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Judd-Ofelt Theory: Principles
           and Practices

                        Brian M. Walsh
                  NASA Langley Research Center


National Aeronautics and   Erice, Italy (June 2005)
Space Administration
Part I: Principles
What is the Judd-Ofelt Theory?

Based on static, free-ion and single configuration approximations:
   • static model - Central ion is affected by the surrounding
                     host ions via a ‘static’ electric field.
   • free ion model - Host environment treated as a perturbation
                       on the free ion Hamiltonian.
   • single configuration model - Interaction of electrons between
                                   configurations are neglected.

The Judd-Ofelt theory describes the intensities of 4f electrons in
solids and solutions. The remarkable success of this theory
provides a sobering testament to simple approximations.

  National Aeronautics and      International School of Atomic and Molecular Spectroscopy
  Space Administration                            Erice, Italy (June 2005)
Distribution of Citations by Year
                                   200
                                              B.R. Judd, Phys. Rev. 127, 750 (1962).
                                              G.S. Ofelt, J. Chem. Phys. 37, 511 (1962).

                                   150         ~ 2000 citations (1962-2004)
             Number of citations




                                   100




                                    50




                                    0
                                         62           72          82           92           02
                                                                 Year



National Aeronautics and                              International School of Atomic and Molecular Spectroscopy
Space Administration                                                    Erice, Italy (June 2005)
Referenced in 169 Journal Titles
          Top 20 Titles                                                  # of citations
          PHYSICAL REVIEW B                                                   127
          JOURNAL OF NON-CRYSTALLINE SOLIDS                                   108
          JOURNAL OF APPLIED PHYSICS                                            90
          JOURNAL OF CHEMICAL PHYSICS                                           83
          JOURNAL OF ALLOYS AND COMPOUNDS                                       81
          JOURNAL OF LUMINESCENCE                                               77
          JOURNAL OF PHYSICS-CONDENSED MATTER                                   58
          MOLECULAR PHYSICS                                                     57
          CHEMICAL PHYSICS LETTERS                                              48
          OPTICAL MATERIALS                                                     43
          JOURNAL OF THE OPTICAL SOCIETY OF AMERICA B                          38
          JOURNAL OF PHYSICS AND CHEMISTRY OF SOLIDS                            35
          PHYSICA STATUS SOLIDI A-APPLIED RESEARCH                              33
          OPTIKA I SPEKTROSKOPIYA                                               30
          IEEE JOURNAL OF QUANTUM ELECTRONICS                                   27
          PHYSICS AND CHEMISTRY OF GLASSES                                      27
          OPTICS COMMUNICATIONS                                                 26
          SPECTROCHIMICA ACTA PART A                                            26
          INORGANIC CHEMISTRY                                                   24
          JOURNAL OF THE AMERICAN CERAMIC SOCIETY                               19



National Aeronautics and     International School of Atomic and Molecular Spectroscopy
Space Administration                           Erice, Italy (June 2005)
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
http://www.chem.ox.ac.uk/icl/heyes/LanthAct/I1.html
( some amusing mnemonics for the Lanthanides and Actinides)



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

National Aeronautics and           International School of Atomic and Molecular Spectroscopy
Space Administration                                 Erice, Italy (June 2005)
Ions in Solids
              Solids
              • insulators (not semiconductors)
              • bandgaps are > 5ev (VUV photon)
              • produce a crystal field
              Ions
              • replace host ions substitutionally
              • transition metal and lanthanide series
              • unfilled electronic shells
              • Stark splitting from crystal field
              • optical transitions occur within bandgap
              Examples
              • Nd:Y3Al5O12 - Er:fiber - Cr:Al2O3 (Ruby)

National Aeronautics and    International School of Atomic and Molecular Spectroscopy
Space Administration                          Erice, Italy (June 2005)
Atomic Structure of Laser Ions




National Aeronautics and   International School of Atomic and Molecular Spectroscopy
Space Administration                         Erice, Italy (June 2005)
Atomic Interactions
                             4f 95d                                          Hc >> Hso (LS-coupling)
                                                                             Hc << Hso (jj-coupling)
                                                                             Hc ≈ Hso (Intermediate coupling)



                                                                                            !1 !2 !3 !4
                                                    5S
                                                                        5I
                              4f10                  5F                       4
                                                                        5I
                                                                          5
                                                    5I                  5I
                       Configurations                                      6
                       Ho = central field                               5I
                                                Terms 2S+1 L               7
                       (Electrons in field                              5I
                                                Hc = Coulomb field         8
                        of the nucleus)
                                                (Mutual repulsion    Levels 2S+1L J
                                                 of electrons)
                                                                     Hso = spin orbit
                                                                     (Coupling between
                                                                     spin and orbital       Stark Levels
                                                                     angular momentum)      Vo = crystal field
                           Ho >Hc , Hso >Vo                                                 (Electric field of host)



                Hund’s Rules*: F. Hund, Z. Phys. 33, 345 (1925)
                1.) Lowest state has maximum 2S+1
                2.) Of these, that with largest L will be lowest
                3.) Shells < 1/2 full (smallest J is lowest), Shells > 1/2 full (largest J is lowest)

                *These rules apply only to the ground state, not to excited states.

National Aeronautics and                      International School of Atomic and Molecular Spectroscopy
Space Administration                                            Erice, Italy (June 2005)
Transitions and Selection Rules
• Not all transitions between atomic states that are energetically
  feasible are quot;allowed”.
• Forbidden transitions are “forbidden*” to first order, which
  means they may occur in practice, but with low probabilities.
• Selection rules for transitions depend on type of transition
    – Electric dipole (E1)
    – Electric quadrupole (E2)
    – Magnetic dipole (M1)
• Wavefunctions must have correct parity (Laporte’s rule)
• Symmetry plays a role in selection rules
    – Vibronics, crystal field, other perturbing effects.
* This nomenclature is historically embedded, although not entirely accurate.
National Aeronautics and    International School of Atomic and Molecular Spectroscopy
Space Administration                          Erice, Italy (June 2005)
Multipole Selection Rules
   !       !                              Electric dipole operator (E1)
   P = quot;e! ri                                           (odd operator)
                       i
  !     equot;   !      !                   Magnetic dipole operator (M1)
  M =quot;     ! I i + 2si
       2mc i                                           (even operator)

 !        ! ! !
      1
 Q = $ ! k # ri quot;ri
      2 i
                           ( )              Quadrupole operator (E2)
                                                       (even operator)



                                 S            L               J (No 0 ↔ 0) Parity
Electric Dipole                ΔS = 0 ΔL= 0, ±1      ΔJ = 0, ±1     opposite
Magnetic dipole                ΔS = 0 ΔL= 0          ΔJ = 0, ±1     same
Electric quadrupole            ΔS = 0 ΔL = 0, ±1, ±2 ΔJ = 0, ±1, ±2 opposite


National Aeronautics and    International School of Atomic and Molecular Spectroscopy
Space Administration                          Erice, Italy (June 2005)
A Brief History of Parity
                Otto Laporte (1902-1971) empirically discovered the law of parity
                conservation in physics. He divided states of the iron spectrum into two
                classes, even and odd, and found that no radiative transitions occurred
                between like states: O.Laporte, Z. Physik 23 135 (1924).

                Eugene Paul Wigner (1902-1995) explicitly formulated the law of parity
                conservation and showed that Laporte’s rule is a consequence of the
                invariance of systems under spatial reflection. E. P. Wigner, “Gruppentheorie
                und Ihre Anwendung auf die Quantenmechanik der Atomspektren”. Braunschweig:F. Vieweg
                und Sohn, 1931. English translation by J. J. Griffin. New York: Academic Press, 1959.

Wavefunctions are classified as even (+1 parity) or odd (-1 parity). By convention,
the parity of a photon is given by the radiation field involved: ED ( -1), MD (+1).
For mathematical reasons, the parity of any system is the product of parities of the
individual components. If the initial and final wavefunction have same parity (±1):
        ED: ±1 = (-1)(±1) Parity is NOT conserved. Transition is forbidden!
        MD: ±1 = (+1)(±1) Parity IS conserved. Transition is allowed!
Laporte Rule: States with even parity can be connected by ED transitions only with
states of odd parity, and odd states only with even ones.
National Aeronautics and           International School of Atomic and Molecular Spectroscopy
Space Administration                                 Erice, Italy (June 2005)
Parity Selection Rules
   ED allowed                 ED forbidden
   MD forbidden               MD allowed
   EQ forbidden               EQ allowed
   s → p                       s → s
   p → d                       d → d
   d → f                       p → p
   f → g                       f → f
   s → f                       g → g
   p → g



Orbital                                               s          p         d          f          g
Angular momentum                     !                0          1         2          3          4
!- odd # electrons
                               ! = ( quot;1)# i
                                          !           even       odd       even       odd        even
!- even # electrons                     i
                                                      odd        even      odd        even       odd


