rare Earth: Y, Sc, La, Ce, Pr, Nd, Pm, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu Lanthanides National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 8. Compositional Tuning Approach • Stoichiometric Materials – Garnet = {A3+}3[B3+]2 (C3+)3O12 – YAG = Y3Al2Al3O12 • Nonstoichiometric Materials – Compositional tuned garnets – YGAG = Y3GaxAl(5-x)O12 (0 < x < 2) – charge neutrality (correct valence) – atomic size (coordination number) • Crystal dependence – LN3+ ion site symmetry (Group theory) – lattice constant variation (Crystal field) – chemistry&crystals (Pauling’s Rules) National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 9. Chemistry and Crystallography • The nature of crystals - Chemistry dictates bonding character (ionic and covalent) - Crystallography dictates geometry and structure • The important role of charge - Pauling’s theory of electronegativity (effective charges) - Influences bond lengths (Pauling’s Rules) J. Am. Chem. Soc. 1929 • Size constraints - cations and anions - As cation size decreases, coordination number (CN) decreases - 1.000 = Rc/Ra (CN =12) Cubic - 1.000 > Rc/Ra > 0.732 (CN =8) Cubic - 0.732 > Rc/Ra > 0.414 (CN = 6) Octahedral - 0.414 > Rc/Ra > 0.225 (CN =4) Tetrahedral - Generally true, but many exceptions exist. National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 10. Ionic and Covalent Bonds Ionic • Atoms (cations and anions) are charged particles and electrostatic forces hold structure together. • Bond strength - ionic charge Covalent • Atoms satisfy charge balance by sharing electrons with adjacent orbitals in hybrid or molecular orbitals. • Bond strength - orbital overlap National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 11. Compositional Tuning Experiments • Wavelength tuning • Cross section ratios • Inhomogeneous broadening • Laser performance - National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 12. Compositional Tuning - YGAG Measurement of Nd 4F3/2 → 4I9/2 transition wavelengths 6 5 R2-Z1 A R2-Z1 B Gallium concentration R1-Z1 4 R2-Z2 R2-Z3 3 R1-Z2 R1-Z3 2 R2-Z4 R1-Z4 A R1-Z4 B 1 R2-Z5 R1-Z5 A 0 R1-Z5 B -1 860 870 880 890 900 910 920 930 940 950 960 Wavelength (nm) • Wavelength tuning is linear with Gallium concentration (x) • Wavelength can be predicted according to: λYGAG = 1/5[(5-x)λYAG+xλYGG] National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 13. Compositional Tuning - Mixed National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 14. Spectral Lineshapes Lorentzian: (Homogeneous width) Line shape parameter 1 !L Gaussian 1 $L SV = Voigt ! (quot; ) = ln 2 ! G # (quot; % quot; 0 ) 2 + $ L 2 Lorentzian Gaussian: (Inhomogeneous width) 1 ln 2 %( ln 2 )(quot; %quot; 0 )2 #G 2 ! (quot; ) = e #G $ Voigt: (Convolution - Lorentzian&Gaussian) Voigt width: * e% t 2 +S 1/2 SV 1 ln 2 ! L # ! L2 & ! (quot; ) = dt !V quot; +% + ! G2 ( #G $ $ 2 + &(quot; % quot; 0 ) ln 2 % t ( 2 2 $ 4 ' %* V ' ) National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 15. Inhomogeneous Broadening - YGAG B.M. Walsh, N.P. Barnes, et al., J. Opt. Soc Am. B., 15, 2794 (1998) YGAG Y3GaxAl(5-x)O12 YAG YGG Y3Al5O12 Y3Ga5O12 National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 16. Inhomogeneous Broadening - YAG/YSAG Nd:YAG Nd:(YAG)0.18(YSAG)0.82 R1→ Z5 line (Voigt shape = 1.74) R1→ Z5 line (Voigt shape = 0.37) More Lorentzian than Gaussian More Gaussian than Lorentzian 4.0 4.0 cross section (x10 -20 cm 2) cross section (x10 -20 cm 2) 3.5 !EL =8.09 cm -1 3.5 !E L= 7.73 cm -1 3.0 !E G=3.85 cm -1 3.0 !E G= 17.28 cm -1 2.5 2.5 !EV=10.02 cm -1 !E V= 21.58 cm -1 2.0 2.0 1.5 1.5 1.0 1.0 0.5 0.5 0.0 0.0 940 942 944 946 948 950 940 942 944 946 948 950 Wavelength(nm) Wavelength(nm) National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 17. Voigt Fitting Parameters Material ! quot;EL quot;EG quot;EV Voigt #R $Z %r 1 5 (nm) (cm-1) (cm-1) (cm-1) shape (x10-20cm2) YSGG 937.75 8.33 13.15 21.02 0.6666 1.7073 5.57 YAG1/2YSGG1/2 942.59 6.76 28.50 32.89 0.1975 1.5050 6.01 YAG3/5YSGG2/5 943.43 7.63 27.61 31.65 0.2303 1.4177 6.25 YAG2/3YSGG1/3 944.24 8.35 26.03 28.83 0.2671 1.5780 6.30 YAG3/4YSGG1/4 944.84 6.76 25.56 26.66 0.3432 1.4026 6.50 YAG 945.87 8.09 3.85 10.02 1.7400 3.7670 7.36 GGG 937.30 10.19 3.94 11.94 2.1491 1.7500 7.66 YSAG2/3GGG1/3 940.96 7.83 28.24 32.42 0.2310 1.4761 6.08 YSAG 943.63 8.15 15.52 20.13 0.43744 2.5825 4.64 YSAG 943.63 8.15 15.52 20.13 0.43744 2.5825 4.64 YAG0.18YSAG0.82 943.93 7.73 17.28 21.58 0.3721 2.3277 5.07 YAG 945.87 8.09 3.85 10.02 1.7400 3.7670 7.36 GSAG - - - - - - - YAG0.45GSAG0.55 944.23 7.37 22.45 26.43 0.2733 1.9673 4.44 YAG0.3GSAG0.050 944.51 7.59 22.55 26.66 0.2803 1.8017 4.75 YAG 945.87 8.09 3.85 10.02 1.7400 3.7670 7.36 YAG0.03(YSAG0.98GGG0.02)0.97 943.66 8.68 17.17 22.06 0.4208 2.1152 4.75 YAG0.20(YSAG0.98GGG0.02)0.80 944.16 7.97 19.26 23.65 0.3447 2.0205 4.96 YAG0.30(YSAG0.90GGG0.10)0.70 944.10 8.12 22.23 26.76 0.3043 1.8765 5.04 YAG0.40(YSAG0.90GGG0.10)0.60 944.81 8.36 22.19 26.65 0.3138 1.7903 5.27 National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 18. YAG / YSAG Garnets Emission cross sections Wavelength tuning Favorable cross section ratio is beneficial in limiting the deleterious effects of ASE YAG for Q-switched laser operation Y3Al5O12 YAG/YSAG (YAG)0.18(YSAG)0.82 YSAG Y3Sc2Al3O12 Wavelength (nm) Wavelength (nm) National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 19. YGAG Material Assessment • Continuous compositional tuning available - YAG (x = 0) through YGG (x = 5) - tuning is linear with Ga concentration (x) • Emission cross section (gain issues) - Some lines are split (A and B sites) - Lines are inhomogeneously broadening - 1.06 to 0.94 µm cross section ratio > 20 • Laser performance issues - Slope efficiency (< 0.1%) - Optical quality problems - ASE (amplified spontaneous emission) problems National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 20. YAGxYSAG(1-x) Material Assessment • Continuous compositional tuning available - YAG (x = 1) to YSAG (x = 0) - Tuning is linear with x • Emission cross section (gain issues) - No line splitting observed - Lines are inhomogeneously broadened - 1.06 to 0.94 µm cross section ratio ~ 5 • Laser performance issues - Slope efficiencies > 0.2% - Optical quality good - ASE (amplified spontaneous emission) somewhat mitigated. National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 21. Laser Schematic • Flashlamp pumped oscillator Nd operating on the • 5 x 55 mm laser rods R1 → Z5 transition. • Acousto-optic Q-switch • Flashlamp pumped Amplifier 0.94 µm resonator A-O HR 0.94 Q-Switch HT 1.06 Laser Oscillator rod Energy Amplifier meter PFN PFN Energy meter Laser Output Pickoff Laser HR 0.94 rod mirror rod HT 1.06 National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 22. Laser Performance 140.0 Slope efficiency ~ 0.5% Slope efficiency ~ 0.2% Threshold ~ 26 J Threshold = 41 J 120.0 λL = 0.946 µm λL = 0.944 µm 100.0 Laser energy (mJ) 80.0 60.0 40.0 Nd:GYAG (NM) Nd:GYAG (QS) 20.0 Nd:YAG/YSAG (NM) Nd:YAG/YSAG (QS) 0.0 20 30 40 50 60 70 80 90 100 Electrical energy (J) National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 23. Summary • Chemistry and crystallography - Chemistry describes bonding - Crystallography describes geometry • Spectroscopy of materials - Wavelength, cross section ratio, linewidth - YAG/YSAG is material of choice. • Laser demonstration - Compositional tuning to 944 nm - Over 100 mJ Q-switched energy National Aeronautics and ICL08 Space Administration Lyon, France (July 2008)
  • 24. NASA Langley Brian M. Walsh Research Center Laser Remote Sensing Branch National Aeronautics and ICL08 Space Administration Email: brian.m.walsh@nasa.gov Lyon, France (July 2008) Phone: 757 864-7112