Polarization - United States

This illustration depicts Faraday rotation in the afterglow of a gamma-ray burst. A powerful jet (upper left) sends polarized radio waves outward through the thin wall of a surrounding bubble of magnetized gas called an HII region. As the light passes through this material, its polarization angle is twisted by the magnetic field. Because the effect is stronger at longer wavelengths, the red and blue waves, which represent different radio wavelengths, exit the bubble oscillating in different directions. By measuring this difference, astronomers were able to map the magnetic environment surrounding GRB 260310A for the first time. Image credit: NSF / AUI / NRAO / M. Weiss

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Astronomers Detect Gamma-Ray Burst’s Magnetic Fingerprint

July 17, 2026

Using NSF’s Very Large Array (VLA), astronomers made the first radio detection of polarized light and Faraday rotation…

The Blueprint

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US makes room-temperature multiferroic for low-energy computing

April 30, 2026

Engineers at Rice University in the U.S. have developed a new room-temperature multiferroic material that shows a 10-fold…

A muon particle passing through lead in a cloud chamber. Image credit: Jino John 1996 / CC BY-SA 4.0.

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Long-Standing Muon Mystery May Be Settled

April 25, 2026

A new high-precision calculation of a key component underpinning the magnetic moment of the muon, a heavier cousin…