2009
DOI: 10.1063/1.3094259
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Calibration of S119n isomer shift usingab initiowave function methods

Abstract: The isomer shift for the 23.87 keV M1 resonant transition in the (119)Sn nucleus is calibrated with the help of ab initio calculations. The calibration constant alpha((119)Sn) obtained from Hartree-Fock (HF) calculations (alpha(HF)((119)Sn) = (0.081+/-0.002)a(0)(-3) mm/s) and from second-order Moller-Plesset (MP2) calculations (alpha(MP2)((119)Sn) = (0.091+/-0.002)a(0)(-3) mm/s) are in good agreement with the previously obtained values. The importance of a proper treatment of electron correlation effects is de… Show more

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Cited by 19 publications
(23 citation statements)
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“…This linear relationship has also been observed in the complete active space self-consistent field (CASSCF) calculations on a small test set 67. For an alternative, non-empirical computation of the isomer shift, which employs derivatives of the electronic energy with respect to the size of the non-point-like nucleus and which is more laborious, see Refs 18,51,68,69. The slope α and intercept C are typically obtained with the least-squares method using a parametrization set of experimental isomer shifts and theoretically-computed densities ρ (0).…”
Section: Isomer Shiftmentioning
confidence: 56%
“…This linear relationship has also been observed in the complete active space self-consistent field (CASSCF) calculations on a small test set 67. For an alternative, non-empirical computation of the isomer shift, which employs derivatives of the electronic energy with respect to the size of the non-point-like nucleus and which is more laborious, see Refs 18,51,68,69. The slope α and intercept C are typically obtained with the least-squares method using a parametrization set of experimental isomer shifts and theoretically-computed densities ρ (0).…”
Section: Isomer Shiftmentioning
confidence: 56%
“…1,2,8,9 The electron density in the vicinity of the nucleus for which the isotope shift was calculated for was obtained from the solution to the Dirac equation for a single electron in the Coulomb potential of a point-charge nucleus and was then expressed in terms of the nonrelativistic electron density at the position of the nucleus. [16][17][18] Recently, an alternative technique to obtain contact densities within isomer-shift calculations was proposed, [20][21][22] where the contact-density is treated as an energy derivative with respect to the nuclear radius. 8 Then, more elaborate fully relativistic approaches based on the Dirac-Coulomb Hamiltonian in combination with a finite nuclear charge distribution model to obtain contact densities were developed.…”
Section: Introductionmentioning
confidence: 99%
“…By employing an extendednucleus model, one may also go beyond the contact density approximation and explicitly calculate the change in nucleus-electron interaction corresponding to the nuclear transition measured in Mössbauer spectroscopy. This approach has been pursued by Filatov and co-workers [19][20][21][22][23] who introduce a difference in radius between the ground-and excited state nucleus as a finite perturbation that can be used to numerically differentiate the electronic energy. An added advantage is that such a finite difference scheme also works for methods for which it is difficult to obtain the relaxed density directly.…”
Section: Introductionmentioning
confidence: 99%