Why ratio atmospheric ##\nu_\mu : \nu_e = 2:1##

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The expected ratio of atmospheric neutrino fluxes, R = (νμ + ν̅μ) / (νe + ν̅e) = 2, is based on the decay processes of pions and muons. However, this ratio may not hold true universally due to factors such as muon decay before interaction and variations in the zenith angle and energy levels. The discussion highlights that low-energy particles dominate the spectrum, impacting the observed neutrino fluxes. Additionally, other particle interactions contributing to muon pair production complicate the ratio. Overall, the ratio of 2 is considered an approximation rather than a definitive value.
ChrisVer
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Why is the ratio of atmospheric neutrino fluxes expected to be:
R= \frac{\nu_\mu + \bar{\nu}_\mu}{\nu_e +\bar{\nu}_e} =2
for no Neutrino Oscillations?
An answer that I found gives:
\pi \rightarrow \mu \nu_{\mu} \rightarrow e \nu_e \nu_\mu \nu_\mu
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 \theta and their energies (boost).
 
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In general, the spectrum is dominated by low-energetic particles, and low-energetic muons decay in flight.
You also have some other particles producing muon pairs. That ratio of 2 is only an approximation.
 

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