Fast radio blast: studies reveal details about the origin

Fast radio bursts, or FRBs, are powerful, bright emissions of radio waves ranging from a fraction of a millisecond to a few thousandths of a second, each producing energy equivalent to the annual output of the Sun.

Recent research has suggested that some FRBs originate from magnetars, which are neutron stars with extremely strong magnetic fields. A fast radio explosion has been found In the Milky Way It was associated with a magnetar, according to a 2020 study.
But scientists have not yet determined the origins of the cosmic FRBs, which lie billions of light years away. It’s a quandary that has led an international team of scientists to see what it can learn from observations of nearly 1,900 bursts from an active fast radio burst source outside our galaxy called FRB 20201124A, according to study Published September 21 in Nature.

Emissions associated with FRB 20201124A occurred for 82 hours over 54 days in the spring of 2021, making it one of the most energetic fast radio bursts. It was visible through the world’s largest radio telescope – the five hundred-meter aperture spherical radio telescope, or FAST.

During the first 36 days, the study team was surprised to see irregular, short duration differences in the Faraday rotation scale, which measures magnetic field strength and particle density in the vicinity of FRB 20201124A. A larger spin scale means the magnetic field near the source of the radio burst is stronger, more intense, or both, and a smaller scale means the opposite, study co-author and astrophysicist Bing Zhang said via email.

“This does not reflect the onset (of life) of the FRB,” said Zhang, founding director of the Center for Astrophysics at the University of Nevada, Las Vegas. “The FRB source has been there for a long time but has been asleep most of the time. It wakes up sometimes (this time for 54 days) and emits a lot of explosions.”

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The scales rose up and down during that time period, then stopped for the last 18 days before the FRB subsided — “indicating that the magnetic field strength and/or intensity along the line-of-sight in the vicinity of the FRB source varies with time.” “It indicates that the FRB source environment is evolving dynamically, with rapid change in magnetic fields, density, or both.”

“I’m like filming a FRB source environment, and our film revealed a complex, dynamically evolving magneto-environment that had never been imagined before,” Zhang said in a press release.

a physical model Another team of researchers suggested based on observations of FRB 20201124A that FRB came from a binary system about 8,480 light-years away that contains a magnetar and Be star, which is a much hotter, larger star that orbits faster than the Sun, according to a separate study published September 21 in the journal Nature Communications. .

The researchers found that the complex magneto-environment of the radio explosion lies within an astronomical unit (the distance between the Earth and the Sun) from its source.

They also discovered that the explosion originated from a narrow, metal-rich spiral galaxy similar in size to the Milky Way, using the 10-meter Keck telescopes in Mauna Kea, Hawaii. The source of the radio burst is located between the spiral arms of the galaxy where no significant star formation occurs, making it unlikely that the origin was solely a magnetar, according to nature study co-author Sobu Dong, associate professor at the Kavli Institute for Astronomy and Astrophysics. at Peking University.

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“Such an environment is not directly predictable for an isolated magnetar,” Zhang said in a press release. “There might be something else near the FRB engine, maybe it’s a binary companion.”

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The authors said the modeling study should encourage further research on fast radio burst signals from Be star/X-ray binaries.

“These notes brought us back to the drawing board,” Zhang said. “FRBs are clearly more mysterious than we imagined. More multi-wavelength observational campaigns are needed to reveal the nature of these things.”

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