Answers are grounded in this paper and cite their sources.
We present a systematic study of potential long-baseline (distances >300 km) neutrino-oscillation experiments performed with ν_μ and {ν}_μ beams from the Fermilab Main Injector (〈E_ν〉{}10--20 GeV). The effects of matter enhancement are included where appropriate. We find that there are three key variables for such an experiment: the length of the baseline, the muon energy threshold, and the minimum measurable oscillation probability. An advantage in one of these variables can easily be neglected by a disadvantage in one of the others. Finally, for any long-baseline experiment at these energies to conclusively confirm or refute the interpretation of the atmospheric neutrino deficit as neutrino oscillations it must have a low energy threshold and a low minimum measurable oscillation probabilty.
No takes yet. Share an insight, caveat, or question.
Bernstein et al. (1991) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: