### Part 2Theoretical Yield/Rate Expectation

For SNO and Super-K atmospheric neutrino,

Φν : SNO uses Bartolνatmos flux distribution.

Super-K uses Honda νatmos flux distribution.

Pαβ : include ① ν propagation from atmosphere to the earth surface

and ② ν propagation from the earth surface to detector

For ① : Need to calculate

For ② : Melin has the code

I have to do.

(C) ϵ : detection efficiency, can be found from published papers.

(D) : total number of target nucleon.

(E) tlive: total livetime.

All are involved in

SNO and Super-K

atmospheric

neutrino analysis

Quasi-Elastic Scattering

Deep-Inelastic Scattering

Single meson production

Coherent π production

(F) : differential cross section

Quantities needed to check:

Quantities needed to calculate:

Pαβ , theoretical yield or rate as functions

of neutrino oscillation parameters