Fourier spectrum analysis of the new solar neutrino capture rate data for the Homestake experiment
نویسنده
چکیده
All four solar neutrino experiments (Homestake, Kamiokande, GALLEX, SAGE) observe a deficit of solar neutrinos compared to the predictions of the Standard Solar Model. Additionally, any two of the three classes of solar neutrino experiments indicate that the largest suppression is in the middle of the solar neutrino spectrum (the Be-7 line and the lower part of the B-8 spectrum)[1]. Among these four experiments the Homestake experiment is taking data for almost 25 years [2,3]. The reliability of the radiochemical method for detecting solar neutrinos has been tested recently by the GALLEX experiment [1].
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تاریخ انتشار 1996