Solar neutrino results from the Sudbury Neutrino Observatory

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作者
Lawson, IT [1 ]
机构
[1] Univ Guelph, Dept Phys, Guelph, ON N1G 2W1, Canada
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中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
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摘要
Solar neutrinos from the decay of B-8 have been detected at the Sudbury Neutrino Observatory (SNO) via the charged-current (CC) reaction on deuterium and the elastic scattering (ES) of electrons. The CC reaction is sensitive exclusively to electron neutrinos while the ES reaction also has a small sensitivity to muon and tau neutrinos. The flux of electron neutrinos from B-8 decays measured by the CC reaction and ES reaction, assuming no flavour transformation, will be presented. These flux measurements provide evidence that there is a non-electron flavour active neutrino component in the solar flux. The total flux of active B-8 neutrinos will be presented and shown to be in good agreement with predictions of solar models.
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页码:308 / 310
页数:3
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