Neutrino Oscillation Probability Calculator
Find the two-flavor neutrino oscillation probability P=sin²(2θ)sin²(1.267Δm²L/E) for a given mixing angle, mass-squared splitting, baseline, and energy.
👻 What is the Neutrino Oscillation Probability Calculator?
This neutrino oscillation probability calculator finds P(νa→νb)=sin²(2θ)sin²(1.267Δm²L/E), the standard two-flavor formula for how likely a neutrino is to change flavor after traveling a given baseline. Enter the mixing angle, mass-squared splitting, baseline distance, and neutrino energy, and it returns the oscillation and survival probabilities.
Using the T2K-like default values (θ=45°, Δm²=2.5×10⁻³ eV², L=295 km, E=0.6 GeV), this calculator reproduces a near-maximal oscillation probability close to 1, matching the real experiment's design goal of sitting near the oscillation maximum.
Neutrino oscillation is direct experimental proof that neutrinos have mass, since oscillation is only possible when the mass-squared splitting Δm² between mass eigenstates is nonzero.
This calculator is useful for particle physics students studying neutrino mixing, the PMNS framework, and long-baseline oscillation experiments like T2K, NOvA, and Super-Kamiokande.
📐 Formula
📖 How to Use This Calculator
Steps
💡 Example Calculations
Example 1 - T2K-like long-baseline experiment
Example 2 - Smaller mixing angle
Example 3 - Very short baseline (near zero oscillation)
❓ Frequently Asked Questions
🔗 Related Calculators
What is neutrino oscillation?
Neutrino oscillation is the quantum mechanical phenomenon where a neutrino created in one flavor (electron, muon, or tau) has a probability of being detected as a different flavor after traveling some distance, caused by neutrinos having mass and their flavor and mass eigenstates being different (mixed) quantum states.
What is the formula for two-flavor neutrino oscillation probability?
P(νa→νb) = sin²(2θ)sin²(1.267Δm²L/E), where θ is the mixing angle, Δm² is the mass-squared splitting in eV², L is the baseline distance in kilometres, and E is the neutrino energy in GeV. The constant 1.267 makes these specific units work directly.
What does the mixing angle θ represent?
The mixing angle describes how much the flavor eigenstates (electron, muon, tau neutrino) overlap with the mass eigenstates. θ=45° gives 'maximal mixing' (the largest possible oscillation amplitude, sin²(2θ)=1), while θ=0° or θ=90° means no mixing (no oscillation) between those two states.
What does Δm² represent?
Δm² is the difference of the squares of two neutrino mass eigenstates (in eV²). Because oscillation only depends on this squared mass difference (not the individual absolute masses), oscillation experiments cannot directly measure absolute neutrino masses, only mass-squared splittings.
What is a realistic example of neutrino oscillation parameters?
The T2K long-baseline experiment uses a baseline of about 295 km and a muon neutrino beam energy around 0.6 GeV, probing the atmospheric mass-squared splitting Δm²≈2.5×10⁻³ eV², producing a large, near-maximal oscillation probability at that baseline and energy.
Why does the oscillation probability depend on L/E rather than L and E separately?
The oscillation phase 1.267Δm²L/E depends only on the ratio L/E (for fixed Δm²), because a neutrino accumulates oscillation phase proportionally to how long it travels relative to its energy (inversely related to its de Broglie wavelength), this is why experiments are often designed around a specific L/E to probe a particular Δm².
Is the two-flavor formula exact for real neutrinos?
No, real neutrino oscillation involves three flavors and three mixing angles (the PMNS matrix) plus two independent mass-squared splittings and a CP-violating phase. The two-flavor formula used here is an excellent approximation when one splitting and one angle dominate a given experiment's sensitivity, the standard simplification used in most introductory treatments.
What is the survival probability?
The survival probability, 1−P(νa→νb), is the probability that a neutrino created in flavor a is still detected in flavor a (has not oscillated away) after traveling the given baseline, this calculator reports it directly alongside the oscillation (flavor-change) probability.
What evidence confirmed neutrino oscillation experimentally?
The Super-Kamiokande experiment's 1998 measurement of atmospheric neutrino flavor ratios, and the Sudbury Neutrino Observatory's measurement of solar neutrino flavors, both provided decisive evidence for oscillation, work recognized with the 2015 Nobel Prize in Physics (Takaaki Kajita and Arthur B. McDonald).
Does neutrino oscillation prove neutrinos have mass?
Yes, oscillation can only occur if Δm²≠0, meaning at least two neutrino mass eigenstates have different (and therefore nonzero) masses, direct proof that neutrinos are not massless as originally assumed in the Standard Model.