Astronomers shed new light on formation of mysterious fast radio bursts

International team reports on a radio pulsar phase of a Galactic magnetar that emitted a fast radio burst in 2020; observations suggest unique origins for “bursts” and “pulses,” which adds to FRB formation theory.

More than 15 years after the discovery of fast radio bursts (FRBs) – millisecond-long, deep-space cosmic explosions of electromagnetic radiation – astronomers worldwide have been combing the universe to uncover clues about how and why they form.

Nearly all FRBs identified have originated in deep space outside our Milky Way galaxy. That is until April 2020, when the first Galactic FRB, named FRB 20200428, was detected. This FRB was produced by a magnetar (SGR J1935+2154), a dense, city-sized neutron star with an incredibly powerful magnetic field.

This groundbreaking discovery led some to believe that FRBs identified at cosmological distances outside our galaxy may also be produced by magnetars. However, the smoking gun for such a scenario, a rotation period due to the spin of the magnetar, has so far escaped detection. New research into SGR J1935+2154 sheds light on this curious discrepancy.

In the July 28 issue of the journal Science Advances, an international team of scientists, including UNLV astrophysicist Bing Zhang, report on continued monitoring of SGR J1935+2154 following the April 2020 FRB, and the discovery of another cosmological phenomenon known as a radio pulsar phase five months later.

Unraveling a Cosmological Conundrum

To aid them in their quest for answers, astronomers rely in part on powerful radio telescopes like the massive Five-hundred-meter Aperture Spherical radio Telescope (FAST) in China to track FRBs and other deep-space activity. Using FAST, astronomers observed that FRB 20200428 and the later pulsar phase originated from different regions within the scope of the magnetar, which hints towards different origins.

“FAST detected 795 pulses in 16.5 hours over 13 days from the source,” said Weiwei Zhu, lead author of the paper from National Astronomical Observatory of China (NAOC). “These pulses show different observational properties from the bursts observed from the source.”

This dichotomy in emission modes from the region of a magnetosphere helps astronomers understand how – and where – FRBs and related phenomena occur within our galaxy and perhaps also those at further cosmological distances.

Radio pulses are cosmic electromagnetic explosions, similar to FRBs, but typically emit a brightness roughly 10 orders of magnitude less than an FRB. Pulses are typically observed not in magnetars but in other rotating neutron stars known as pulsars. According to Zhang, a corresponding author on the paper and director of the Nevada Center for Astrophysics, most magnetars do not emit radio pulses most of the time, probably due to their extremely strong magnetic fields. But, as was the case with SGR J1935+2154, some of them become temporary radio pulsars after some bursting activities.

Another trait that makes bursts and pulses different are their emission “phases”, i.e. the time window where radio emission is emitted in each period of emission.

“Like pulses in radio pulsars, the magnetar pulses are emitted within a narrow phase window within the period,” said Zhang. “This is the well-known `lighthouse’ effect, namely, the emission beam sweeps the line of sight once a period and only during a short interval in time in each period. One can then observe the pulsed radio emission.”

Zhang said the April 2020 FRB, and several later, less energetic bursts were emitted in random phases not within the pulse window identified in the pulsar phase.

“This strongly suggests that pulses and bursts originate from different locations within the magnetar magnetosphere, suggesting possibly different emission mechanisms between pulses and bursts,” he said.

Implications for Cosmological FRBs

Such a detailed observation of a Galactic FRB source sheds light on the mysterious FRBs prevailing at cosmological distances.

Many sources of cosmological FRBs – those occurring outside our galaxy – have been observed to repeat. In some instances, FAST has detected thousands of repeated bursts from a few sources. Deep searches for seconds-level periodicity have been carried out using these bursts in the past and so far no period was discovered.

According to Zhang, this casts doubt on the popular idea that repeating FRBs are powered by magnetars in the past.

“Our discovery that bursts tend to be generated in random phases provides a natural interpretation to the non-detection of periodicity from repeating FRBs,” he said. “For unknown reasons, bursts tend to be emitted in all directions from a magnetar, making it impossible to identify periods from FRB sources.”

Publication Details

The study, “A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism”, appeared July 28 in the journal Science Advances and includes 37 co-authors from 10 co-authors from 17 institutions. Besides NAOC and UNLV, primary collaborating institutions include Peking University and Beijing Normal University from China, George Washington University from the U.S., and Sabancı University from Turkey.

Journal: Science Advances
DOI: 10.1126/sciadv.adf6198
Method of Research: Observational study
Subject of Research: Not applicable
Article Title: A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism
Article Publication Date:28-Jul-2023

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