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, and M. B. Bainbridge
Phys. Rev. Lett. 107, 191101 – Published 31 October 2011

Abstract

We previously reported Keck telescope observations suggesting a smaller value of the fine structure constant α at high redshift. New Very Large Telescope (VLT) data, probing a different direction in the Universe, shows an inverse evolution; α increases at high redshift. Although the pattern could be due to as yet undetected systematic effects, with the systematics as presently understood the combined data set fits a spatial dipole, significant at the 4.2σ level, in the direction right ascension 17.5±0.9 h, declination 58±9 deg. 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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  • Received 23 August 2010

DOI:https://doi.org/10.1103/PhysRevLett.107.191101

© 2011 American Physical Society

Authors & Affiliations

J. K. Webb1, J. A. King1, M. T. Murphy2, V. V. Flambaum1, R. F. Carswell3, and M. B. Bainbridge1

  • 1School of Physics, University of New South Wales, Sydney, New South Wales 2052, Australia
  • 2Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H30, PO Box 218, Victoria 3122, Australia
  • 3Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, United Kingdom

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Issue

Vol. 107, Iss. 19 — 4 November 2011

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