THE QUASAR ABSORPTION LINE FINE STRUCTURE EXPERIMENT Based upon the Physical Review Letter entitled "Further Evidence for Cosmological Evolution of the Fine Structure Constant"J.K. Webb (1), M.T. Murphy (1), V.V. Flambaum (1), V.A. Dzuba (1),J.D. Barrow (2), C.W. Churchill (3), J.X. Prochaska (4), A.M. Wolfe (5) (1) University of New South Wales, (2) Cambridge University (3) The Pennsylvania State University, (4) The Carnegie Observatories, (5) University of California, San Deigo Web Page by Chris Churchill This work funded in part by NASA, National Science Foundation, John Templeton Foundation Listen to an audio presentation with accompanying Power Point slides.
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Evolution in the Fine Structure Constant?: The Results ![]() Figure 1. The measured fractional change in the fine structure constant, alpha=e^2/hc, is plotted as a function of fractional look-back time (0=present day, 1=beginning of time). The corresponding cosmological redshift is shown along the top axis. The blue data show the results of hydrogen 21-cm absorption lines (using radio telescopes). The red data point show the results of the standard "alkali-doublet" method. The black data points show the new "many-multiplet" method developed for this work. This latter method provides an order of magnitude increase in the precision. There is now evidence that the constant evolves one part in 100,000 over the last 10 billion (or so) years. It may be that the the "constant" is slightly increasing with cosmic time. | |
The Experiment
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Web page by Chris Churchill: last updated Aug 29, 2K+1 cwc@astro.psu.edu 525 Davey Laboratory Department of Astonomy & Astrophysics Penn State University, University Park, PA, 16802 ph. 814-863-2918; fax. 814-863-3399 |