The alpha-dependence of transition frequencies for some ions of Ti, Mn, Na, C, and O, and the search for variation of the fine structure constant
arXiv:physics/0404008 · doi:10.1103/PhysRevA.70.064101
Abstract
We use the relativistic Hartree-Fock method, many-body perturbation theory and configuration-interaction method to calculate the dependence of atomic transition frequencies on the fine structure constant, alpha. The results of these calculations will be used in the search for variation of the fine structure constant in quasar absorption spectra.
arXiv comment4 pages, 5 tables
References in corpus (14)
- The String Dilaton and a Least Coupling Principle
- The fundamental constants and their variation: observational status and theoretical motivations
- Further Evidence for Cosmological Evolution of the Fine Structure Constant
- A Search for Time Variation of the Fine Structure Constant
- Limits on the time variation of the electromagnetic fine-structure constant in the low energy limit from absorption lines in the spectra of distant quasars
- Space-Time Variation of Physical Constants and Relativistic Corrections in Atoms
- Calculations of the Relativistic Effects in Many-Electron Atoms and Space-Time Variation of Fundamental Constants
- Probing the cosmological variation of the fine-structure constant: Results based on VLT-UVES sample
- Probing the variability of the fine-structure constant with the VLT/UVES
- Astrophysical Limits on the Evolution of Dimensionless Physical Constants over Cosmological Time
- Does the fine-structure constant vary with cosmological epoch?
- The -dependence of transition frequencies for ions Si II, Cr II, Fe II, Ni II, and Zn II
- Energy levels and lifetimes of Gd IV and enhancement of the electron dipole moment
- Energy levels and lifetimes of Nd IV, Pm IV, Sm IV, and Eu IV
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