   National Aeronautics and              International School of Atomic and Molecular Spectroscopy
   Space Administration                                    Erice, Italy (June 2005)
Historical Perspective I
• J.H. Van Vleck - J. Phys. Chem. 41, 67-80 (1937)
    (The Puzzle of Rare-Earth Spectra in Solids)
     – Why are spectral lines in rare earths observable?
     – Electric dipole(E1), magnetic dipole(M1), quadrupole(E2)?
     – Concludes a combination is possible.
     – Suggests that crystal field makes mixed parity states (E1).
• L.J.F. Broer, et al., - Physica XI, 231- 250 (1945)
    (On the Intensities and the multipole character in the
     spectra of the rare earth ions)
     – Considers all mechanisms.
     – Concludes quadrupole radiation is too weak.
     – Considers magnetic dipole , but as a special case only.
     – ED transitions dominate as suggested by Van Vleck!
National Aeronautics and   International School of Atomic and Molecular Spectroscopy
Space Administration                         Erice, Italy (June 2005)
Historical Perspective II
• G. Racah - Phys. Rev. 76, 1352 (1949)
   (Theory of Complex Spectra IV)
    – Applies group theory to problems of complex spectra
    – Creates the tools required to make detailed spectroscopic
      calculations involving states of the 4f shell.
    – Revolutionizes the entire subject of rare earth spectroscopy.
• Subsequent developments
    – Racah’s methods applied to crystal field theory.
    – Ideas of Racah applied to transition metal ions (Griffiths).
    – Practical calculations assisted by computer generated
      tables of angular momentum coupling coefficients.
• By 1962 the stage was set for the next major development:
  The Judd-Ofelt theory of the intensities of RE transitions.
 National Aeronautics and   International School of Atomic and Molecular Spectroscopy
 Space Administration                         Erice, Italy (June 2005)
The Stage is Set


  “I suggest that the coincidence of discovery was indicative
  that the time was right for the solution of the problem.”

            Brian G. Wybourne
            “The fascination of rare earths - then, now and in the future”
            Journal of Alloys and Compounds 380, 96-100 (2004)




National Aeronautics and       International School of Atomic and Molecular Spectroscopy
Space Administration                             Erice, Italy (June 2005)
Judd and Ofelt Publish (1962)




National Aeronautics and   International School of Atomic and Molecular Spectroscopy
Space Administration                         Erice, Italy (June 2005)
States of an Ion in the Crystal
The Crystal field, V, is considered as a first order perturbation
that ‘admixes’ in higher energy opposite parity configurations:



                                                          }
                                     quot;a V quot;#
                      ! a = quot;a + %               quot;#
                                #    Ea $ E#                       Mixed Parity
                                     quot;# V quot;b                          States
                      ! b = quot;b + %               quot;#
                                #    Eb $ E#
                                                   !             !
                  !       ( +a V +*
                          quot;                    + * P +b      + a P + * + * V +b %
                                                                                quot;
               ,a P,b = !'                                 +                    $
                        * quot;
                          &      Ea ) E *                          Eb ) E*      quot;
                                                                                #
 φa and φb have the same parity (4f N states)
 φβ has opposite parity (4f N-15d states)
 V is the crystal field (treated as a perturbation)
  !
 P is the electric dipole operator
National Aeronautics and       International School of Atomic and Molecular Spectroscopy
Space Administration                             Erice, Italy (June 2005)
Tensor Forms of Operators
Racah defined irreducible tensors, C(k), which transform as
spherical harmonics, having the components:
                                     quot; 4! %
                                                  1/2

                             Cq )
                              (k
                                    =$
                                     # 2k + 1 '
                                                        Ykq
                                              &

The position vector r is a tensor of rank 1, defined as r = rC (1)

                           Dipole Operator                         Crystal Field
                             !       !
Standard Form                P = quot;e! ri                       V = ! ! Akq ri kYkq (quot; i , # i )
                                           i                         i   kq

                           Dq = !equot; ri #Cq %                   D p ) = ! Atp ! rit quot;C p ) $
                            (1)          (1)                     (t                   (t
Tensor Form                            $     &          i                          #      %   i
                                       i                                 tp    i

   Note: t is odd since only odd order terms contribute to parity mixing.
   Even order terms are responsible for energy level splitting.
National Aeronautics and        International School of Atomic and Molecular Spectroscopy
Space Administration                              Erice, Italy (June 2005)
J-O Theory Assumptions 1&2
1.) The states of φβ are completely degenerate in J.

    Assume an average energy for the excited configuration
    above the 4fN, that is, the 4f N-15d.
2.) The energy denominators are equal ( Ea-Eβ = Eb-Eβ )
    Assume that the difference of average energies, ΔE(4f-5d),
    is the same as the difference between the average energy
    of the 4f N-15d and the energy of the initial and final states
    of the 4fN
    These assumptions are only moderately met, but offer a
    great simplification. Otherwise, the many fold sum of
    perturbation expansions is not suitable for numerical
    applications.
National Aeronautics and   International School of Atomic and Molecular Spectroscopy
Space Administration                         Erice, Italy (June 2005)
4f and 4f N                  N-15d           configurations
                   35
                                 4fn configuration
                   30            4fn-15d1 configuration

                   25
Energy(×104cm-1)




                   20                                                                         Lanthanides in YLF:

                                                                                              K. Ogasawara et al.,
                   15                                                                          J. Solid State Chem.
                                                                                              vol. 178, 412 (2005

                   10

                    5

                    0
                        Ce   Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb
                        58   59 60 61 62 63 64 65 66 67 68 69 70
                                    Atomic Number & Symbol
National Aeronautics and                     International School of Atomic and Molecular Spectroscopy
Space Administration                                           Erice, Italy (June 2005)
Advantages of the Assumptions
 I.) Energy denominators can be removed from the summations
II.) Closure can be used ( the excited configuration forms a
     complete orthonormal set of basis functions)
                                         #!       quot;   !quot; = 1
                                              quot;
III.) Angular parts of the electric dipole operator and crystal field
                Cq = ! C (1) !! U q
                 (1)              (1)
                                                  and    C p ) = ! C (t ) !! U p )
                                                           (t                  (t



      can be combined into an effective tensor operator
                                                        %t 1 quot; ( + t 1 quot; . (quot; )
      U U (1)    (t )
                        = # (!1) 1+t + quot; +Q
                                              (2 quot; + 1) &        )-        0 UQ
                                                        ' ! ! !$ * , p q Q /
          q      p
                            quot;Q

The 3j symbol ( ) is related to the coupling probability for two angular momenta.
The 6j symbol { } is related to the coupling probability for three angular momenta.
The Wigner 3-j and 6-j symbols are related to Clebsch-Gordon coupling coefficients.

 National Aeronautics and            International School of Atomic and Molecular Spectroscopy
 Space Administration                                  Erice, Italy (June 2005)
Reduced Matrix Elements
 Nevertheless, combining the tensors for the electric dipole
 and crystal field terms in a combined tensor operator, UQ! ) ,
                                                          (

 can be simplified further by the Wigner-Eckart Theorem:
                                               Geometry              Physics
                                           (transformations)        (Dynamics)
                                           % J      quot; J# ( N
   f N! JM UQquot; ) f N! # J #M # = ($1)J $ M '
            (
                                                           f ! J U ( quot; ) f N! # J #
                                           & $M     Q M #*
                                                         )

 The matrix elements on the right side have been tabulated:
 “Spectroscopic Coefficients of the p N, d N, and f N Configurations,”
 C.W. Nielson and G.F. Koster, M.I.T Press, Cambridge, MA (1963).

 The 3-j and 6-j symbols have also been tabulated:
 “The 3-j and 6-j symbols,” M. Rotenberg, R, Bivens, N. Metropolis,
  J.K. Wooten Jr., Technology Press, M.I.T, Cambridge, MA (1959).

National Aeronautics and     International School of Atomic and Molecular Spectroscopy
Space Administration                           Erice, Italy (June 2005)
“Full Judd-Ofelt Theory”
    !                                                   1 *                    * J( $
                    () 1)J )M )Q (2* + 1)AtpY (t , * )'
                                                                   t $' J
, a P , b = )e!!                                      %
                                                      %q Q           quot;%             quot; + a U ( * ) +b
              tp *Q                                   &            p quot;% ) M
                                                                     #&        Q M (quot;
                                                                                    #

                                     n! r nquot;!quot; nquot;!quot; r t n!                        &1 t ! )
   Where,           Y (t, ! ) = 2%                         ! C (1) !quot; !quot; C (t ) ! '        *
                               n!          Ea # E$                                ( ! !quot; ! +


This is the “Full Solution” of the Judd-Ofelt Theory. This form
can be used to find electric dipole matrix elements between mixed
parity states for individual Stark level to Stark level transitions.

Application of “Full Judd-Ofelt Theory”:
R.P. Leavitt and C.A. Morrison, “Crystal-field Analysis of triply Ionized lanthanum
trifluoride. II. Intensity Calculations.” Journal Of Chemical Physics, 73, 749-757 (1980).



