Abstract

The effects of the variation of the dimensionless strong interaction parameter X{sub q}=m{sub q}/{lambda}{sub QCD} (m{sub q} is the quark mass, {lambda}{sub QCD} is the QCD scale) are enhanced about 1.5x10{sup 5} times in the 7.6 eV ''nuclear clock'' transition between the ground and first excited states in the {sup 229}Th nucleus and about 1x10{sup 8} times in the relative shift of the 0.1 eV compound resonance in {sup 150}Sm. The best terrestrial limit on the temporal variation of the fundamental constants, |{delta}X{sub q}/X{sub q}|<4x10{sup -9} at 1.8 billion years ago (|X{center_dot}{sub q}/X{sub q}|<2.2x10{sup -18}y{sup -1}), is obtained from the shift of this Sm resonance derived from the Oklo natural nuclear reactor data. The results for {sup 229}Th and {sup 150}Sm 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 calculations in heavy nuclei. The extrapolation results are compared with the ''direct'' estimates obtained using the Walecka model. A number of numerical relations needed for the calculations of the variation effects in nuclear physics and atomic spectroscopy have been obtained: for the nuclear binding energy {delta}E/E{approx_equal}-1.45 {delta}m{sub q}/m{sub q},more » for the spin-orbit intervals {delta}E{sub so}/E{sub so}{approx_equal}-0.22 {delta}m{sub q}/m{sub q}, for the nuclear radius {delta}r/r{approx_equal}0.3 {delta}m{sub q}/m{sub q} (in units of {lambda}{sub QCD}); for the shifts of nuclear resonances and weakly bound energy levels {delta}E{sub r}{approx_equal}10 {delta}X{sub q}/X{sub q} MeV.« less

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