ar X iv : h ep - p h / 99 09 26 4 v 1 6 S ep 1 99 9 Atmospheric
نویسنده
چکیده
The early history of the atmospheric neutrino anomaly is closely tied to the growth of grand unified theories. Grand unified theories inspired the experimental search for proton decay which led to large well shielded detectors. The primary background to proton decay was due to atmospheric neutrinos so they were studied in some detail. Neutrino oscillations figured prominently at the first workshop on grand unification. About half of the IMB paper at that meeting 1 was devoted to the question of studying neutrino oscillations with atmospheric neutrinos.
منابع مشابه
ar X iv : h ep - p h / 99 09 26 3 v 1 6 S ep 1 99 9
To study diffractive photon production at HERA, we compute the projection of the γ * γ impact-factor on the BFKL leading-order eigenfunctions E n,ν for non-zero transfer. This calculation supplements former ones performed for n = 0. We provide an expression for n = ±2 and check that all the other components are zero.
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