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Magnetar Confirms: The Vacuum Isn't Empty ⚡ экспресс

Original: "Evidence of magnetospheric vacuum birefringence in the polarized X-rays of a radio magnetar"
arXiv:2509.19446 · 2025-09-23 · CC BY 4.0 · ⏱ 1 min · High Energy HEP Experiment Quantum Physics
The ultra-strong magnetic field of a neutron star transforms empty space into a crystal-like state—and we've finally seen it.
Abstract

Quantum electrodynamics predicts that empty vacuum in an ultra-strong magnetic field can change light's polarization. Scientists studied a magnetar (a neutron star with a record-breaking magnetic field) and saw unusually high polarization of its X-rays, which can only be explained by the vacuum's influence. So, does space around such stars act like a giant prism?

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According to quantum theory, in an ultra-strong magnetic field, emptiness is no longer empty. It becomes akin to a crystal that transmits light differently—like polarized sunglasses filtering out glare. This effect, predicted by pioneers like Richard Feynman, has waited nearly a century for direct proof.

The IXPE X-ray telescope aimed at the magnetar 1E 1547.0-5408—a dead star with a magnetic field billions of times stronger than anything in Earth's labs. Its radiation's polarization—how much the light waves are 'combed'—was measured. At typical medical X-ray energies, it reached 65%, sometimes soaring to 80%.

For comparison: this object's field is 100 billion tesla. It would wipe a credit card's data from the distance of the Moon.

As energy increased, polarization dropped sharply. Only one explanation fits: the vacuum around the star bends light like a crystal. Curiously, the first radio pulsar—also a neutron star—was mistaken for an alien signal by Jocelyn Bell Burnell in 1967. Today we know: the signals are strange, but nature is even stranger.

🎯 The magnetic field of this magnetar is 100 billion times stronger than a fridge magnet's: it can tear apart water molecules from a thousand kilometers away.

Scientists
Emmy NoetherEnrico FermiPaul DiracWolfgang PauliSubrahmanyan ChandrasekharChien-Shiung Wu
Tags
neutron star Standard Model pulsar
Laws
Noether's theoremFermi–Dirac statisticsspin–statistics theoremFermi's golden ruleChandrasekhar limitCPT theorem
Original: arXiv:2509.19446 · CC BY 4.0 · bridge42worlds