Atomic transition frequencies, isotope shifts, and sensitivity to variation of the fine structure constant for studies of quasar absorption spectra

TL;DR

This paper compiles precise atomic transition data and isotope shift measurements crucial for detecting potential variations in the fine structure constant alpha through quasar absorption spectra analysis.

Contribution

It provides a comprehensive set of atomic transition frequencies, isotope shifts, and sensitivity coefficients to alpha-variation, aiding future astrophysical tests of fundamental constant variability.

Findings

Compiled atomic transition frequencies with high accuracy.

Identified isotope shifts necessary for systematic error correction.

Presented sensitivity coefficients to alpha-variation.

Abstract

Theories unifying gravity with other interactions suggest spatial and temporal variation of fundamental "constants" in the Universe. A change in the fine structure constant, alpha, could be detected via shifts in the frequencies of atomic transitions in quasar absorption systems. Recent studies using 140 absorption systems from the Keck telescope and 153 from the Very Large Telescope, suggest that alpha varies spatially. That is, in one direction on the sky alpha seems to have been smaller at the time of absorption, while in the opposite direction it seems to have been larger. To continue this study we need accurate laboratory measurements of atomic transition frequencies. The aim of this paper is to provide a compilation of transitions of importance to the search for alpha variation. They are E1 transitions to the ground state in several different atoms and ions, with wavelengths ranging from around 900 - 6000 A, and require an accuracy of better than 10^{-4} A. We discuss isotope shift measurements that are needed in order to resolve systematic effects in the study. The coefficients of sensitivity to alpha-variation (q) are also presented.