   National Aeronautics and           International School of Atomic and Molecular Spectroscopy
   Space Administration                                 Erice, Italy (June 2005)
J-O Theory Assumptions 3&4
Oscillator strength (f-number) for electric dipole transition:
                                                2
                 8+ mc     2
                                   (n + 2%
                                        2                   !
                                                    !
                                                                            2
          f =                     n&
                                   & 3n ##              )JM P ) quot;J quot;M quot;
              3quot;* (2 J + 1)e 2     '     $
                 L.J.F. Broer, et al., - Physica XI, 231- 250 (1945)

3.) Sum over Stark split J-levels
   (Assumes all Stark levels equally populated)
      $ J      ! Jquot; ' $ J       !quot; J quot; '    1
 *&            Q M quot; ) & #M
                                         =      + +
                                Qquot; M quot; ) 2 ! + 1 !! quot; QQ quot;
                                                                  M = -J, -(J-1), …, 0, …, (J-1), J
 MM quot; % #M           (%                (


4.) Sum over dipole orientations
    (Assumes optically isotropic situation)
   quot;1 !           t % quot;1 !     t) %   1
 ($ q Q           p' $ q Q
                                    =     * *
                               p) ' 2t + 1 tt ) pp )
                                                                 Q = 0 (π-polarized, E ⊥ c)
 Q #                &#            &                              Q = ±1 (σ-polarized, E || c)

National Aeronautics and           International School of Atomic and Molecular Spectroscopy
Space Administration                                 Erice, Italy (June 2005)
“Approximate Judd-Ofelt Theory”
                                   2                                                  2
      8! mc 2
                 # n + 2&  2                                                    Atp
                                            ) ))
                                                                                                                        2
                                                                                                            (quot; )
f =             n%                                              (2 quot; + 1)                 Y (t, quot; ) * a U
                                                                                           2
                                                                                                                   *b
    3hquot; (2J + 1) $ 3n ( '              quot; = 2, 4,6 p t =1, 3,5               (2t + 1)
                                                                                2
                                                                          Atp
Defining Ωλ as:                !quot; = (2 quot; + 1)#                    # (2t + 1)Y 2 (t, quot; )            Judd-Ofelt
                                                            p   t =1, 3,5
                                                                                                   parameters
                                       2
      8! 2 mc    # n2 + 2 &
                                             +
                                                                                2
                                                                   (quot; )
f =             n%                                      )quot; * a U          *b              Oscillator
    3hquot; (2J + 1) $ 3n (   '                quot; = 2, 4,6                                     strength


            $
                                                        2
                                  (quot; )
SED =                  !quot; # a U             #b              is called the Linestrength.
          quot; = 2, 4,6


This is the “Approximate Solution” of the Judd-Ofelt theory.
It can be used to find electric dipole matrix elements between
mixed parity states for manifold to manifold transitions.
National Aeronautics and            International School of Atomic and Molecular Spectroscopy
Space Administration                                  Erice, Italy (June 2005)
Judd-Ofelt Parameters
In principle, the Judd-Ofelt parameters can be calculated
“ab-initio” if the crystal structure is known, and hence, Atp:
                                                               2
                                                         Atp
                              !quot; = (2 quot; + 1)#    #                Y 2 (t, quot; )
                                            p   t =1, 3,5 (2t + 1)


                            n! r nquot;!quot; nquot;!quot; r t n!                 &1 t ! )
     Y (t, ! ) = 2%                               ! C !quot; !quot; C ! '
                                                     (1)     (t )
                                                                           *
                      n!          Ea # E$                         ( ! !quot; ! +

                          # ! 1 !! &
       ! C (1) !! = (quot;1)! %          ( 2! + 1)1/2 ( 2!! + 1)1/2
                          $0 0 0(  '
                            # !! t ! &
       ! C (t ) !! = (quot;1)!! %          ( 2!! + 1)1/2 ( 2! + 1)1/2
                            $ 0 0 0( '
3-j and 6-j symbols can be calculated for ! = 3 (4f ) and !! = 2 (5d)
Radial integrals between configurations and crystal field components, Atp, are difficult
to calculate. Instead, Judd-Ofelt parameters are usually treated as phenomenological
parameters, determined by fitting experimental linestrength data.
 National Aeronautics and            International School of Atomic and Molecular Spectroscopy
 Space Administration                                  Erice, Italy (June 2005)
Intermission

 “The two papers of 1962 represent a paradigm that has
 dominated all further work on the intensities of rare earth
 transitions in solutions and solids up to the present time.”

               Brian G. Wybourne
               “The fascination of rare earths - then, now and in the future”
               Journal of Alloys and Compounds 380, 96-100 (2004).




National Aeronautics and        International School of Atomic and Molecular Spectroscopy
Space Administration                              Erice, Italy (June 2005)
Part II: Practices
The Judd-Ofelt theory, in practice, is used to determine a set
of phenomenological parameters, Ωλ (λ=2,4,6), by fitting the
experimental absorption or emission measurements, in a
least squares difference sum, with the Judd-Ofelt expression.
     Absorption                                        Least Squares             Judd-Ofelt
                              Collect Matrix
    Measurements                                          Fitting                Parameters
                                Elements
         #
                                                          ( )=0
                                                         ! quot;2
                                                                                     Ωλ
      manifold
                 ! (quot; )d quot;      |<U(λ)>|2                 !# k


                                                             Transition
                                   τr and β                 Probabilities
                                                                 AJ′J


The Judd-Ofelt parameters can then be used to calculate the
transition probabilities, AJ′J, of all excited states. From these,
the radiative lifetimes, τr, and branching ratios, β, are found.
National Aeronautics and          International School of Atomic and Molecular Spectroscopy
Space Administration                                Erice, Italy (June 2005)
Selection Rules Revisited
! j1   j2     j3 $            #1 t ! &                ! j1     j2     j3 $            $ J     ! Jquot; '
quot;                %=0          $        '              #m                   =0
#! 1   !2     !3 &              ! !quot; ! (              quot; 1      m2     m3 &
                                                                         %            & #M
                                                                                      %       Q M quot;)
                                                                                                   (
                              %
Unless:                                               Unless:                            J! quot; J # $
                                ! = 2, 4, 6
ji ! 0                                                ji ! 0
                                t = 1, 3, 5, 7                                              !J quot; 6
!i ! 0                                                mi quot; ji
                                    ! quot;1+ t                                                 !L quot; 6
 j1 quot; j2 # j3 # j1 + j2                               m1 + m2 + m3 = 0
                                                                                            !S = 0
                                   !! quot; ! # 1         ji , mi (1, 1/2 integer)
 ! 2 quot; ! 3 # j1 # ! 2 + ! 3                                                           J = 0 : J # $ even
                                   Only d or g         j1 # j2 quot; j3 quot; j1 + j2
 ! 1 quot; ! 3 # j2 # ! 1 + ! 3        orbitals can                                       J # = 0 : J $ even
                                   mix parity
 ! 1 quot; ! 2 # j3                New Selection Rules From Judd-Ofelt Theory

                               S                  L                    J (No 0 ↔ 0)          Parity

 Electric Dipole              ΔS = 0       ΔL ≤ 6   ΔJ ≤ 6                   opposite
                                                    ΔJ = 2,4,6 (J or J′ = 0)
 Magnetic dipole              ΔS = 0 ΔL = 0         ΔJ = 0, ±1               same
 Electric quadrupole          ΔS = 0 ΔL = 0, ±1, ±2 ΔJ = 0, ±1, ±2           opposite

   National Aeronautics and             International School of Atomic and Molecular Spectroscopy
   Space Administration                                   Erice, Italy (June 2005)
Judd-Ofelt Analysis I
                                                                                        Matrix Forms
              3ch(2J + 1) # 3 &
                                                      2

         Sm =
                8! e quot;
                  3 2
                         n% 2
                          $ n + 2(
                                 '                           *
                                                          manifold
                                                                     ) (quot; )d quot;              S jm
                                                                                                   Components of
                                                                                                   1 x N matrix
                                                                                  3

                     $                                                     S = quot; M ij !i
                                                      2
                                          (quot; )
         SED =                 !quot; # a U          #b                          t
                                                                             j
                  quot; = 2, 4,6                                                     i =1
                                                                                            N = number of tramsitions
 Mij - components of N x 3 matrix for square matrix elements of U ( 2 ), U ( 4 ), U (6 )
 Ωi - components of 1 x 3 matrix for Judd-Ofelt parameters Ω 2, Ω 4, Ω 6
                                    2
          N
           % m 3          (
  ! = $ ' S j quot; $ M ij #i *
   2
                                        LEAST SQUARES DIFFERENCE
      j =1 &    i =1      )

   ( ) = $2
 ! quot;2            N
                          & m 3             )                                                         (
                                                                                             !(0) = M †M    )
                                                                                                                quot;1


  !# k
                % '  M jk ( S j $ % M ij #i + = 0 MINIMIZED
                                            *
                                                                                                                     M †Sm
                j =1              i =1
                                                                                        Judd-Ofelt Parameters
                                                                                            1 x 3 Matrix

National Aeronautics and                International School of Atomic and Molecular Spectroscopy
Space Administration                                      Erice, Italy (June 2005)
Judd-Ofelt Fit (Ho:YLF)
                  6.0
                          Visible absorption spectrum of Ho:YLF
                  5.0
!ab (10-20 cm2)


                                   (! and quot; polarization)
                  4.0
                  3.0
                  2.0
                  1.0
                  0.0
                        280     330       380       430     480        530        580       630       680
                                                       Wavelength (nm)




National Aeronautics and                        International School of Atomic and Molecular Spectroscopy
Space Administration                                              Erice, Italy (June 2005)
Judd-Ofelt Analysis II
With the Judd-Ofelt parameters, the ED transition probability
for any excited state transition (J´→ J) can be calculated

                    64quot; 4 e2     * $ n2 + 2 ' 2             -      Transition probability
      A J !J   =               3 ,n &           SED + n SMD /
                                                       2

                 3h(2 J ! + 1)# , %
                                 +      3 ) (               /
                                                            .
                                                                   (Einstein A coefficient)

      1
         = # AJ quot;J          Radiative lifetime
      !r   J               (natural decay time)

                  AJ quot;J             Branching ratio
      ! J quot;J =
                 # AJ quot;J    (fraction of total photon flux)
                  J


MD transitions are normally orders of magnitude smaller than ED transitions. Since
ED transitions for ions in solids occur as a result of a perturbation, some MD
transitions will make significant contributions.

