Enhanced effect of quark mass variation in 229Th and limits from Oklo data
V. V. Flambaum, R. B. Wiringa

TL;DR
This paper investigates how variations in quark mass influence nuclear transition energies in 229Th and resonance shifts in 150Sm, deriving limits from Oklo data and comparing extrapolated and direct calculations.
Contribution
It provides new estimates of quark mass variation effects in heavy nuclei using extrapolation from light nuclei and compares these with direct models, refining constraints on fundamental constant variations.
Findings
Enhanced sensitivity of nuclear transitions to quark mass variations.
Best terrestrial limit on quark mass variation from Oklo data.
Numerical relations for nuclear energy shifts related to quark mass changes.
Abstract
The effects of the variation of the dimensionless strong interaction parameter Xq=mq/Lambda{QCD} (mq is the quark mass, Lambda{QCD} is the QCD scale) are enhanced about 1.5 x 10**5 times in the 7.6 eV "nuclear clock" transition between the ground and first excited states in the 229Th nucleus and about 1 x 10**8 times in the relative shift of the 0.1 eV compound resonance in 150Sm.The best terrestrial limit on the temporal variation of the fundamental constants, |delta(Xq)/Xq| < 4 x 10**-9 at 1.8 billion years ago (|d(Xq/Xq)/dt| < 2.2 x 10**-18 y**-1), is obtained from the shift of this Sm resonance derived from the Oklo natural nuclear reactor data. The results for 229Th and 150Sm are obtained by extrapolation from light nuclei where the many-body calculations can be performed more accurately. The errors produced by such extrapolation may be smaller than the errors of direct…
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