Popular

Plasma Sphere Explains Magnetars and Radio Bursts ⚡ экспресс

Original: "Magnetic plasmoid explosions in the context of magnetar giant flares and fast radio bursts"
arXiv:2601.00441v2 · 2026-01-01 · CC BY 4.0 · ⏱ 1 min · High Energy Plasma Physics
A magnetic plasma sphere explosion explains two mysteries at once: giant magnetar flares and mysterious radio pulses from other galaxies.
Links in the knowledge graph 1

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

A magnetar is a neutron star with a magnetic field a quadrillion times stronger than Earth's. Sometimes it ejects a blob of plasma, like a tiny balloon with thousands of invisible springs bouncing around inside. The material flies apart at nearly the speed of light, and the flare itself outshines an entire galaxy in a tenth of a second.

What happens next depends on the sphere's density. If it's denser than the surrounding space, it creates an X-ray or gamma-ray burst — a giant magnetar flare. But if the sphere is thinner, yet its magnetic field is wound up tighter, it gives rise to a fast radio burst, a radio wave that can cross half the universe. These signals baffled astronomers for a long time. The more tightly the magnetic field is wound inside the sphere, the slower it expands.

This simple model, for the first time, ties two cosmic wonders together with unified physics. The first pulsar — a cousin of magnetars — was discovered by Jocelyn Bell Burnell; today her successors are unraveling the secrets of the most powerful explosions in the universe.

🎯 A magnetar flare can outshine all the stars in a galaxy combined in just a tenth of a second.

🎬 Like in the movie 'Contact,' fast radio bursts were initially mistaken for alien signals.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
neutron star pulsar speed of light
Laws
Doppler effectprinciple of constancy of the speed of lightmass–energy equivalenceMaxwell's equationsLorentz transformationsFermi–Dirac statistics
Original: arXiv:2601.00441v2 · CC BY 4.0 · bridge42worlds