Do Radioactive Half-Lives Depend on the Earth-Sun Distance?

Physics – Nuclear Physics

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In recent articles [1-4], Jenkins et al. claim to have evidence that radioactive half-lives vary as a function of the earth-to-sun distance. They base their claims on data obtained by others over the space of several years -- the decay of ^32Si as measured at Brookhaven National Laboratory [5] from 1982-85 and that of ^226Ra as measured at the Physikalisch Technische Bundesanstalt in Germany [6] from 1984-88 -- in which the decay rates show a small but statistically significant oscillation with a period of one year and approximately correlated with the earth-sun distance (and with the seasons). Here we report a series of seven measurements of the ^198Au half-life (see [7] for a description of two of these) made by us at various intervals over a period of one aphelion-aphelion cycle. Each measured half-life has a precision of about 0.02%. There is no evidence of any deviation from a constant half-life. [1] J. H. Jenkins et al., Astropart. Phys. 31 407 (2009) [2] J. H. Jenkins et al., Astropart. Phys. 32, 42 (2010) [3] E. Fischbach et al., Space Sci. Rev. 145, 285 (2009) [4] J. Jenkins et al., arxiv:0912:5385v1 [5] D. Alburger et al., Earth and Planet. Sci. Lett. 78, 168 (1986) [6] H. Siegert et al., Appl. Radiat. Isot. 49, 1397 (1998) [7] J. R. Goodwin et al., Eur. Phys. J. A 34, 271 (2007).

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