When Light Gets Heavy: The Unexpected Decay of a Photon ✛ ✎ ✦

Original: "Lorentz-Violating Photon Decay into Neutrinos and Constraints from PeV Photon Stability"
· Zurab Kepuladze
arXiv:2607.10404 · 2026-07-11 · arXiv non-exclusive · independent analysis · 1 min
A super-energetic photon can give birth to a pair of neutrinos if the speed of light in space slightly fluctuates.

A photon is like a soap bubble: weightless, swift, indestructible. It can cross the universe unchanged. But in the far reaches of space, where the speed of light might fluctuate slightly, the bubble suddenly gets heavy. And then, as if under its own weight, it pops into two even lighter bubbles — neutrinos. These ghostly twins pass through planets like a knife through butter.

The idea that the speed of light is not constant dates back to Lorentz. Today, it may explain anomalies in the gamma-ray emission from the Crab Nebula — the remnant of a supernova with a spinning pulsar.

Recent calculations combining the laws of electricity and magnetism with quantum field theory have shown: super-energetic cosmic rays from the Crab Nebula challenge the Standard Model of physics, as described by Einstein and Sunyaev. If a photon acquires a tiny mass, it can transform into two neutrinos.

To calculate the probability of such an event, scientists combined the laws of electromagnetism and quantum fields.

The decay is extremely rare and takes a thousand years — a cosmic blink. But future observatories, sensitive to both light and neutrinos, will be able to detect the sudden disappearance of photons using methods of ultra-precise light measurement. A dip in the gamma-ray glow would be the first signal: the universe is more complex than we thought.

A "heavier" photon weighs 10,000 times less than an electron, but that's enough for it to split into two neutrinos over a thousand years, a cosmic instant.

m_{\text{eff}}^2 = \delta E_\gamma^2
The effective mass grows proportionally to the photon energy and the parameter δ, which characterizes the deviation of the speed of light from a constant.
\Gamma_\gamma = \frac{2\alpha}{3} \frac{m_{\text{eff}}^6}{k_0} \sum_{\ell} a_{\nu_\ell}^2
The decay probability depends on the sixth power of the effective mass, making the process extremely sensitive to the magnitude of the violation: even a slight shift δ sharply slows the decay.
Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterPaul Dirac
Concepts
neutrino decay Lorentz Invariance Violation decay constant lepton flavor violation antineutrino neutrino quantum decoherence neutron mass positronium electron positron pair branching fraction neutron star mass limit electron capture nuclear stability two photon absorption tau lepton particle antiparticle pair newtonian limit Einstein's photoelectric equation Lorentz transformations neutral pion