Neutrino Strikes a Proton: The Most Precise Measurement Yet express

Original: "Measurement of the $$\bar ν_μ-$$Hydrogen Charged-Current Quasi-Elastic Cross Section using the NOvA Near Detector"
· The NOvA Collaboration
arXiv:2608.12293v1 · 2026-08-12 · CC BY 4.0 · 2 min
The NOvA detector caught 35,509 encounters between neutrinos and hydrogen nuclei.

An invisible stream of particles passes through your body every second. These are neutrinos — tiny messengers from distant stars and earthly reactors. Catching them is nearly impossible: they fly through matter like a bullet through fog. But physicists have learned to set traps for them.

In the NOvA experiment, the trap is a detector weighing hundreds of tons, filled with a special liquid. Inside it are many hydrogen atoms — the simplest kind: one proton, one electron. When a muon antineutrino hits a proton dead-on, two particles are born: a muon (a heavy cousin of the electron) and a neutron. Over two years of operation, the detector recorded 35,509 such collisions. That's like counting shooting stars and amassing a whole army.

Neutrinos are so elusive that catching them requires detectors the size of a house. NOvA is located in the United States, and its near detector holds 300 tons of liquid scintillator.

The new measurement gives a number: 0.538 × 10⁻³⁸ square centimeters. This is the area that a neutrino "sees" on a proton. It seems tiny, and it is. But now it's known to four significant figures. Previously, impurities from heavy nuclei in the detector got in the way. Now scientists have subtracted their contribution using separate control datasets. The main uncertainty left is the neutrino flux itself, which is currently measured less precisely.

Such a precise result is like a newly sharpened tool. With it, we can test how well we understand the weak interaction — one of the four forces of nature. And in the future, if the neutrino flux becomes better known, this same measurement will allow us to refine it without additional experiments. So one hunt helps another.

Through the nail of your pinky finger, billions of neutrinos from the Sun pass every second, but over a lifetime, only one or two will ever get stuck in your body.

In Stanisław Lem's novel "Solaris," the planet's ocean communicates with humans via neutrinos, which pass freely through any barrier.

\sigma(\bar{\nu}_\mu H \to \mu^+ n) = 0.538 \pm 0.009 (\text{stat}) \pm 0.010 (\text{syst}) \pm 0.055 (\text{flux}) \times 10^{-38} \text{ cm}^2
Total cross section of the process: muon antineutrino + proton → muon + neutron. The value is given with three types of uncertainties: statistical, systematic, and flux uncertainty.
Scientists
Paul DiracEmmy NoetherWolfgang PauliEnrico FermiChien-Shiung WuEugene Wigner
Concepts
neutron detection techniques