A new approach for testing variations of fundamental constants over cosmic epochs using FIR fine-structure lines

Abstract

Aims. To obtain limits on the variation of the fine-structure constant alpha and the electron-to-proton mass ratio mu over different cosmological epochs. Methods. A new approach based on the comparison of redshifts of far infrared (FIR) fine-structure lines and low-lying rotational transitions in CO is proposed which is in principle more sensitive by a factor of 10 compared to QSO metal absorption lines. Results. Estimations of the quotient F = alpha^2/mu obtained for two distant quasars J1148+5251 (z = 6.42) and BR1202-0725 (z = 4.69) provide Delta F/F = (0.1+/-1.0)10^{-4} and (1.4+/-1.5)10^{-4}, respectively. The obtained limits are consistent with no variation of physical constants at the level of 0.01% over a period of 13 Gyr. Conclusions. Upcoming observations of quasars and distant galaxies in FIR fine-structure lines of different species and in CO low rotational lines at the SOFIA, HSO, and ALMA are expected to improve the current limit by, at least, an order of magnitude.

5 pages, to appear in A&A main journal

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Cited by in corpus (4)

• $\Lambda$-doublet spectra of diatomic radicals and their dependence on fundamental constants
• Unifying cosmological and recent time variations of fundamental couplings
• Mid- and far-infrared fine-structure line sensitivities to hypothetical variability of the fine-structure constant
• Sensitivity coefficients to $\alpha$-variation for fine-structure transitions in Carbon-like ions