JUNO · REACTOR ν̄ₑ
Neutrino oscillation
JUNO — the Jiangmen Underground Neutrino Observatory — watches electron antineutrinos from two nuclear power plants about 52.5 km away. At that baseline the survival probability carries both the slow “solar” oscillation (Δm²₂₁) and the fast “atmospheric” one (Δm²₃₁); the interference between them is what lets JUNO pin down the neutrino mass ordering. Drag the parameters and watch the curve move.
━ normal ordering━ inverted orderingL = 52.5 km
Survival P(E)
Power |F|²
Sine (FST, imag)
Cosine (FCT, real)
▲ = PDG best-fit (click to snap). The spectra change mainly with Δm²₃₁ and the resolution; finite resolution low-pass-filters the atmospheric peak. θ₂₃, δ_CP are absent (no reactor effect).