Vacuum oscillation probability
The signature expression of neutrino oscillation. The observation that this probability is non-zero forced the Standard Model to accommodate non-degenerate neutrino masses.
See PMNS matrix →Evidence-based research portal
Ninety-five years of experimental and theoretical neutrino physics. Organized as a navigable evidence base — papers, experiments, timelines, curated research threads, and editorial writing.
Topics
What a neutrino is, flavors, mass, helicity, and the Standard Model context.
PMNS matrix, mixing angles, mass ordering, and MSW matter effects.
Cherenkov detection, CEvNS, liquid scintillator, tritium beta endpoint.
Solar, atmospheric, reactor, accelerator, supernova, and geoneutrinos.
Cosmic neutrino background, early-universe neutrinos, dark-matter bounds.
Neutrinovoltaics, the Master Equation, and energy harvesting from the invisible spectrum.
Formulas
The expression that made oscillation measurable. The coherent cross-section that opened low-energy neutrino detection. The engineering-integration framework that connects them to applied research.
The signature expression of neutrino oscillation. The observation that this probability is non-zero forced the Standard Model to accommodate non-degenerate neutrino masses.
See PMNS matrix →Coherent elastic neutrino-nucleus scattering scales quadratically with neutron number — the largest neutrino cross-section below 50 MeV. Predicted by Freedman 1974, observed by COHERENT 2017.
See CEvNS concept →The engineering-integration framework for neutrinovoltaic conversion — packaging CEvNS, cosmic-ray muon flux, ambient electromagnetic, and thermal contributions into a single expression for device output power.
See full concept page →Editorial
Selected articles from the editorial programme — fundamentals, historical breakthroughs, contemporary experiments, and the applied-research frontier.
An examination of the integrated expression relating invisible radiation flux, cross-sections, material volume, and efficiency to device output power — anchored in established neutrino physics.
China's 20-kiloton liquid-scintillator detector has delivered its first oscillation spectrum measurement. Here is what the data look like — and what they will tell us over the next five years.
How the 1998 Super-Kamiokande atmospheric result and the 2001 SNO solar measurement forced the Standard Model to accommodate massive neutrinos.
An introduction to the neutrino — the lightest known massive particle, invisible to electromagnetism, a witness to the Sun's core and the first second after the Big Bang.
What you'll find
From Pauli 1930 to JUNO 2025 — with DOI/arXiv references, filters, and citation export.
Fifteen milestone experiments at launch, each with objective, method, results, and significance.
Curated sequences — the oscillation evidence, the solar neutrino problem, the mass hunt.
A 3-flavor oscillation calculator, a CEvNS cross-section plot, and a Master Equation simulator.