Magnetar Confirms: The Vacuum Isn't Empty ✛

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
The ultra-strong magnetic field of a neutron star transforms empty space into a crystal-like state, and we've finally seen it.

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.

B_{\mathrm{crit}} = \frac{m_e^2 c^3}{e \hbar} \approx 4.4 \times 10^{13} \ \mathrm{G}
The critical QED magnetic field: at this strength, the energy of the magnetic interaction of an electron is comparable to its rest mass. Above this threshold, vacuum begins to noticeably affect the propagation of light.
\Delta n \propto \frac{\alpha}{45\pi} \left( \frac{B}{B_{\mathrm{crit}}} \right)^2
The difference in refractive indices for two polarizations of light in vacuum placed in a magnetic field B. The effect is quadratic in the field and becomes significant only near magnetars.
Scientists
Michael FaradayHendrik LorentzSubrahmanyan ChandrasekharJocelyn Bell BurnellWolfgang PauliJohn Archibald Wheeler
Concepts
magnetar magnetic radiation effects polarization measurement vacuum birefringence magnetar pulsations in grb ixpe vacuum polarization pulsar radio pulsar X-ray radiation x ray pulse neutron star light emission cosmic birefringence rotation measure stellar flares magnetar plasma geometry pulsar phenomena fast radio burst xray polarization electromagnetic radiation