A possible new interpretation of the results of α/α from QSO absorption lines
Abstract
The measurement of α/α from the QSO absorption lines of FeII taken at two different redshifts (Quast et al, Levshakov et al) is compared with the result based on the 23 data points also obtained from VLT/UVES (Chand et al), to demonstrate that the apparent oscillatory time-dependence fitting the latter taken at face value is reinforced by the former claimed to be of much better accuracy.
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