National Aeronautics and          International School of Atomic and Molecular Spectroscopy
Space Administration                                Erice, Italy (June 2005)
Magnetic Dipole Contributions
 Magnetic dipole contributions can be easily calculated using an
 appropriate set of intermediate coupled wavefunctions for
 transitions obeying the selection rules ( ΔS = 0, ΔL= 0, ΔJ = 0, ±1).
                                   2
                    ' quot; $                        !    !
                                       f n [SL]J L + 2S f n [S !L!]J !
                                                                             2
            S MD   =%     quot;                                                          MD Linestrength
                    & 2mc #
                                                                                                   1/ 2    LS-coupled
                                                      2 - (J + 1) . (L . S ) * !
        !     ! n              '-
                               !
                                                                 2          2
                                                                               *$
f [SL]J L + 2 S f [S /L/]J / = &+(S + L + 1) . (J + 1) +                                                  matrix elements
 n                                          2
                                                                              ((#
                               !+
                               %,                       ,       4(J + 1)      )(!
                                                                               )quot;                         G.H. Shortley
                                                                                                    Phys. Rev. 57, 225 (1940)

                                                                Intermediate coupled wavefunctions
           f n [SL]J = ! C ( S, L ) f n SLJ
                              SL
                                                                  (linear combination of LS states)

           !    ! n                                                                  quot;    ! n
   f [SL]J L + 2S f [S quot;Lquot;]J quot; =
    n
                                               !          C (S , L )C (S , L ) f SLJ L + 2S f S quot;Lquot;J quot;
                                                                             n

                                              SL ,S quot;Lquot;

                                                                     Intermediate coupled matrix elements

   National Aeronautics and                   International School of Atomic and Molecular Spectroscopy
   Space Administration                                         Erice, Italy (June 2005)
Judd-Ofelt Results (Ho:YLF)




National Aeronautics and   International School of Atomic and Molecular Spectroscopy
Space Administration                         Erice, Italy (June 2005)
Testing the J-O theory
    Branching ratios can be measured directly from emission
    spectra. Use reciprocity of emission and absorption to
    indirectly “measure” the radiative lifetimes.

                           Z!     *$      hc '  -
 ! em ( quot; ) = ! ab ( quot; )      exp ,& EZL # ) kT /                          D.E. McCumber
                           Zu     +%      quot;(    .                    Phys. Rev. 136, A954 (1964).


    By comparing the measured emission cross section
                quot;5                       3I& ( quot; )
 ! (quot; ) =                                                                     P. Moulton
          8# cn 2 ($ r / % ) + ' 2I ! ( quot; ) + I # ( quot; ) ) quot; d quot;
                               (                        *
                                                                   J. Opt. Soc Am. B 3, 131 (1986).



   with the emission cross section derived from absorption, the
   quantity (τr/β) can be determined and the radiative lifetime
   extracted for comparison with the Judd-Ofelt theory

National Aeronautics and                 International School of Atomic and Molecular Spectroscopy
Space Administration                                       Erice, Italy (June 2005)
Reciprocity of Ho:YLF (5I7 ↔ 5I8)




National Aeronautics and   International School of Atomic and Molecular Spectroscopy
Space Administration                         Erice, Italy (June 2005)
Accuracy of J-O theory (Ho&Tm)
          Results are somewhat better
          in Ho3+ than Tm3+. Overall,
          the accuracy of the Judd-Ofelt
          theory is quite good, despite
          the approximations used.




National Aeronautics and       International School of Atomic and Molecular Spectroscopy
Space Administration                             Erice, Italy (June 2005)
Special Case I:                         Pr3+          ion
                  (A failure of the standard Judd-Ofelt theory?)
Pr3+ ions suffer from several problems in applying Judd-Ofelt theory
      1.) Large deviations between calculations and experiment observations.
      2.) Negative Ω2 sometimes obtained, in opposition with definition.
      3.) Ω2, Ω4, Ω6 highly dependent on transitions used in fit.
These inconsistencies are usually explained by the small energy gap
(~ 50,000 cm -1) between the 4f N and 4f N-15d configurations in Pr3+
 Solutions:
     1.) Modify the standard theory: quot;!# = quot;# &1 + ( $Eij % 2E4 f ) ( E5d % E4 f ) (
                                              '
                                                                       0
                                                                                   )
                   E.E. Dunina, et al., Sov. Phys. Solid State 32, 920 (1990).
     2.) Remove 3H4 → 3P2 from the fit, or augment fit with fluorescence β’s
                   R.S.Quimby, et al., J. Appl. Phys. 75, 613 (1994).
                                                                                                          2
                                                                            N
                                                                               +%               (     .
     3.) Use normalized least squares fitting procedure:              ! = $ -' S jm quot; $ M ij #i * ! i 0
                                                                       2

                                                                          j =1 , &    i         )     /
                   P. Goldner, et al., J. Appl. Phys. 79, 7972 (1996).
   National Aeronautics and         International School of Atomic and Molecular Spectroscopy
   Space Administration                               Erice, Italy (June 2005)
Special Case II:                            Eu3+          ions
                            (Beyond the standard Judd-Ofelt theory)

 The ED transitions 7F0 ↔ 5DJodd, 7FJodd ↔ 5D0 and 7F0 ↔ 5D0 in Eu3+ are
   “forbidden” in standard JO-theory. They violate the selection rules:
     • ΔS = 0                                  G.W. Burdick, J. Chem Phys. 91 (1989).
     • If J = 0 then J′ is even
     • If J′ = 0 then J is even                M. Tanaka, Phys. Rev. B, 49, 16917 (1994).
     •0↔0
                                               T. Kushida, Phys. Rev B, 65, 195118 (2002).
 These transitions are primarily MD, but all three do occur as ED with low intensity
    in the spectra of some materials.

 This implies that the standard Judd-Ofelt theory is incomplete. These ‘forbidden’
    transitions provide an ideal testing ground for extensions to the standard theory.

 What mechanism or mechanisms could be responsible? Are they meaningful!

 National Aeronautics and          International School of Atomic and Molecular Spectroscopy
 Space Administration                                Erice, Italy (June 2005)
Europium’s Peculiar Properties
                                              (Adventures of The Atom)
        The Atom, Issue 2
          August 1962
          (DC Comics)
 Coincident with the publications of
 Judd and Ofelt, who were both also
 interested in Europium’s peculiar
 properties.




National Aeronautics and    International School of Atomic and Molecular Spectroscopy
Space Administration                          Erice, Italy (June 2005)
Extensions I
 1) J-mixing:
       The wavefunctions of the J ≠ 0 state are mixed into the J = 0 state by even
       parity terms of the crystal field. Explains the radiative transition 7F3 ↔ 5D0
         in Eu3+. J.E. Lowther, J. Phys. C: Solid State Phys. 7, 4393 (1974).

 2) Electron correlation:
       Electrostatic interaction between electrons is taken into account. Goes
       beyond the single configuration approximation and electron correlation
       within the 4f shell is incorporated by configuration interactions. Contributes
       to “allowing” the “forbidden” 0 ↔ 0 transitions such as 7F0 ↔ 5D0 in Eu3+.
       K. Jankowski, J. Phys B: At. Mol. Phys. 14, 3345 (1981).

 3) Dynamic coupling:
      The mutual interaction of the lanthanide ion and the crystal environment
      are taken into account. Goes beyond the static coupling model. Explains
      hypersensitive transitions (transitions highly sensitive to changes in
      environment). M.F. Reid et al., J. Chem Phys. 79, 5735 (1983).


National Aeronautics and       International School of Atomic and Molecular Spectroscopy
Space Administration                             Erice, Italy (June 2005)
Extensions II
4) Wybourne-Downer mechanism:
    Involves spin-orbit interaction among states of the excited configurations,
    leading to an admixing of spin states into the 4f N configuration. This
    accounts for the observed spin “forbidden” transitions ΔS = 1
    B.G. Wybourne, J. Chem. Phys. 48, 2596 (1968).
    M.C. Downer et al., J. Chem. Phys 89, 1787 (1988).

