2009
DOI: 10.1088/0953-4075/42/17/175002
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Irreducible tensor form of the relativistic corrections to the M1 transition operator

Abstract: The relativistic corrections to the magnetic dipole moment operator in the Pauli approximation were derived originally by Drake [1]. In the present paper, we derive their irreducible tensor-operator form to be used in atomic structure codes adopting the Fano-Racah-Wigner algebra for calculating its matrix elements.

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Cited by 10 publications
(10 citation statements)
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“…To fill this gap, we compare our transition probabilities with others for the first elements of its isoelectronic sequence, i.e., N I and O II. A priori, the omission of the relativistic corrections to the M1 transition operator [4,64] could be a serious limitation of our calculations. Indeed, Eissner and Zeippen [65] showed that for transitions between terms of the 2p 3 configuration, in particular, the relativistic corrections are of the same order of magnitude as the usual nonrelativistic amplitude (see N I and O II data of Table XII).…”
Section: Transition Probabilitiesmentioning
confidence: 99%
See 1 more Smart Citation
“…To fill this gap, we compare our transition probabilities with others for the first elements of its isoelectronic sequence, i.e., N I and O II. A priori, the omission of the relativistic corrections to the M1 transition operator [4,64] could be a serious limitation of our calculations. Indeed, Eissner and Zeippen [65] showed that for transitions between terms of the 2p 3 configuration, in particular, the relativistic corrections are of the same order of magnitude as the usual nonrelativistic amplitude (see N I and O II data of Table XII).…”
Section: Transition Probabilitiesmentioning
confidence: 99%
“…The carbon negative ion is important in astrophysics and atmosphere physics since nitrogen-like 2p 3 4 S o -2 D o forbidden lines are recognized as useful transitions for abundances determination [4][5][6]. It has also recently been suggested by Le Padellec et al [7] that C − negative ion could intervene in astrophysical reactions.…”
Section: Introductionmentioning
confidence: 99%
“…This small contribution, however, is sufficient to perturb the intended high-accuracy lifetime measurements on the 3s 2 3p 2 P o 3/2 level of principal interest. An accurate lifetime measurement on that lower level is of particular interest because it might test a detail of atomic structure (the electron anomalous magnetic moment (EAMM) contribution to the M1 line strength, an uncommonly large quantum electrodynamics (QED) effect at 0.45%; see Reference [62]). It has been conjectured that a test of the EAMM might reveal the presence of "new physics beyond the Standard Model".…”
Section: Al-like Ionsmentioning
confidence: 99%
“…Several measurements of E1-forbidden transition rates have reached an accuracy of better than 0.5%, which implies a significant challenge and requires a qualitative step forward for theory. Conceptually established in the 1950s, but largely overlooked and neglected by atomic structure theoreticians, the anomalous magnetic moment of the electron (EAMM)-beyond the (g − 2) QED effect on the level energy-causes an increase of the M1 transition rate by 0.45% [156,157,159]. A lifetime measurement of an accuracy better than this percentage can in principle test a leading QED correction-and there are not many QED contributions as large as this one.…”
Section: E1-forbidden Transition Ratesmentioning
confidence: 99%