Physics beyond the Standard Model from hydrogen spectroscopy
Wim Ubachs, Jeroen C.J. Koelemeij, Kjeld S.E. Eikema, Edcel J., Salumbides

TL;DR
Hydrogen spectroscopy, both astronomical and laboratory-based, provides stringent tests for physics beyond the Standard Model by constraining variations in fundamental constants and searching for new forces or dimensions.
Contribution
This paper combines astrophysical observations and high-precision laboratory measurements to set new bounds on physics beyond the Standard Model, including variations in the proton-electron mass ratio and fifth forces.
Findings
Constraints on proton-electron mass ratio variation: |bc/bc|< 5 imes 10^{-6}
Laboratory measurements agree with quantum electrodynamics calculations
Bounds on fifth forces and extra dimensions derived from hydrogen spectroscopy
Abstract
Spectroscopy of hydrogen can be used for a search into physics beyond the Standard Model. Differences between the absorption spectra of H as observed at high redshift and those measured in the laboratory can be interpreted in terms of possible variations of the proton-electron mass ratio. Investigation of some ten of such absorbers in the redshift range yields a constraint of at 3. Observation of H from the photospheres of white dwarf stars inside our Galaxy delivers a constraint of similar magnitude on a dependence of on a gravitational potential times as strong as on the Earth's surface. Laser-based precision measurements of dissociation energies, vibrational splittings and rotational level energies in H molecules and their deuterated isotopomers HD and D produce values for the rovibrational binding…
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