does anyone know why atmospheric neutrinos are detected more frequently horizontally for high energies???? any help would be appreciated, thanks!
What's an atmospheric neutrino? And what does it mean to detect one horizontally? These may have obvious meanings in a specialized field, but they don't make sense to me a priori.
I know what a neutrino is, by the way, and where they come from and how they're detected. It's the adjectives "atmospheric" and "horizontal" that aren't makign sense to me here.
atmospheric neutrinos are produced in the atmosphere by pion decays (I think) and im doing a project using data from a detector in japan, Super kamiokande. |dw:1355442019463:dw| I've got to try and explain why theres a higher neutrino flux when cos theta=0, as opposed to any other angle i.e when theta =Pi/4 And i havent got a clue =s
Hmm, ok. So you're not looking at solar neutrinos? Because those would come preferentially from the direction of the Sun, of course. If you're looking at neutrinos from pion decay, then I would say they are most likely the debris from a cosmic ray air shower: http://en.wikipedia.org/wiki/Air_shower_%28physics%29 Now I don't know much about air showers, but I would guess if you look in a direction in which you look through a thicker slice of the Earth's atmosphere, you will observe more debris, just because the original cosmic ray has a better chance of hitting something, and the debris particles have a better chance of hitting something else. That is, if you look parallel to the surface of the Earth, out towards space, you are looking through a thicker slice of atmosphere: |dw:1355516200283:dw| Maybe that helps? Anyway, if your source if air showers, maybe look up some of their characteristics. If your source is lower-energy charged particles (which doesn't seem super likely, as they aren't likely to be able to do nuclear reactions) then the Earth's magnetic field may make a difference. For air showers I think the particles are too energetic to notice the Earth's field, but I'm not sure.
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