Please use this identifier to cite or link to this item: https://apo.ansto.gov.au/dspace/handle/10238/12258
Title: On decay constants and orbital distance to the Sun—part II: beta minus decay
Authors: Pommé, S
Stroh, H
Paepen, J
Van Ammel, R
Marouli, M
Altzitzoglou, A
Hult, M
Kossert, K
Nähle, O
Schrader, H
Juget, F
Bailat, C
Nedjadi, Y
Bochud, F
Buchillier, T
Michotte, M
Courte, S
van Rooy, MW
van Staden, MJ
Lubbe, L
Simpson, BRS
Fazio, A
De Felice, D
Jackson, TW
van Wyngaardt, WM
Reinhard, MI
Golya, J
Bourke, S
Roy, T
Galea, R
Keightley, JD
Ferreira, KM
Collins, SM
Ceccatelli, A
Verheyen, L
Bruggeman, M
Vodenik, M
Korun, M
Chisté, V
Amiot, MN
Keywords: Decay
Sun
Beta decay
Isotopes
Radionuclide metrology
Metrology
Oscillations
Earth planet
Distance
Issue Date: 28-Nov-2016
Publisher: IOP Publishing
Citation: Pommé, S., Stroh, H., Paepen, J., Van Ammel, R., Marouli, M., Altzitzoglou, T., Hult, M., Kossert, K., Nähle, O., Schrader, H., Juget, F., Bailat, C., Nedjadi, Y., Bochud, F., Buchillier, T., Michotte, C., Courte, S., van Rooy, M. W., van Staden, M. J., Lubbe, J., Simpson, B. R. S., Fazio, A., De Felice, P., Jackson, T. W., Van Wyngaardt, W. M., Reinhard, M. I., Golya, J., Bourke, S., Roy, T., Galea, R., Keightley, J. D., Ferreira, K. M., Collins, S. M., Ceccatelli, A., Verheyen, L., Bruggeman, M., Vodenik, B., Korun, M., Chisté, V., & Amiot, M.-N. (2016). On decay constants and orbital distance to the Sun—part II: beta minus decay. Metrologia, 54(1), 19-35. doi:10.1088/1681-7575/54/1/19
Abstract: Claims that proximity to the Sun causes variations of decay constants at the permille level have been investigated for beta-minus decaying nuclides. Repeated activity measurements of 3H, 14C, 60Co, 85Kr, 90Sr, 124Sb, 134Cs, 137Cs, and 154Eu sources were performed over periods of 259 d up to 5 decades at various nuclear metrology institutes. Residuals from the exponential decay curves were inspected for annual oscillations. Systematic deviations from a purely exponential decay curve differ in amplitude and phase from one data set to another and appear attributable to instabilities in the instrumentation and measurement conditions. Oscillations in phase with Earth's orbital distance to the Sun could not be observed within 10−4–10−5 range precision. The most stable activity measurements of β− decaying sources set an upper limit of 0.003%–0.007% to the amplitude of annual oscillations in the decay rate. There are no apparent indications for systematic oscillations at a level of weeks or months. © The Authors CC BY 3.0 licence
URI: https://iopscience.iop.org/article/10.1088/1681-7575/54/1/19
https://apo.ansto.gov.au/dspace/handle/10238/12258
ISSN: 1681-7575
Appears in Collections:Journal Articles



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