Indications of a spatial variation of the fine structure constant
J. K. Webb, J. A. King, M. T. Murphy, V. V. Flambaum, R. F. Carswell,, M. B. Bainbridge

TL;DR
This study suggests a possible spatial variation in the fine structure constant across the universe, supported by combined telescope data indicating a dipole pattern with high statistical significance.
Contribution
It provides evidence for a spatial dipole variation in alpha, combining data from Keck and VLT telescopes, which is a novel approach in this research area.
Findings
Combined dataset fits a spatial dipole with 4.2-sigma significance.
VLT and Keck data show consistent dipole directions and amplitudes.
No systematic effects identified that could explain the observed pattern.
Abstract
We previously reported Keck telescope observations suggesting a smaller value of the fine structure constant, alpha, at high redshift. New Very Large Telescope (VLT) data, probing a different direction in the universe, shows an inverse evolution; alpha increases at high redshift. Although the pattern could be due to as yet undetected systematic effects, with the systematics as presently understood the combined dataset fits a spatial dipole, significant at the 4.2-sigma level, in the direction right ascension 17.5 +/- 0.9 hours, declination -58 +/- 9 degrees. The independent VLT and Keck samples give consistent dipole directions and amplitudes, as do high and low redshift samples. A search for systematics, using observations duplicated at both telescopes, reveals none so far which emulate this result.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
