Sensitivity coefficients to -variation for astrophysically relevant transitions in Ni II
arXiv:1407.1860 · doi:10.1103/PhysRevA.90.042512
Abstract
We calculated the dependence of the transition frequencies on the fine-structure constant (-factors) for Ni~II. Nickel is one of the few elements with high sensitivity to -variation, whose lines are observed at high redshifts. This makes it a sensitive probe for -variation on the cosmological timescale. The electronic structure of Ni II ion was treated within the configuration interaction (CI) method using Dirac-Coulomb Hamiltonian.
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