5) Relativistic contributions:
     Relativistic treatment of f → f transitions in crystal fields. Reformulation of
     crystal field and operators in relativistic terms. Importance unknown.
     L. Smentek, B.G. Wybourne, J. Phys. B: At. Mol. Opt, Phys. 33, 3647 (2000).
     L. Smentek, B.G. Wybourne, J. Phys. B: At. Mol. Opt, Phys. 34, 625 (2001).


                              Review Articles
   Early development:
            R.D. Peacock, Structure and Bonding, vol. 22, 83-122 (1975).
   Later developments
            L. Smentek, Physics Reports, vol. 297, 155-237 (1998).

National Aeronautics and    International School of Atomic and Molecular Spectroscopy
Space Administration                          Erice, Italy (June 2005)
Summary
 Physical Mechanisms: (Not a complete list)
  Crystal field influence based on static model. Second order in the perturbation.
   (This is the standard Judd-Ofelt theory).
  Crystal field influence based on static and dynamic model. Second order.
  Electron correlation based on static and dynamic model. Third order.
  Spin-orbit interaction. Intermediate coupling and Third order effects.
  Relativistic effects.
 Remaining Problems:
  Estimating the relative importance of each mechanism is considerable.
   (Many competing mechanisms producing various effects. Entangled situation)
  Ab-initio calculations still not entirely successful.
    - Theory of f - f transitions not yet complete.
    - Calculation of Radial integrals and knowledge of odd crystal field parameters.
    - Vibronics (Vibrational lattice-ion coupling)
  Multitude of mechanisms and new parameters abandons simplicity.
    - Simple linear parametric fitting to observed spectra is lost.
    - Physically meaningful descriptions can be obscured.
National Aeronautics and    International School of Atomic and Molecular Spectroscopy
Space Administration                          Erice, Italy (June 2005)
What’s next?

        “It has been in a very real sense the first step in the
        journey to an understanding of the rare earths and
        their much heavier cousins, the actinides, but like many
        journeys into the unknown, the end is not in sight.”


                 Brian G. Wybourne
                 “The fascination of rare earths - then, now and in the future”
                 Journal of Alloys and Compounds 380, 96-100 (2004).




National Aeronautics and         International School of Atomic and Molecular Spectroscopy
Space Administration                               Erice, Italy (June 2005)
Judd and Ofelt Finally Meet
                              40 years after publications




                           B.R. Judd   G.S. Ofelt     B.G. Wybourne


                 Ladek Zdroj,Poland - June 22, 2003
                 “4th International Workshop on Spectroscopy.
                 Structure and Synthesis of Rare Earth Systems.”


National Aeronautics and         International School of Atomic and Molecular Spectroscopy
Space Administration                               Erice, Italy (June 2005)
2007 School of Atomic and
               Molecular Spectroscopy
2007 will be the 45th anniversary of the simultaneous publications of Brian Judd and
George Ofelt. A special session is certainly worth considering in the next course.
    “The fascination of the Rare Earths - 45th Anniversary of Judd-Ofelt theory”
                             Possible invited lecturers:
      Brian R. Judd - The Johns Hopkins University, Baltimore, MD 21218, USA
                            E-mail: juddbr@eta.pha.edu
     George S. Ofelt - 824 Saint Clement Road, Virginia Beach, VA 23455, USA
                            E-mail: gsofelt@pilot,infi,net
Lydia Smentek - Vanderbilt University, Box 1547, Station B. Nashville, TN 37235, USA
                            E-mail: sementek1@aol.com
         G.W. Burdick - Andrews University, Berrien Springs, MI 49104, USA
                           E-mail: gburdick@andrews.edu
          Francois Auzel -UMR7574, CNRS, 92195 Meudon Cedux, France
                          E-mail: francois.auzel@wanaoo.fr
      Sverker Edvardsson, Mid Sweden University, S-851 70, Sundsvall, Sweden
                       E-mail: Sverker.Edvardsson@mh.se

 National Aeronautics and    International School of Atomic and Molecular Spectroscopy
 Space Administration                          Erice, Italy (June 2005)
Acknowledgements
  Rino DiBartolo-
  Thank you for your years of wisdom and my first lecture on
  Judd-Ofelt theory in your office in ‘old’ Higgins Hall. Also
  for inviting me to Erice these last 10 years.

  Norm Barnes-
  Thank you for helping me see the laser side of life. The
  discussions we have had over the years remain with me.




National Aeronautics and      International School of Atomic and Molecular Spectroscopy
Space Administration                            Erice, Italy (June 2005)
Dedication
 Brian G. Wybourne (1935-2003)
Professor Brian G Wybourne
Commemorative Meeting: Symmetry, Spectroscopy and Schur
Institute of Physics, Nicolaus Copernicus University, Torun, Poland
June 12-14, 2005.




A commemorative meeting in honor of Professor Brian G. Wybourne will be
held in Torun, Poland from 12-th to 14-th June 2005. The aim is to celebrate
Brian's academic life and his contributions to many aspects of physics and
mathematics. This meeting will bring together friends, students, collaborators
of Brian as well as people interested in the results and consequences of his research.

National Aeronautics and      International School of Atomic and Molecular Spectroscopy
Space Administration                            Erice, Italy (June 2005)
National Aeronautics and   Erice, Italy (June 2005)
Space Administration
National Aeronautics and   International School of Atomic and Molecular Spectroscopy
Space Administration                         Erice, Italy (June 2005)

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Judd-Ofelt Theory: Principles and Practices

