Indications of a Spatial Variation of the Fine Structure Constant

被引:399
作者
Webb, J. K. [1 ]
King, J. A. [1 ]
Murphy, M. T. [2 ]
Flambaum, V. V. [1 ]
Carswell, R. F. [3 ]
Bainbridge, M. B. [1 ]
机构
[1] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
[2] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[3] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
基金
澳大利亚研究理事会;
关键词
WAVELENGTH CALIBRATION; TIME-VARIATION; SPECTROGRAPH; ACCURACY; SPECTRA;
D O I
10.1103/PhysRevLett.107.191101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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 data set fits a spatial dipole, significant at the 4.2 sigma 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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页数:5
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