2005
DOI: 10.1103/physreva.72.022503
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Calculation of isotope shifts for cesium and francium

Abstract: We perform ab initio calculations of isotope shifts for isotopes of cesium (from A=123 to A=137) and francium (from A=207 to A=228). These calculations start from the relativistic Hartree-Fock method and make use of several techniques to include correlations. The field (volume) isotope shift is calculated by means of an all-order correlation potential method and within the singlesdoubles partial triples linearized coupled-cluster approach. Many-body perturbation theory in two different formulations is used to … Show more

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Cited by 54 publications
(85 citation statements)
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“…Unfortunately, the same method cannot be used for the calculation of the SMS for reasons explained in Ref. [111]. The SMS shift was calculated in Ref.…”
Section: Isotope Shiftmentioning
confidence: 99%
See 1 more Smart Citation
“…Unfortunately, the same method cannot be used for the calculation of the SMS for reasons explained in Ref. [111]. The SMS shift was calculated in Ref.…”
Section: Isotope Shiftmentioning
confidence: 99%
“…[111], where Table 17 Comparison of the total isotope shifts with experiment for Na (δν 22,23 ), K (δν 41,39 ), and Ca + (δν 43,40 Expt.…”
Section: Isotope Shiftmentioning
confidence: 99%
“…These reach from the extraction of nuclear properties from atomic spectra to applications in astronomy and fundamental physics. The spectrum of atoms and ions encodes information that provides a key to the ground-state properties of nuclei [2,3], small parity-violating effects caused by the weak interaction [4], for unitarity tests of the Cabibbo-Kobayashi-Maskawa (CKM) matrix [5], or for probing the Higgs coupling between electrons and quarks [6]. Light appearing on earth from stars at large distances is red shifted and can provide information about the spectra of atoms in ancient times and whether there have been changes, for example from a variation of the fine structure constant α.…”
Section: Introductionmentioning
confidence: 99%
“…The contribution due to configuration mixing with the ν1i 11/2 orbital (using the calculated magnetic moment for 209 Pb [49]) is relatively small, at 3.8%. However, in contrast, ν1i 11/2 configuration mixing accounts for 33.5% of the 214 Fr ground state assignment when I = (2 − ), with g( 214g Fr I=(2 − ) ) = +0.144 (10). In either case, evidence of a contribution from the ν1i 11/2 orbital supports previous theoretical studies that require this in order to reproduce the kink in the mean square charge-radii values at the N = 126 shell closure [14,15,17].…”
Section: Discussionmentioning
confidence: 99%
“…In this paper we focus on the charge radii in the trans-lead region and in particular, the characteristic increase in the gradient that is observed at a shell closure crossing. This is often referred to as a "kink" [4] and has already been seen at N = 126 in the neighboring isotopes from thallium to radium [5][6][7][8][9][10][11][12].…”
Section: Introductionmentioning
confidence: 99%