2001MNRAS.327.1244M

Quasar (QSO) absorption spectra provide an extremely useful probe of possible cosmological variation in various physical constants. Comparison of Hi 21-cm absorption with corresponding molecular (rotational) absorption spectra allows us to constrain variation in y≡α^2g_p, where α is the fine-structure constant and g_p is the proton g-factor. We analyse spectra of two QSOs, PKS 1413+135 and TXS 0218+357, and derive values of Δy/y at absorption redshifts of z=0.2467 and 0.6847 by simultaneous fitting of the Hi 21-cm and molecular lines. We find Δy/y=(-0.20±0.44)×10^-5 and Δy/y=(-0.16±0.54)×10^-5 respectively, indicating an insignificantly smaller y in the past. We compare our results with other constraints from the same two QSOs given recently by Drinkwater et al. and Carilli et al., and with our recent optical constraints, which indicated a smaller α at higher redshifts.