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arxiv: 1008.3907 · v2 · submitted 2010-08-23 · 🌌 astro-ph.CO · gr-qc· hep-ph· hep-th· nucl-th· physics.atom-ph

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Indications of a spatial variation of the fine structure constant

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classification 🌌 astro-ph.CO gr-qchep-phhep-thnucl-thphysics.atom-ph
keywords highredshiftalphaconstantdipoledirectionfinekeck
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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.

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  1. New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method

    astro-ph.CO 2026-02 unverdicted novelty 5.0

    Galaxy cluster observations yield two preferred directions with cosmic anisotropy amplitude of about 5.3 times 10 to the minus 4 at roughly 1 sigma overall significance, though higher in the XMM-Newton subsample.