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 alpha, g(p), and yequivalent tom(e)/m(p). 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 zsimilar to0.68 to constrain changes in the three parameters over the redshift range 0</p
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We have detected the four 18 cm OH lines from the z ∼ 0.765 gravitational lens toward PMN J013...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to measure variations in the fundamental parameters α and y≡me/mp, using...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters α and y≡m<SUB>e</SUB...
International audienceWe have detected the four 18 cm OH lines from the z˜0.765 gravitational ...
International audienceWe have detected the four 18 cm OH lines from the z˜0.765 gravitational ...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We have detected the four 18 cm OH lines from the z ∼ 0.765 gravitational lens toward PMN J013...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to estimate variations in the fundamental constants using 18 cm OH absor...
We describe a new technique to measure variations in the fundamental parameters α and y≡me/mp, using...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters α and y≡m<SUB>e</SUB...
International audienceWe have detected the four 18 cm OH lines from the z˜0.765 gravitational ...
International audienceWe have detected the four 18 cm OH lines from the z˜0.765 gravitational ...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We describe a new technique to measure variations in the fundamental parameters alpha and yequivalen...
We have detected the four 18 cm OH lines from the z ∼ 0.765 gravitational lens toward PMN J013...