Astronomers Link a Mysterious Fast Radio Burst With Gravitational Waves for the First Time

A team of colleagues and I have just published evidence in Nature Astronomy for what might be producing mysterious bursts of radio waves coming from distant galaxies, known as fast radio bursts or FRBs.

Two colliding neutron stars—each the super-dense core of an exploded star—produced a burst of gravitational waves when they merged into a “supramassive” neutron star. The team found that two and a half hours later they produced an FRB when the neutron star collapsed into a black hole.

Or so we think. The key piece of evidence that would confirm or refute our theory—an optical or gamma-ray flash coming from the direction of the fast radio burst—vanished almost four years ago. In a few months, we might get another chance to find out if we are correct.

Brief and Powerful

FRBs are incredibly powerful pulses of radio waves from space lasting about a thousandth of a second. Using data from a radio telescope in Australia, the Australian Square Kilometer Array Pathfinder (ASKAP), astronomers have found that most FRBs come from galaxies so distant light takes billions of years to reach us. But what produces these radio wave bursts has been puzzling astronomers since an initial detection in 2007.

The best clue comes from an object in our galaxy known as SGR 1935+2154. It’s a magnetar, which is a neutron star with magnetic fields about a trillion times stronger than a fridge magnet. On April 28, 2020, it produced a violent burst of radio waves—similar to an FRB, although less powerful.

Astronomers have long predicted that two neutron stars—a binary—merging to produce a black hole should also produce a burst of radio waves. The two neutron stars will be highly magnetic, and black holes cannot have magnetic fields. The idea is that the sudden vanishing of magnetic fields when the neutron stars merge and collapse into a black hole produces a fast radio burst. Changing magnetic fields produce electric fields—it’s how most power stations produce electricity. And the huge change in magnetic fields at the time of collapse could produce the intense electromagnetic fields of an FRB.

A black field with two illustrations of galaxies in the foreground, and a yellow beam connecting them
Artist’s impression of a fast radio burst traveling through space and reaching Earth. Image Credit: ESO/M. Kornmesser, CC BY

The Search for the Smoking Gun

To test this idea, Alexandra Moroianu, a masters student at the University of Western Australia, looked for merging neutron stars detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO) in the US. The gravitational waves LIGO searches for are ripples in spacetime, produced by the collisions of two massive objects, such as neutron stars.

LIGO has found two binary neutron star mergers. Crucially, the second, known as GW190425, occurred when a new FRB-hunting telescope called CHIME was also operational. However, being new, it took CHIME two years to release its first batch of data. When it did so, Moroianu quickly identified a fast radio burst called FRB 20190425A which occurred only two and a half hours after GW190425.

Exciting as this was, there was a problem—only one of LIGO’s two detectors was working at the time, making it very uncertain where exactly GW190425 had come from. In fact, there was a five percent chance this could just be a coincidence.

Worse, the Fermi satellite, which could have detected gamma rays from the merger—the “smoking gun” confirming the origin of GW190425—was blocked by Earth at the time.

A nighttime view of white curved pipes arranged in a grid pattern
CHIME, the Canadian Hydrogen Intensity Mapping Experiment, has turned out to be uniquely suited to detecting FRBs. Image Credit: Andre Renard/Dunlap Institute/CHIME Collaboration

Unlikely to Be a Coincidence

However, the critical clue was that FRBs trace the total amount of gas they have passed through. We know this because high-frequency radio waves travel faster through the gas than low-frequency waves, so the time difference between them tells us the amount of gas.

Because we know the average gas density of the universe, we can relate this gas content to distance, which is known as the Macquart relation. And the distance travelled by FRB 20190425A was a near-perfect match for the distance to GW190425. Bingo!

So, have we discovered the source of all FRBs? No. There are not enough merging neutron stars in the universe to explain the number of FRBs—some must still come from magnetars, like SGR 1935+2154 did.

And even with the evidence, there’s still a 1 in 200 chance this could all be a giant coincidence. However, LIGO and two other gravitational wave detectors, Virgo and KAGRA, will turn back on in May this year, and be more sensitive than ever, while CHIME and other radio telescopes are ready to immediately detect any FRBs from neutron star mergers.

In a few months, we may find out if we’ve made a key breakthrough—or if it was just a flash in the pan.

Clancy W. James would like to acknowledge Alexandra Moroianu, the lead author of the study; his co-authors, Linqing Wen, Fiona Panther, Manoj Kovalem (University of Western Australia), Bing Zhang and Shunke Ai (University of Nevada); and his late mentor, Jean-Pierre Macquart, who experimentally verified the gas-distance relation, which is now named after him.The Conversation

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Image Credit: CSIRO/Alex Cherney

Clancy William James
Clancy William James
I got my PhD from the University of Adelaide in 2009 for my thesis entitled "Ultra-High Energy Particle Detection with the Lunar Cherenkov Technique" in the field of astroparticle physics. I then worked from 2009-2011 at Radboud University, the Netherlands, on the LOFAR radio telescope, before moving to Erlangen, Germany at the Friedrich-Alexander University of Erlangen-Nuremberg to work on the ANTARES and KM3NeT neutrino detectors. Since 2017, I have been based at Curtin University, Perth as part of the International Centre of Radio Astronomy Research. My current formal position is "senior lecturer."
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