Hunting Ghost Particles from a Supernova ✎ express

Original: "Direct Detection of Millicharged Particles from Supernovae"
arXiv:2606.11310 · 2026-06-09 · arXiv non-exclusive · independent analysis · 1 min
Physicists have found a way to catch mysterious particles that reach Earth with a delay — like an echo of the neutrino burst.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

When a massive star dies, its core collapses, and a supernova explosion occurs. The cataclysm births streams of particles — like ripples from a thrown stone. The first to arrive are swift neutrinos, which pierce the Earth, hardly interacting. Then, hours later, ghost particles with a tiny charge appear.

Just as a delayed swell rolls in after a storm, these particles signal when the neutrino burst has already faded.

Underground detectors catch faint flashes from these particles colliding with electrons. Because of their mass, they travel slower than neutrinos and arrive later, like an echo. Detectors could register up to tens of events per year — dozens of times more than previous estimates. Perhaps these ghost particles are dark matter — the invisible scaffolding of the Universe.

Neutrinos from supernova 1987A outpaced light by three hours — proving they have a tiny mass.

Scientists
Paul DiracStephen HawkingJacob BekensteinDavid DeutschErwin SchrödingerJohn Stewart Bell
Concepts
supernova jets neutrino emission neutron star super kamiokande neutrino telescope supernova 1987a hyper kamiokande cms detector coronal mass ejection pulsar wind nebula neutron star light emission nuclear recoil markov chain monte carlo superconducting detector NOAA CPC superdense matter chandra km3net sub neptune stellar explosion microscopic black hole