  • 1. Judd-Ofelt Theory: Principles and Practices Brian M. Walsh NASA Langley Research Center National Aeronautics and Erice, Italy (June 2005) Space Administration
  • 2. Part I: Principles What is the Judd-Ofelt Theory? Based on static, free-ion and single configuration approximations: • static model - Central ion is affected by the surrounding host ions via a ‘static’ electric field. • free ion model - Host environment treated as a perturbation on the free ion Hamiltonian. • single configuration model - Interaction of electrons between configurations are neglected. The Judd-Ofelt theory describes the intensities of 4f electrons in solids and solutions. The remarkable success of this theory provides a sobering testament to simple approximations. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 3. Distribution of Citations by Year 200 B.R. Judd, Phys. Rev. 127, 750 (1962). G.S. Ofelt, J. Chem. Phys. 37, 511 (1962). 150 ~ 2000 citations (1962-2004) Number of citations 100 50 0 62 72 82 92 02 Year National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 4. Referenced in 169 Journal Titles Top 20 Titles # of citations PHYSICAL REVIEW B 127 JOURNAL OF NON-CRYSTALLINE SOLIDS 108 JOURNAL OF APPLIED PHYSICS 90 JOURNAL OF CHEMICAL PHYSICS 83 JOURNAL OF ALLOYS AND COMPOUNDS 81 JOURNAL OF LUMINESCENCE 77 JOURNAL OF PHYSICS-CONDENSED MATTER 58 MOLECULAR PHYSICS 57 CHEMICAL PHYSICS LETTERS 48 OPTICAL MATERIALS 43 JOURNAL OF THE OPTICAL SOCIETY OF AMERICA B 38 JOURNAL OF PHYSICS AND CHEMISTRY OF SOLIDS 35 PHYSICA STATUS SOLIDI A-APPLIED RESEARCH 33 OPTIKA I SPEKTROSKOPIYA 30 IEEE JOURNAL OF QUANTUM ELECTRONICS 27 PHYSICS AND CHEMISTRY OF GLASSES 27 OPTICS COMMUNICATIONS 26 SPECTROCHIMICA ACTA PART A 26 INORGANIC CHEMISTRY 24 JOURNAL OF THE AMERICAN CERAMIC SOCIETY 19 National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 5. 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 http://www.chem.ox.ac.uk/icl/heyes/LanthAct/I1.html ( some amusing mnemonics for the Lanthanides and Actinides) So much for ‘Understanding Chemistry’… Let’s do some physics! National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 6. Ions in Solids Solids • insulators (not semiconductors) • bandgaps are > 5ev (VUV photon) • produce a crystal field Ions • replace host ions substitutionally • transition metal and lanthanide series • unfilled electronic shells • Stark splitting from crystal field • optical transitions occur within bandgap Examples • Nd:Y3Al5O12 - Er:fiber - Cr:Al2O3 (Ruby) National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 7. Atomic Structure of Laser Ions National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 8. Atomic Interactions 4f 95d Hc >> Hso (LS-coupling) Hc << Hso (jj-coupling) Hc ≈ Hso (Intermediate coupling) !1 !2 !3 !4 5S 5I 4f10 5F 4 5I 5 5I 5I Configurations 6 Ho = central field 5I Terms 2S+1 L 7 (Electrons in field 5I Hc = Coulomb field 8 of the nucleus) (Mutual repulsion Levels 2S+1L J of electrons) Hso = spin orbit (Coupling between spin and orbital Stark Levels angular momentum) Vo = crystal field Ho >Hc , Hso >Vo (Electric field of host) Hund’s Rules*: F. Hund, Z. Phys. 33, 345 (1925) 1.) Lowest state has maximum 2S+1 2.) Of these, that with largest L will be lowest 3.) Shells < 1/2 full (smallest J is lowest), Shells > 1/2 full (largest J is lowest) *These rules apply only to the ground state, not to excited states. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 9. Transitions and Selection Rules • Not all transitions between atomic states that are energetically feasible are quot;allowed”. • Forbidden transitions are “forbidden*” to first order, which means they may occur in practice, but with low probabilities. • Selection rules for transitions depend on type of transition – Electric dipole (E1) – Electric quadrupole (E2) – Magnetic dipole (M1) • Wavefunctions must have correct parity (Laporte’s rule) • Symmetry plays a role in selection rules – Vibronics, crystal field, other perturbing effects. * This nomenclature is historically embedded, although not entirely accurate. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 10. Multipole Selection Rules ! ! Electric dipole operator (E1) P = quot;e! ri (odd operator) i ! equot; ! ! Magnetic dipole operator (M1) M =quot; ! I i + 2si 2mc i (even operator) ! ! ! ! 1 Q = $ ! k # ri quot;ri 2 i ( ) Quadrupole operator (E2) (even operator) S L J (No 0 ↔ 0) Parity Electric Dipole ΔS = 0 ΔL= 0, ±1 ΔJ = 0, ±1 opposite Magnetic dipole ΔS = 0 ΔL= 0 ΔJ = 0, ±1 same Electric quadrupole ΔS = 0 ΔL = 0, ±1, ±2 ΔJ = 0, ±1, ±2 opposite National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 11. A Brief History of Parity Otto Laporte (1902-1971) empirically discovered the law of parity conservation in physics. He divided states of the iron spectrum into two classes, even and odd, and found that no radiative transitions occurred between like states: O.Laporte, Z. Physik 23 135 (1924). Eugene Paul Wigner (1902-1995) explicitly formulated the law of parity conservation and showed that Laporte’s rule is a consequence of the invariance of systems under spatial reflection. E. P. Wigner, “Gruppentheorie und Ihre Anwendung auf die Quantenmechanik der Atomspektren”. Braunschweig:F. Vieweg und Sohn, 1931. English translation by J. J. Griffin. New York: Academic Press, 1959. Wavefunctions are classified as even (+1 parity) or odd (-1 parity). By convention, the parity of a photon is given by the radiation field involved: ED ( -1), MD (+1). For mathematical reasons, the parity of any system is the product of parities of the individual components. If the initial and final wavefunction have same parity (±1): ED: ±1 = (-1)(±1) Parity is NOT conserved. Transition is forbidden! MD: ±1 = (+1)(±1) Parity IS conserved. Transition is allowed! Laporte Rule: States with even parity can be connected by ED transitions only with states of odd parity, and odd states only with even ones. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 12. Parity Selection Rules ED allowed ED forbidden MD forbidden MD allowed EQ forbidden EQ allowed s → p s → s p → d d → d d → f p → p f → g f → f s → f g → g p → g Orbital s p d f g Angular momentum ! 0 1 2 3 4 !- odd # electrons ! = ( quot;1)# i ! even odd even odd even !- even # electrons i odd even odd even odd National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 13. Historical Perspective I • J.H. Van Vleck - J. Phys. Chem. 41, 67-80 (1937) (The Puzzle of Rare-Earth Spectra in Solids) – Why are spectral lines in rare earths observable? – Electric dipole(E1), magnetic dipole(M1), quadrupole(E2)? – Concludes a combination is possible. – Suggests that crystal field makes mixed parity states (E1). • L.J.F. Broer, et al., - Physica XI, 231- 250 (1945) (On the Intensities and the multipole character in the spectra of the rare earth ions) – Considers all mechanisms. – Concludes quadrupole radiation is too weak. – Considers magnetic dipole , but as a special case only. – ED transitions dominate as suggested by Van Vleck! National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 14. Historical Perspective II • G. Racah - Phys. Rev. 76, 1352 (1949) (Theory of Complex Spectra IV) – Applies group theory to problems of complex spectra – Creates the tools required to make detailed spectroscopic calculations involving states of the 4f shell. – Revolutionizes the entire subject of rare earth spectroscopy. • Subsequent developments – Racah’s methods applied to crystal field theory. – Ideas of Racah applied to transition metal ions (Griffiths). – Practical calculations assisted by computer generated tables of angular momentum coupling coefficients. • By 1962 the stage was set for the next major development: The Judd-Ofelt theory of the intensities of RE transitions. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 15. The Stage is Set “I suggest that the coincidence of discovery was indicative that the time was right for the solution of the problem.” Brian G. Wybourne “The fascination of rare earths - then, now and in the future” Journal of Alloys and Compounds 380, 96-100 (2004) National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 16. Judd and Ofelt Publish (1962) National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 17. States of an Ion in the Crystal The Crystal field, V, is considered as a first order perturbation that ‘admixes’ in higher energy opposite parity configurations: } quot;a V quot;# ! a = quot;a + % quot;# # Ea $ E# Mixed Parity quot;# V quot;b States ! b = quot;b + % quot;# # Eb $ E# ! ! ! ( +a V +* quot; + * P +b + a P + * + * V +b % quot; ,a P,b = !' + $ * quot; & Ea ) E * Eb ) E* quot; # φa and φb have the same parity (4f N states) φβ has opposite parity (4f N-15d states) V is the crystal field (treated as a perturbation) ! P is the electric dipole operator National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 18. Tensor Forms of Operators Racah defined irreducible tensors, C(k), which transform as spherical harmonics, having the components: quot; 4! % 1/2 Cq ) (k =$ # 2k + 1 ' Ykq & The position vector r is a tensor of rank 1, defined as r = rC (1) Dipole Operator Crystal Field ! ! Standard Form P = quot;e! ri V = ! ! Akq ri kYkq (quot; i , # i ) i i kq Dq = !equot; ri #Cq % D p ) = ! Atp ! rit quot;C p ) $ (1) (1) (t (t Tensor Form $ & i # % i i tp i Note: t is odd since only odd order terms contribute to parity mixing. Even order terms are responsible for energy level splitting. