بنيت نظرية فرمي على افتراض أن الكتلة السكونية للنترينو تساوي الصفر. و قد جرت محاولات
عديدة لإختبار صحة الفرضية تجريبيا، إلا أن جميعها باءت بالفشل.
في مؤتمر النترينو المنعقد عام ١٩٩٠ ، اقترح D.W.Sciama النظرية التالية: إن الفوتونات الصادرة
عن تفكك نترينوهات المادة المظلمة في درب التبانة تؤلف المنبع الرئيسي للتشرد الواسع الانتشار في
الوسط بين النجوم.
No English abstract
References used
W.N. Cottengham and D.A.Greenwood,Introduction Nuclear Physics Cambridge Uniersity Publications1987
K.S.Krame, Introductory Nuclear Physics.John-wiely and Sons Inc1987
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