How Neutron Stars Ignite Cosmic Searchlights ✎ express

Original: "Hadronic Processes, Plasma Evolution and Neutrino Emission in Magnetic Towers of Neutron-Star Merger Remnants"
· Rostom Mbarek, Jiaxi Wu, Elias R. Most
arXiv:2605.24083 · 2026-05-22 · arXiv non-exclusive · independent analysis · 2 min
When neutron stars collide, they create magnetic towers where protons, like billiard balls, trigger an avalanche of particles and neutrinos.

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Two neutron stars (the remnants of dead stars, compressed to the size of a city but weighing as much as the Sun) spiral around each other and eventually collide. At that moment, something between a black hole and a super-powered magnet is born: a field billions of times stronger than that of the most powerful MRI machine. From the poles of this object erupt 'magnetic towers'—streams of field lines resembling tornadoes, but instead of wind, the very fabric of spacetime is twisted within them.

Inside these towers, magnetic lines tear and reconnect, like rubber bands that are stretched and then suddenly released. This process, called magnetic reconnection, releases energy. But until now, it was unclear which particles become the 'projectiles' in this accelerator. It turns out that electrons and their antimatter counterparts, positrons, are not enough. They quickly lose speed, like a cyclist trying to accelerate through thick syrup: radiation instantly quenches their transverse motion. Something heavier is needed.

The magnetic field of such a 'tower' reaches 10¹⁵–10¹⁶ gauss. For comparison, a refrigerator magnet produces about 100 gauss. The difference is like between a whisper and the roar of a jet engine.

Enter protons. They are almost two thousand times more massive than electrons, and when the field accelerates them to even half the speed of light, things get interesting. Colliding with each other, protons produce short-lived particles — pions. These, in turn, decay into gamma-ray photons, which then produce electron-positron pairs. The result is a cascade reminiscent of a chain reaction in billiards: one ball hits two, those hit four, and so on. Each proton collision produces, on average, four new electron-positron pairs. This avalanche fills the tower with matter that later lights up as a powerful gamma-ray burst.

In addition to gamma-ray light, neutrinos are born — nearly undetectable particles that pass through planets like light through glass. Their energy can reach 300 million electronvolts — hundreds of times more than neutrinos from the Sun.

This mechanism not only explains the brightness of gamma-ray bursts but also predicts a neutrino 'tail' that could be caught by detectors like IceCube at the South Pole. If the source is within our galaxy or its nearest satellites (up to a hundred thousand light-years away), the signal would stand out against other cosmic noise. Thus, protons born in the fiery vortex of a merger become messengers of the most energetic events in the universe.

The magnetic field in the polar towers is so strong that it can affect the structure of vacuum, spawning particle pairs literally out of nothing.

Scientists
Bernhard RiemannJoseph WeberKarl SchwarzschildKip ThorneRainer WeissAlbert Einstein
Concepts
neutron star binary merger neutron star nuclear fusion magnetorotational supernova pulsar hadron electron positron pair pulsar wind nebula magnetar photon pair generation pion neutrino decay magnetar pulsations in grb high energy neutrino polaron fusion energy r process magnetic reconnection magnetic radiation effects quark decay processes