Laboratory Limits for Temporal Variations of Fundamental Constants:. AN Update

Astronomy and Astrophysics – Astrophysics

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Precision comparisons of different atomic frequency standards over a period of a few years can be used for a sensitive search for temporal variations of fundamental constants. We present recent frequency measurements of the 688 THz transition in the 171Yb+ ion. For this transition frequency a record over six years is now available, showing that a possible frequency drift relative to a cesium clock can be constrained to (-0.54 ± 0.97) Hz/yr, i.e. at the level of 2 · 10-15 per year. Combined with precision frequency measurements of an optical frequency in 199Hg+ and of the hyperfine ground state splitting in 87Rb a stringent limit on temporal variations of the fine structure constant α: d ln α/dt = (-0.26 ± 0.39) · 10-15 yr-1 and a model-dependent limit for variations of the proton-to-electron mass ratio μ in the present epoch can be derived: d ln μ/dt = (-1.2 ± 2.2) · 10-15 yr-1. We discuss these results in the context of astrophysical observations that apparently indicate changes in both of these constants over the last 5-10 billion years.

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