- #1
ChrisVer
Gold Member
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Why is the ratio of atmospheric neutrino fluxes expected to be:
[itex]R= \frac{\nu_\mu + \bar{\nu}_\mu}{\nu_e +\bar{\nu}_e} =2[/itex]
for no Neutrino Oscillations?
An answer that I found gives:
[itex] \pi \rightarrow \mu \nu_{\mu} \rightarrow e \nu_e \nu_\mu \nu_\mu[/itex]
But I think this is "wrong" in general, because the muons can reach the Earth before interacting... at least it should be a function of the Zenith angle [itex]\theta[/itex] and their energies (boost).
[itex]R= \frac{\nu_\mu + \bar{\nu}_\mu}{\nu_e +\bar{\nu}_e} =2[/itex]
for no Neutrino Oscillations?
An answer that I found gives:
[itex] \pi \rightarrow \mu \nu_{\mu} \rightarrow e \nu_e \nu_\mu \nu_\mu[/itex]
But I think this is "wrong" in general, because the muons can reach the Earth before interacting... at least it should be a function of the Zenith angle [itex]\theta[/itex] and their energies (boost).