Limits on the Dependence of the Fine-Structure Constant on Gravitational Potential from White-Dwarf Spectra

被引:61
作者
Berengut, J. C. [1 ]
Flambaum, V. V. [1 ]
Ong, A. [1 ]
Webb, J. K. [1 ]
Barrow, John D. [2 ]
Barstow, M. A. [3 ]
Preval, S. P. [3 ]
Holberg, J. B. [4 ]
机构
[1] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
[2] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 0WA, England
[3] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[4] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
关键词
PHYSICAL CONSTANTS; TIME-VARIATION; TERM ANALYSIS; ELEMENTS; G191-B2B; NICKEL; ALPHA;
D O I
10.1103/PhysRevLett.111.010801
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We propose a new probe of the dependence of the fine-structure constant alpha on a strong gravitational field using metal lines in the spectra of white-dwarf stars. Comparison of laboratory spectra with far-UV astronomical spectra from the white-dwarf star G191-B2B recorded by the Hubble Space Telescope Imaging Spectrograph gives limits of Delta alpha/alpha = (4.2 +/- 1.6) x 10(-5) and (-6.1 +/- 5.8) x 10(-5) from FeV and NiV spectra, respectively, at a dimensionless gravitational potential relative to Earth of Delta phi approximate to 5 x 10(-5). With better determinations of the laboratory wavelengths of the lines employed these results could be improved by up to 2 orders of magnitude.
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页数:5
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