Constraining the variation of fundamental constants using 18 cm OH lines

We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absorption lines, with the advantage that all lines arise in the same species, allowing a clean comparison between the measured redshifts. In conjunction with one additional transition, it is possible to simultaneously measure changes in a, g<SUB>p</SUB>, and yΞm<SUB>e</SUB>/m<SUB>p</SUB>. We use the 1665 and 1667 MHz line redshifts in conjunction with those of HI 21 cm and mm-wave molecular absorption in a gravitational lens at z˜0.68 to constrain changes in the three parameters over the redshift range 0&lt;z˜0.68. While the constraints are relatively weak (˜1 part in 10<SUP>3</SUP>), this is the first simultaneous constraint on the variation of all three parameters. Either one (or more) of α, g<SUB>p</SUB>, and y must vary with cosmological time or there must be systematic velocity offsets between the OH, HCO<SUP>+</SUP>, and HI absorbing clouds