Probing fundamental constant evolution with redshifted conjugate-satellite OH lines
Nissim Kanekar (1,2), Jayaram N. Chengalur (1), Tapasi Ghosh (3) ((1), National Centre for Radio Astrophysics, India, (2) National Radio Astronomy, Observatory, USA, (3) Arecibo Observatory, USA)

TL;DR
This study uses conjugate satellite OH lines at redshift z~0.247 to investigate potential variations in fundamental constants over cosmic time, finding tentative evidence for a smaller fine structure constant in the past.
Contribution
It introduces a novel method using conjugate satellite OH lines to probe changes in fundamental constants with minimal systematic effects.
Findings
Tentative 2.6 sigma evidence for variation in constants at z~0.247
Estimated change in alpha: (-3.1 ± 1.2) × 10^{-6}
No systematic effects detected that could explain the observed offset
Abstract
We report Westerbork Synthesis Radio Telescope and Arecibo Telescope observations of the redshifted satellite OH-18cm lines at towards PKS1413+135. The "conjugate" nature of these lines, with one line in emission and the other in absorption, but with the same shape, implies that the lines arise in the same gas. The satellite OH-18cm line frequencies also have different dependences on the fine structure constant , the proton-electron mass ratio , and the proton gyromagnetic ratio . Comparisons between the satellite line redshifts in conjugate systems can hence be used to probe changes in , , and , with few systematic effects. The technique yields the expected null result when applied to Cen.A, a nearby conjugate satellite system. For the system towards PKS1413+135, we find, on combining results from the two…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
