Another Clue Into the True Nature of Fast Radio Bursts

Fast radio bursts (FRBs) are strange events. They can last only milliseconds, but during that time can outshine a galaxy. Some FRBs are repeaters, meaning that they can occur more than once from the same location, while others seem to occur just once. We still aren’t entirely sure what causes them, or even if the two types have the same cause. But thanks to a collaboration of observations from ground-based radio telescopes and space-based X-ray observatories, we are starting to figure FRBs out.

Most FRBs happen well beyond our galaxy, so while we can pin down their locations, it’s difficult to observe any details about their cause. Then in 2020 we observed a fast radio burst in our galaxy. Subsequent observations found that it originated in the region of a highly magnetized neutron star known as a magnetar. This led to the idea that magnetars were the source of FRBs, possibly through magnetic flares similar to solar flares. But magnetars and Sun-like stars are very different. It still wasn’t clear how a magnetar could release such a tremendous amount of energy so quickly, even with their intense magnetic fields. Now a new study suggests the magnetar’s rotation plays a key role.

The study focuses on the 2020 FRB magnetar. Known as SGR 1935+2154, it is both a magnetar and a pulsar. This means it emits a regular radio pop as it rotates. Pulsars are incredibly regular and are used as a kind of cosmic clock for everything from studying gravitational waves to hypothetical navigation through the galaxy. But over time a pulsar’s rotation slows down as rotational energy radiates away thanks to its magnetic field. By observing this rate of decay, astronomers can better understand the structure of neutron stars and magnetars.

How two magnetar glitches correlate with a fast radio burst. Credit: Hu, Chin-Ping, et al

But sometimes the rate of rotation will shift suddenly. It’s known as a glitch if the rotation suddenly speeds up, and an anti-glitch if it suddenly slows down. These glitches are thought to occur when there’s some kind of sudden structural change in the neutron star, such as a starquake.

In 2022, NASA’s Nuclear Spectroscopic Telescope Array (NUSTAR) spacecraft and the Neutron Star Interior Composition Explorer (NICER) on the international space station both observed another fast radio burst from SGR 1935+2154. Together they had X-ray data on the magnetar before, during, and after the burst. The team then looked at radio observations during the same time and found a dip in the pulsar rotation rate during the burst. This implies a connection between rotation and burst.

Overall what the team observed was a fluttering of X-ray emissions from SGR 1935+2154 a bit before the burst, then a glitch in the rotation, the burst itself, and a return to the regular rotation rate. This is only one observation, but it looks like the magnetar had the magnetic energy ready to release before the burst, and the shift in rotation created the conditions necessary to generate the FRB.

Reference: Hu, Chin-Ping, et al. “Rapid spin changes around a magnetar fast radio burst.” Nature 626 (2024): 500-504.

One Reply to “Another Clue Into the True Nature of Fast Radio Bursts”

  1. Looks like a tremendous observation from coincidental factors involving distances and alignments:

    “Until 2020, almost all known FRBs originated in faraway galaxies. … The team watched the neutron star rotate by virtue of a hotspot on its surface, which likely marks one of the poles of the star’s magnetic field. As the hotspot spins in and out of view — 3.2 times every second! —the neutron star’s brightness appears to pulse.” [Sky&Telescope]

    It potentially explains neutron star superfluid innards and superfluid/hard crust coupling as well as FRBs in magnetars and some rapidly spinning neutron stars.

    The paper mentions a pair-production cascade model that implies the laser analog process [ibid.].

    “That makes sense, though, if the glitch marked a starquake also released charged particles in a brief blast of wind. That wind would have robbed the star of its spin almost as quickly as it had gained it.

    Then, with all of those particles hanging around in an uber-powerful magnetic field — which is far stronger than any we can make on Earth — the conditions were right for an extreme scenario. Particles (specifically, electrons and their antimatter partners, positrons) are born in pairs from the magnetic field’s energy, resulting in what Hu calls an “avalanche.”

    “One electron makes a pair, and then each child makes several more, and so on for several generations, until there are thousands of progenies per electron,” he says. These electron-positron pairs could ultimately be responsible for the sudden burst of radio emission in a “laser-like process,” Hu adds.”

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