Why There Are No Classical Particles of Light ✎ express

Original: "No classical particle limit for massless quanta"
· Riccardo Falcone, Simon Fuchs
arXiv:2606.14632 · 2026-06-12 · arXiv non-exclusive · independent analysis · 1 min
Theory forbids the existence of classical massless particles, such as light corpuscles.

A billiard game would be strange if the balls had no mass. They wouldn't collide but would pass through each other, ignoring obstacles. That's roughly what it looks like to imagine light as a stream of classical particles — tiny elastic bodies flying in straight lines. A new proof puts an end to that picture.

The authors built a rigorous mathematical framework: how, in general, a quantum object can turn into something familiar and classical. They didn't tie themselves to a specific instrument or medium — only to the most general requirements of reasonableness and spacetime symmetry. It turned out that for massless particles, these requirements are incompatible. Spacetime simply doesn't allow them to become classical.

A massless particle always moves at the speed of light, and in any reference frame, you cannot stop it. A classical object must have a trajectory, but here it cannot be defined.

This doesn't forbid light from exhibiting wave properties or generating electromagnetic fields. But a separate classical particle — a 'classical photon'—will never exist. The same conclusion applies to hypothetical gravitons: if they are massless, they cannot become classical. Thus, the quantum world reminds us once again: familiar intuition often fails here.

If a photon had even a tiny mass, it could become a classical particle. But then light from distant stars would reach us at different speeds, and we would see stars of different colors simultaneously.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterNiels Bohr
Concepts
classical gravity classical limit massless particle no-cloning theorem newtonian limit massless scalar field non singular cosmology background independent quantum gravity particle number quantum field theory in curved spacetime null energy condition spacetime emergence flat space Klein-Gordon equation