Space-time variation of the s and c quark masses

Space-time variation of fundamental physical constants in expanding Universe is predicted by a number of popular models. The masses of second generation quarks are larger than first generation quark masses by several orders of magnitude, therefore space-time variation in quark masses may significantly vary between each generation. We evaluate limits on variation in the s and c quark masses from Big Bang nucleosynthesis, Oklo natural nuclear reactor, Yb+, Cs and Rb clock data. The construction of 229Th nuclear clock is expected to enhance these limits by several orders of magnitude. Furthermore, constraints are obtained on an oscillating scalar or pseudoscalar cold dark matter field, as interactions of the field with quarks produce variations in quark masses

Effects of the long-range neutrino-mediated force in atomic phenomena

As known, electron vacuum polarization by nuclear Coulomb field produces Uehling potential with the range $\hbar/2m_e c$. Similarly, neutrino vacuum polarization by $Z$ boson field produces long range potential $\sim G_F^2/r^5$ with a very large range $\hbar/2m_{\nu}c$. Measurements of macroscopic effects produced by potential $G_{eff}^2/r^5$ give limits on the effective interaction constant $G_{eff}$ which exceed Fermi constant $G_F$ by many orders of magnitude, while limits from spectroscopy of simple atomic systems are approaching the standard model predictions. In the present paper we consider limits on $G_{eff}$ from muonium, positronium, hydrogen and deuterium spectra and isotope shift in hydrogen and heavy atoms including corrections leading to the King plot non-linearity.Comment: 8 pages, 3 figures, 4 table