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 19. J-O Theory Assumptions 1&2 1.) The states of φβ are completely degenerate in J. Assume an average energy for the excited configuration above the 4fN, that is, the 4f N-15d. 2.) The energy denominators are equal ( Ea-Eβ = Eb-Eβ ) Assume that the difference of average energies, ΔE(4f-5d), is the same as the difference between the average energy of the 4f N-15d and the energy of the initial and final states of the 4fN These assumptions are only moderately met, but offer a great simplification. Otherwise, the many fold sum of perturbation expansions is not suitable for numerical applications. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 20. 4f and 4f N N-15d configurations 35 4fn configuration 30 4fn-15d1 configuration 25 Energy(×104cm-1) 20 Lanthanides in YLF: K. Ogasawara et al., 15 J. Solid State Chem. vol. 178, 412 (2005 10 5 0 Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb 58 59 60 61 62 63 64 65 66 67 68 69 70 Atomic Number & Symbol National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 21. Advantages of the Assumptions I.) Energy denominators can be removed from the summations II.) Closure can be used ( the excited configuration forms a complete orthonormal set of basis functions) #! quot; !quot; = 1 quot; III.) Angular parts of the electric dipole operator and crystal field Cq = ! C (1) !! U q (1) (1) and C p ) = ! C (t ) !! U p ) (t (t can be combined into an effective tensor operator %t 1 quot; ( + t 1 quot; . (quot; ) U U (1) (t ) = # (!1) 1+t + quot; +Q (2 quot; + 1) & )- 0 UQ ' ! ! !$ * , p q Q / q p quot;Q The 3j symbol ( ) is related to the coupling probability for two angular momenta. The 6j symbol { } is related to the coupling probability for three angular momenta. The Wigner 3-j and 6-j symbols are related to Clebsch-Gordon coupling coefficients. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 22. Reduced Matrix Elements Nevertheless, combining the tensors for the electric dipole and crystal field terms in a combined tensor operator, UQ! ) , ( can be simplified further by the Wigner-Eckart Theorem: Geometry Physics (transformations) (Dynamics) % J quot; J# ( N f N! JM UQquot; ) f N! # J #M # = ($1)J $ M ' ( f ! J U ( quot; ) f N! # J # & $M Q M #* ) The matrix elements on the right side have been tabulated: “Spectroscopic Coefficients of the p N, d N, and f N Configurations,” C.W. Nielson and G.F. Koster, M.I.T Press, Cambridge, MA (1963). The 3-j and 6-j symbols have also been tabulated: “The 3-j and 6-j symbols,” M. Rotenberg, R, Bivens, N. Metropolis, J.K. Wooten Jr., Technology Press, M.I.T, Cambridge, MA (1959). National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 23. “Full Judd-Ofelt Theory” ! 1 * * J( $ () 1)J )M )Q (2* + 1)AtpY (t , * )' t $' J , a P , b = )e!! % %q Q quot;% quot; + a U ( * ) +b tp *Q & p quot;% ) M #& Q M (quot; # n! r nquot;!quot; nquot;!quot; r t n! &1 t ! ) Where, Y (t, ! ) = 2% ! C (1) !quot; !quot; C (t ) ! ' * n! Ea # E$ ( ! !quot; ! + This is the “Full Solution” of the Judd-Ofelt Theory. This form can be used to find electric dipole matrix elements between mixed parity states for individual Stark level to Stark level transitions. Application of “Full Judd-Ofelt Theory”: R.P. Leavitt and C.A. Morrison, “Crystal-field Analysis of triply Ionized lanthanum trifluoride. II. Intensity Calculations.” Journal Of Chemical Physics, 73, 749-757 (1980). National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 24. J-O Theory Assumptions 3&4 Oscillator strength (f-number) for electric dipole transition: 2 8+ mc 2 (n + 2% 2 ! ! 2 f = n& & 3n ## )JM P ) quot;J quot;M quot; 3quot;* (2 J + 1)e 2 ' $ L.J.F. Broer, et al., - Physica XI, 231- 250 (1945) 3.) Sum over Stark split J-levels (Assumes all Stark levels equally populated) $ J ! Jquot; ' $ J !quot; J quot; ' 1 *& Q M quot; ) & #M = + + Qquot; M quot; ) 2 ! + 1 !! quot; QQ quot; M = -J, -(J-1), …, 0, …, (J-1), J MM quot; % #M (% ( 4.) Sum over dipole orientations (Assumes optically isotropic situation) quot;1 ! t % quot;1 ! t) % 1 ($ q Q p' $ q Q = * * p) ' 2t + 1 tt ) pp ) Q = 0 (π-polarized, E ⊥ c) Q # &# & Q = ±1 (σ-polarized, E || c) National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 25. “Approximate Judd-Ofelt Theory” 2 2 8! mc 2 # n + 2& 2 Atp ) )) 2 (quot; ) f = n% (2 quot; + 1) Y (t, quot; ) * a U 2 *b 3hquot; (2J + 1) $ 3n ( ' quot; = 2, 4,6 p t =1, 3,5 (2t + 1) 2 Atp Defining Ωλ as: !quot; = (2 quot; + 1)# # (2t + 1)Y 2 (t, quot; ) Judd-Ofelt p t =1, 3,5 parameters 2 8! 2 mc # n2 + 2 & + 2 (quot; ) f = n% )quot; * a U *b Oscillator 3hquot; (2J + 1) $ 3n ( ' quot; = 2, 4,6 strength $ 2 (quot; ) SED = !quot; # a U #b is called the Linestrength. quot; = 2, 4,6 This is the “Approximate Solution” of the Judd-Ofelt theory. It can be used to find electric dipole matrix elements between mixed parity states for manifold to manifold transitions. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 26. Judd-Ofelt Parameters In principle, the Judd-Ofelt parameters can be calculated “ab-initio” if the crystal structure is known, and hence, Atp: 2 Atp !quot; = (2 quot; + 1)# # Y 2 (t, quot; ) p t =1, 3,5 (2t + 1) n! r nquot;!quot; nquot;!quot; r t n! &1 t ! ) Y (t, ! ) = 2% ! C !quot; !quot; C ! ' (1) (t ) * n! Ea # E$ ( ! !quot; ! + # ! 1 !! & ! C (1) !! = (quot;1)! % ( 2! + 1)1/2 ( 2!! + 1)1/2 $0 0 0( ' # !! t ! & ! C (t ) !! = (quot;1)!! % ( 2!! + 1)1/2 ( 2! + 1)1/2 $ 0 0 0( ' 3-j and 6-j symbols can be calculated for ! = 3 (4f ) and !! = 2 (5d) Radial integrals between configurations and crystal field components, Atp, are difficult to calculate. Instead, Judd-Ofelt parameters are usually treated as phenomenological parameters, determined by fitting experimental linestrength data. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 27. Intermission “The two papers of 1962 represent a paradigm that has dominated all further work on the intensities of rare earth transitions in solutions and solids up to the present time.” Brian G. Wybourne “The fascination of rare earths - then, now and in the future” Journal of Alloys and Compounds 380, 96-100 (2004). National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 28. Part II: Practices The Judd-Ofelt theory, in practice, is used to determine a set of phenomenological parameters, Ωλ (λ=2,4,6), by fitting the experimental absorption or emission measurements, in a least squares difference sum, with the Judd-Ofelt expression. Absorption Least Squares Judd-Ofelt Collect Matrix Measurements Fitting Parameters Elements # ( )=0 ! quot;2 Ωλ manifold ! (quot; )d quot; |<U(λ)>|2 !# k Transition τr and β Probabilities AJ′J The Judd-Ofelt parameters can then be used to calculate the transition probabilities, AJ′J, of all excited states. From these, the radiative lifetimes, τr, and branching ratios, β, are found. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 29. Selection Rules Revisited ! j1 j2 j3 $ #1 t ! & ! j1 j2 j3 $ $ J ! Jquot; ' quot; %=0 $ ' #m =0 #! 1 !2 !3 & ! !quot; ! ( quot; 1 m2 m3 & % & #M % Q M quot;) ( % Unless: Unless: J! quot; J # $ ! = 2, 4, 6 ji ! 0 ji ! 0 t = 1, 3, 5, 7 !J quot; 6 !i ! 0 mi quot; ji ! quot;1+ t !L quot; 6 j1 quot; j2 # j3 # j1 + j2 m1 + m2 + m3 = 0 !S = 0 !! quot; ! # 1 ji , mi (1, 1/2 integer) ! 2 quot; ! 3 # j1 # ! 2 + ! 3 J = 0 : J # $ even Only d or g j1 # j2 quot; j3 quot; j1 + j2 ! 1 quot; ! 3 # j2 # ! 1 + ! 3 orbitals can J # = 0 : J $ even mix parity ! 1 quot; ! 2 # j3 New Selection Rules From Judd-Ofelt Theory S L J (No 0 ↔ 0) Parity Electric Dipole ΔS = 0 ΔL ≤ 6 ΔJ ≤ 6 opposite ΔJ = 2,4,6 (J or J′ = 0) Magnetic dipole ΔS = 0 ΔL = 0 ΔJ = 0, ±1 same Electric quadrupole ΔS = 0 ΔL = 0, ±1, ±2 ΔJ = 0, ±1, ±2 opposite National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 30. Judd-Ofelt Analysis I Matrix Forms 3ch(2J + 1) # 3 & 2 Sm = 8! e quot; 3 2 n% 2 $ n + 2( ' * manifold ) (quot; )d quot; S jm Components of 1 x N matrix 3 $ S = quot; M ij !i 2 (quot; ) SED = !quot; # a U #b t j quot; = 2, 4,6 i =1 N = number of tramsitions Mij - components of N x 3 matrix for square matrix elements of U ( 2 ), U ( 4 ), U (6 ) Ωi - components of 1 x 3 matrix for Judd-Ofelt parameters Ω 2, Ω 4, Ω 6 2 N % m 3 ( ! = $ ' S j quot; $ M ij #i * 2 LEAST SQUARES DIFFERENCE j =1 & i =1 ) ( ) = $2 ! quot;2 N & m 3 ) ( !(0) = M †M ) quot;1 !# k % ' M jk ( S j $ % M ij #i + = 0 MINIMIZED * M †Sm j =1 i =1 Judd-Ofelt Parameters 1 x 3 Matrix National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 31. Judd-Ofelt Fit (Ho:YLF) 6.0 Visible absorption spectrum of Ho:YLF 5.0 !ab (10-20 cm2) (! and quot; polarization) 4.0 3.0 2.0 1.0 0.0 280 330 380 430 480 530 580 630 680 Wavelength (nm) National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 32. Judd-Ofelt Analysis II With the Judd-Ofelt parameters, the ED transition probability for any excited state transition (J´→ J) can be calculated 64quot; 4 e2 * $ n2 + 2 ' 2 - Transition probability A J !J = 3 ,n & SED + n SMD / 2 3h(2 J ! + 1)# , % + 3 ) ( / . (Einstein A coefficient) 1 = # AJ quot;J Radiative lifetime !r J (natural decay time) AJ quot;J Branching ratio ! J quot;J = # AJ quot;J (fraction of total photon flux) J MD transitions are normally orders of magnitude smaller than ED transitions. Since ED transitions for ions in solids occur as a result of a perturbation, some MD transitions will make significant contributions. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 33. Magnetic Dipole Contributions Magnetic dipole contributions can be easily calculated using an appropriate set of intermediate coupled wavefunctions for transitions obeying the selection rules ( ΔS = 0, ΔL= 0, ΔJ = 0, ±1). 2 ' quot; $ ! ! f n [SL]J L + 2S f n [S !L!]J ! 2 S MD =% quot; MD Linestrength & 2mc # 1/ 2 LS-coupled 2 - (J + 1) . (L . S ) * ! ! ! n '- ! 