Black Holes: Neutrino Factories ✎ express

Original: "On the Blueprint of Active Galaxies Producing Neutrinos"
· Chen Li, Francis Halzen
arXiv:2607.27658v1 · 2026-07-30 · arXiv non-exclusive · independent analysis · 2 min
In the cores of active galaxies, supermassive black holes act like giant factories, turning X-rays into streams of elusive neutrinos, unraveling the mystery of the cosmic particle background.

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At the centers of many galaxies lurk giant black holes. They are surrounded by dense clouds of hot plasma that emit a powerful X-ray glow. In a cramped region, just a few gravitational radii (the radii of Karl Schwarzschild — the boundary beyond which even light disappears), protons are accelerated to monstrous energies. This is the entrance to nature’s factory.

When an accelerated proton collides with an X-ray photon, a reaction kicks off: $p + \gamma \rightarrow \Delta \rightarrow n + \pi^+$. Here’s how it plays out: the short-lived delta particle decays into a neutron and a pion, and the pion splits into a neutrino and a muon. Neutrinos fly outward, carrying energies of tens of teraelectronvolts (that’s trillions of times more energetic than visible light particles). Meanwhile, gamma rays get absorbed by the dense plasma, and from the outside, the source appears silent. Neutrinos become the factory’s only voice.

Neutrinos barely notice matter. They can travel through the entire Earth without touching a single atom. Every second, about a hundred billion neutrinos— mostly from the Sun— pass through a square centimeter of your skin.

Data from the IceCube neutrino telescope, built deep in the Antarctic ice, paint a clear picture. The captured neutrino flux turned out to be directly proportional to the X-ray brightness from a compact region no larger than ten radii of Karl Schwarzschild. This allows us to confidently say: the main sources of such particles are the active cores of galaxies, where black holes grind the energy of infalling matter into directed beams. Most likely, these hidden factories create the very diffuse background of neutrinos and extragalactic cosmic rays that has puzzled scientists for decades. The conveyor belt runs nonstop.

This is the essence of multimessenger astronomy— looking at the sky with different eyes. If our eyes could detect neutrinos, the whole sky would glow with a uniform light, while gamma-ray surveys would be empty voids. Two “windows” complement each other, letting us peer into the very heart of cosmic factories.

Neutrinos are so elusive that it would take a lead slab a light-year thick to guarantee stopping just one.

p + \gamma \rightarrow \Delta \rightarrow n + \pi^+
A proton (p) collides with an X-ray photon (γ), forming a short-lived Δ particle, which then decays into a neutron (n) and a pion (π+).
Scientists
Stephen HawkingJacob BekensteinFritz ZwickyKarl SchwarzschildSubrahmanyan ChandrasekharJocelyn Bell Burnell
Concepts
neutrino sources black hole neutrino source active galactic nucleus active galactic nucleus red dots X-ray radiation ultraluminous x ray source neutron star light emission radio galaxy xmm newton icecube ultra fast outflow nucleosynthesis obscured agn central engine radio loud quasar neutron star changing agn activity torus black hole corona antineutrino