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A Question about energy transfer between Rare-Earth ions

  1. May 22, 2017 #1
    Dear all,

    I have a question about one of the values presented in a paper, which is crucial in calculating energy transfer probability between two Yb3+ ions.

    This is the paper:
    T. Kushida, "Energy Transfer and Cooperative Optical Transitions in Rare-Earth Doped Inorganic Materials. I. Transition Probability Calculation", J. Phys. Soc. Jpn. 1973, 34, 1318-1326. DOI: http://dx.doi.org/10.1143/JPSJ.34.1318

    The summary of this paper is that it uses similar approach to Judd-Ofelt theory (spherical harmonics with Coulomb interaction operator and extensive use of reduced matrix elements) to derive equations for dipole-dipole, dipole-quadrupole, quadrupole-quadrupole interactions. For the calculation of the actual values of these rates, one needs reduced matrix elements of the electronic transition.

    In line 27 and 36-37 of page 1323, the author presents the reduced matrix element values for 2F5/22F7/2 transition of Yb3+ ions, namely <f13 2F5/2||U(2)||f13 2F7/2> = 6/49, <f13 2F5/2||U(4)||f13 2F7/2> = 20/49, and <f13 2F5/2||U(6)||f13 2F7/2> = 6/7. However, there is no reference to where these values came from. If it is a theoretical value, it still wouldn't make sense because Judd-Ofelt calculations for Yb3+ is impossible considering that it only has one excited state level (Judd-Ofelt analysis requires several to make sense).

    How do you get these parameters?

    Actually, there is another paper by O.L. Malta:
    O. L. Malta, "Mechanisms of non-radiative energy transfer involving lanthanide ions revisited", J. non-Cryst. Solids 2008, 354, 4770-4776. DOI: http://dx.doi.org/10.1016/j.jnoncrysol.2008.04.023

    In page 4775, there is a calculation of energy transfer rate, but also provides no values they used for the calculation. They provide ΣΩk<f13 2F5/2||U(k)||f13 2F7/2>, but that is only enough to calculate dipole-dipole, and every other multipole calculation requires reduced matrix element of each tensor rank.

    Am I missing something in the theoretical or experimental aspect?

    Thank you,
  2. jcsd
  3. May 22, 2017 #2


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  4. May 22, 2017 #3
    Thank you DrDu, but I am very aware of that and it is precisely the reason why I am confused in the case of Yb3+.

    Racah parameters for rare earth ions are derived experimentally. A typical procedure requires absorption spectrum of multiple levels (to derive energy of each states), and a fitting is done with theoretical equation to obtain these three Racah parameters as well as spin-orbit coupling constant (and in some cases several other constants). In principle, this means that Racah parameters cannot be derived for Ce3+ and Yb3+ ions experimentally because the energy level difference is dependent only on the spin-orbit coupling constant for two-level case and the values for Racah parameters are arbitrary.

    Consequently, almost all reference I have seen that provides Racah parameters and Spin-orbit coupling constant for all lanthanide ions, shows only spin-orbit coupling constant for Ce3+ and Yb3+ and no Racah parameters. Without Racah parameters, one is unable to calculate reduced matrix elements in the intermediate coupling scheme.

    There is one, a theoretical work, that derives Racah parameters for all lanthanide ions, but they deviate quite off from the experimental values. Thus I cannot trust the values they provided for Yb3+.

    That means there must be some other way of obtaining racah parameters, or way of directly obtaining the reduced matrix elements for Yb3+ and Ce3+, in which the author of the paper I have shown above decided not to mention. I want to know how they did it.
    Last edited: May 22, 2017
  5. May 22, 2017 #4


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    From what I understand, the parameters U depend very little on the environment of the f orbitals and can therefore be calculated analytically. However, I have no access to the article you are citing.
  6. May 22, 2017 #5
    Yes indeed. U as well as F(k) are only slightly affected by the environment around f orbitals (they are still affected and there are tons of references out there reporting these parameters for different hosts, except for Yb3+ and Ce3+).**

    But that have nothing to do with obtaining U(k) itself. They cannot be obtained analytically because we have 4 unknown parameters (5 if you include F(0) and 9 if you include other parameters for precision) that are independent. It is entirely done by numerical method, most commonly least square fitting of energies of levels and you definitely need more than 2 levels to do this.

    **It should be well noted that it is sometimes a poor choice to be overconfident about this fact because some hosts do deviate from average value. For example, using parameters obtained in LaF3:Er3+ and applying it to Y2O2S:E3+ may lead to error by 17.5% in U(2)!! However, the common practice is to apply parameters obtained in a certain host to another host, and most of the time it works fine, especially if you re-optimize the F(k) and spin-orbit parameters.
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