2 2 *$ f [SL]J L + 2 S f [S /L/]J / = &+(S + L + 1) . (J + 1) + matrix elements n 2 ((# !+ %, , 4(J + 1) )(! )quot; G.H. Shortley Phys. Rev. 57, 225 (1940) Intermediate coupled wavefunctions f n [SL]J = ! C ( S, L ) f n SLJ SL (linear combination of LS states) ! ! n quot; ! n f [SL]J L + 2S f [S quot;Lquot;]J quot; = n ! C (S , L )C (S , L ) f SLJ L + 2S f S quot;Lquot;J quot; n SL ,S quot;Lquot; Intermediate coupled matrix elements National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 34. Judd-Ofelt Results (Ho:YLF) National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 35. Testing the J-O theory Branching ratios can be measured directly from emission spectra. Use reciprocity of emission and absorption to indirectly “measure” the radiative lifetimes. Z! *$ hc ' - ! em ( quot; ) = ! ab ( quot; ) exp ,& EZL # ) kT / D.E. McCumber Zu +% quot;( . Phys. Rev. 136, A954 (1964). By comparing the measured emission cross section quot;5 3I& ( quot; ) ! (quot; ) = P. Moulton 8# cn 2 ($ r / % ) + ' 2I ! ( quot; ) + I # ( quot; ) ) quot; d quot; ( * J. Opt. Soc Am. B 3, 131 (1986). with the emission cross section derived from absorption, the quantity (τr/β) can be determined and the radiative lifetime extracted for comparison with the Judd-Ofelt theory National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 36. Reciprocity of Ho:YLF (5I7 ↔ 5I8) National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 37. Accuracy of J-O theory (Ho&Tm) Results are somewhat better in Ho3+ than Tm3+. Overall, the accuracy of the Judd-Ofelt theory is quite good, despite the approximations used. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 38. Special Case I: Pr3+ ion (A failure of the standard Judd-Ofelt theory?) Pr3+ ions suffer from several problems in applying Judd-Ofelt theory 1.) Large deviations between calculations and experiment observations. 2.) Negative Ω2 sometimes obtained, in opposition with definition. 3.) Ω2, Ω4, Ω6 highly dependent on transitions used in fit. These inconsistencies are usually explained by the small energy gap (~ 50,000 cm -1) between the 4f N and 4f N-15d configurations in Pr3+ Solutions: 1.) Modify the standard theory: quot;!# = quot;# &1 + ( $Eij % 2E4 f ) ( E5d % E4 f ) ( ' 0 ) E.E. Dunina, et al., Sov. Phys. Solid State 32, 920 (1990). 2.) Remove 3H4 → 3P2 from the fit, or augment fit with fluorescence β’s R.S.Quimby, et al., J. Appl. Phys. 75, 613 (1994). 2 N +% ( . 3.) Use normalized least squares fitting procedure: ! = $ -' S jm quot; $ M ij #i * ! i 0 2 j =1 , & i ) / P. Goldner, et al., J. Appl. Phys. 79, 7972 (1996). National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 39. Special Case II: Eu3+ ions (Beyond the standard Judd-Ofelt theory)  The ED transitions 7F0 ↔ 5DJodd, 7FJodd ↔ 5D0 and 7F0 ↔ 5D0 in Eu3+ are “forbidden” in standard JO-theory. They violate the selection rules: • ΔS = 0 G.W. Burdick, J. Chem Phys. 91 (1989). • If J = 0 then J′ is even • If J′ = 0 then J is even M. Tanaka, Phys. Rev. B, 49, 16917 (1994). •0↔0 T. Kushida, Phys. Rev B, 65, 195118 (2002).  These transitions are primarily MD, but all three do occur as ED with low intensity in the spectra of some materials.  This implies that the standard Judd-Ofelt theory is incomplete. These ‘forbidden’ transitions provide an ideal testing ground for extensions to the standard theory.  What mechanism or mechanisms could be responsible? Are they meaningful! National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 40. Europium’s Peculiar Properties (Adventures of The Atom) The Atom, Issue 2 August 1962 (DC Comics) Coincident with the publications of Judd and Ofelt, who were both also interested in Europium’s peculiar properties. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 41. Extensions I 1) J-mixing: The wavefunctions of the J ≠ 0 state are mixed into the J = 0 state by even parity terms of the crystal field. Explains the radiative transition 7F3 ↔ 5D0 in Eu3+. J.E. Lowther, J. Phys. C: Solid State Phys. 7, 4393 (1974). 2) Electron correlation: Electrostatic interaction between electrons is taken into account. Goes beyond the single configuration approximation and electron correlation within the 4f shell is incorporated by configuration interactions. Contributes to “allowing” the “forbidden” 0 ↔ 0 transitions such as 7F0 ↔ 5D0 in Eu3+. K. Jankowski, J. Phys B: At. Mol. Phys. 14, 3345 (1981). 3) Dynamic coupling: The mutual interaction of the lanthanide ion and the crystal environment are taken into account. Goes beyond the static coupling model. Explains hypersensitive transitions (transitions highly sensitive to changes in environment). M.F. Reid et al., J. Chem Phys. 79, 5735 (1983). National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 42. Extensions II 4) Wybourne-Downer mechanism: Involves spin-orbit interaction among states of the excited configurations, leading to an admixing of spin states into the 4f N configuration. This accounts for the observed spin “forbidden” transitions ΔS = 1 B.G. Wybourne, J. Chem. Phys. 48, 2596 (1968). M.C. Downer et al., J. Chem. Phys 89, 1787 (1988). 5) Relativistic contributions: Relativistic treatment of f → f transitions in crystal fields. Reformulation of crystal field and operators in relativistic terms. Importance unknown. L. Smentek, B.G. Wybourne, J. Phys. B: At. Mol. Opt, Phys. 33, 3647 (2000). L. Smentek, B.G. Wybourne, J. Phys. B: At. Mol. Opt, Phys. 34, 625 (2001). Review Articles Early development: R.D. Peacock, Structure and Bonding, vol. 22, 83-122 (1975). Later developments L. Smentek, Physics Reports, vol. 297, 155-237 (1998). National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 43. Summary Physical Mechanisms: (Not a complete list)  Crystal field influence based on static model. Second order in the perturbation. (This is the standard Judd-Ofelt theory).  Crystal field influence based on static and dynamic model. Second order.  Electron correlation based on static and dynamic model. Third order.  Spin-orbit interaction. Intermediate coupling and Third order effects.  Relativistic effects. Remaining Problems:  Estimating the relative importance of each mechanism is considerable. (Many competing mechanisms producing various effects. Entangled situation)  Ab-initio calculations still not entirely successful. - Theory of f - f transitions not yet complete. - Calculation of Radial integrals and knowledge of odd crystal field parameters. - Vibronics (Vibrational lattice-ion coupling)  Multitude of mechanisms and new parameters abandons simplicity. - Simple linear parametric fitting to observed spectra is lost. - Physically meaningful descriptions can be obscured. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 44. What’s next? “It has been in a very real sense the first step in the journey to an understanding of the rare earths and their much heavier cousins, the actinides, but like many journeys into the unknown, the end is not in sight.” Brian G. Wybourne “The fascination of rare earths - then, now and in the future” Journal of Alloys and Compounds 380, 96-100 (2004). National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 45. Judd and Ofelt Finally Meet 40 years after publications B.R. Judd G.S. Ofelt B.G. Wybourne Ladek Zdroj,Poland - June 22, 2003 “4th International Workshop on Spectroscopy. Structure and Synthesis of Rare Earth Systems.” National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 46. 2007 School of Atomic and Molecular Spectroscopy 2007 will be the 45th anniversary of the simultaneous publications of Brian Judd and George Ofelt. A special session is certainly worth considering in the next course. “The fascination of the Rare Earths - 45th Anniversary of Judd-Ofelt theory” Possible invited lecturers: Brian R. Judd - The Johns Hopkins University, Baltimore, MD 21218, USA E-mail: juddbr@eta.pha.edu George S. Ofelt - 824 Saint Clement Road, Virginia Beach, VA 23455, USA E-mail: gsofelt@pilot,infi,net Lydia Smentek - Vanderbilt University, Box 1547, Station B. Nashville, TN 37235, USA E-mail: sementek1@aol.com G.W. Burdick - Andrews University, Berrien Springs, MI 49104, USA E-mail: gburdick@andrews.edu Francois Auzel -UMR7574, CNRS, 92195 Meudon Cedux, France E-mail: francois.auzel@wanaoo.fr Sverker Edvardsson, Mid Sweden University, S-851 70, Sundsvall, Sweden E-mail: Sverker.Edvardsson@mh.se National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 47. Acknowledgements Rino DiBartolo- Thank you for your years of wisdom and my first lecture on Judd-Ofelt theory in your office in ‘old’ Higgins Hall. Also for inviting me to Erice these last 10 years. Norm Barnes- Thank you for helping me see the laser side of life. The discussions we have had over the years remain with me. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 48. Dedication Brian G. Wybourne (1935-2003) Professor Brian G Wybourne Commemorative Meeting: Symmetry, Spectroscopy and Schur Institute of Physics, Nicolaus Copernicus University, Torun, Poland June 12-14, 2005. A commemorative meeting in honor of Professor Brian G. Wybourne will be held in Torun, Poland from 12-th to 14-th June 2005. The aim is to celebrate Brian's academic life and his contributions to many aspects of physics and mathematics. This meeting will bring together friends, students, collaborators of Brian as well as people interested in the results and consequences of his research. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)
  • 49. National Aeronautics and Erice, Italy (June 2005) Space Administration
  • 50. National Aeronautics and International School of Atomic and Molecular Spectroscopy Space Administration Erice, Italy (June 2005)