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   <subfield code="a">Further Evidence Suggestive of a Solar Influence on Nuclear Decay Rates</subfield>
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   <subfield code="c">[P. Sturrock, E. Fischbach, J. Jenkins]</subfield>
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   <subfield code="a">Recent analyses of nuclear decay data show evidence of variations suggestive of a solar influence. Analyses of datasets acquired at the Brookhaven National Laboratory (BNL) and at the Physikalisch-Technische Bundesanstalt (PTB) both show evidence of an annual periodicity and of periodicities with sidereal frequencies in the neighborhood of 12.25year−1 (at a significance level that we have estimated to be 10−17). It is notable that this implied rotation rate is lower than that attributed to the solar radiative zone, suggestive of a slowly rotating solar core. This leads us to hypothesize that there may be an &quot;inner tachocline” separating the core from the radiative zone, analogous to the &quot;outer tachocline” that separates the radiative zone from the convection zone. The Rieger periodicity (which has a period of about 154 days, corresponding to a frequency of 2.37 year−1) may be attributed to an r-mode oscillation with spherical-harmonic indices l=3,m=1, located in the outer tachocline. This suggests that we may test the hypothesis of a solar influence on nuclear decay rates by searching BNL and PTB data for evidence of a &quot;Rieger-like” r-mode oscillation, with l=3,m=1, in the inner tachocline. The appropriate search band for such an oscillation is estimated to be 2.00 - 2.28 year−1. We find, in both datasets, strong evidence of a periodicity at 2.11 year−1. We estimate that the probability of obtaining these results by chance is 10−12.</subfield>
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