Author/Authors :
Jenkins، نويسنده , , Jere H. and Herminghuysen، نويسنده , , Kevin R. and Blue، نويسنده , , Thomas E. and Fischbach، نويسنده , , Ephraim and Javorsek II، نويسنده , , Daniel and Kauffman، نويسنده , , Andrew C. and Mundy، نويسنده , , Daniel W. and Sturrock، نويسنده , , Peter A. and Talnagi، نويسنده , , Joseph W.، نويسنده ,
Abstract :
Additional experimental evidence is presented in support of the recent hypothesis that a possible solar influence could explain fluctuations observed in the measured decay rates of some isotopes. These data were obtained during routine weekly calibrations of an instrument used for radiological safety at The Ohio State University Research Reactor using 36Cl. The detector system used was based on a Geiger–Müller gas detector, which is a robust detector system with very low susceptibility to environmental changes. A clear annual variation is evident in the data, with a maximum relative count rate observed in January/February, and a minimum relative count rate observed in July/August, for seven successive years from July 2005 to June 2011. This annual variation is not likely to have arisen from changes in the detector surroundings, as we show here.
Keywords :
Nuclear decay fluctuations , beta decay , Solar influence , Gas detectors