“New Clues” -Causes of Enigmatic Fast Radio Bursts Remain Unknown

Quasar FRB


“We still have no new clue on whether the origin is artificial or natural,” said Harvard astronomer Avi Loeb about fast radio bursts (FRBs), one of the great astrophysical mysteries. In a rare feat, Caltech researchers have caught a new burst, called FRB 190523, pinpointing its origins to a galaxy 7.9 billion light-years away.

Fast radio bursts (FRBs) are among the most enigmatic and powerful events in the cosmos. Around 80 of these events–intensely bright millisecond-long bursts of radio waves coming from beyond our galaxy–have been witnessed so far, but their causes remain unknown

Despite happening frequently – thousands occur over the entire sky every day – only a couple dozen FRBs have ever been seen. Scientists don’t know what causes them but it must involve incredible energy–equivalent to the amount released by the Sun in 80 years.

In a earlier 2018 study, Harvard’s Loeb had examined the possibility that fast radio bursts come from radio transmitters constructed by an advanced alien civilization — perhaps evidence of powerful energy beams used to propel alien starships. He also theorized that repeater sources are more likely to be such alien signals because natural origin explanations would most likely produce only a single burst.

Identifying the galaxies from which these radio bursts erupt is a critical step toward solving the mystery of what triggers them. Before this new discovery made by Caltech team at Caltech’s Owens Valley Radio Observatory (OVRO), together with the W. M. Keck Observatory in Hawaii, only one other burst, called FRB 121102, had been localized to a host galaxy.

FRB 121102 was reported in 2014 and then later, in 2017, was pinpointed to a galaxy lying 3 billion light-years away. Recently, a second localized FRB was announced on June 27, 2019. Called FRB 180924, this burst was discovered by a team using the Australian Square Kilometer Array Pathfinder and traced to a galaxy about 4 billion light-years away.

“What’s Going On Out There?” -Deepening Mystery of Fast Radio Bursts

FRB 121102 was easiest to find because it continues to burst every few weeks. Most FRBs, however–including the Australian and OVRO finds–just go off once, making the job of finding their host galaxies harder.

“Finding the locations of the one-off FRBs is challenging because it requires a radio telescope that can both discover these extremely short events and locate them with the resolving power of a mile-wide radio dish,” says Vikram Ravi, a new assistant professor of astronomy at Caltech who works with the radio telescopes at OVRO, situated east of the Sierra Nevada mountains in California, focusing on exploring the ephemeral, unseen Universe.

“At OVRO, we built a new array of ten 4.5-meter dishes that collectively act like a mile-wide dish to cover an area on the sky the size of 150 full moons,” he says. “To do this, a powerful digital system ingests and processes an amount of data equivalent to a DVD every second.”

“The Enigma Deepens” –Fast Radio Bursts Detected Repeating Every 16-Days

The new OVRO instrument is called the Deep Synoptic Array-10, with the “10” referring to the number of dishes. This array serves as a stepping stone for the planned Deep Synoptic Array (DSA), funded by the National Science Foundation (NSF), which, when completed by 2021, will ultimately consist of 110 radio dishes.

“The DSA is expected to discover and localize more than 100 FRBs per year,” says Richard Barvainis, program director at the NSF for the Mid-Scale Innovations Program, which is funding the construction of the DSA. “Astronomers have been chasing FRBs for a decade now, and we’re finally drawing a bead on them with new instruments like DSA-10 and, eventually, the full DSA. Now we have a chance of figuring out just what these exotic objects might be.”

The new observations show that the host galaxy for FRB 190523 is similar to our Milky Way. This is a surprise because the previously located FRB 121102 originates from a dwarf galaxy that is forming stars more than a hundred times faster than the Milky Way.

“This finding tells us that every galaxy, even a run-of-the-mill galaxy like our Milky Way, can generate an FRB,” says Ravi.

The discovery also suggests that a leading theory for what causes FRBs–the eruption of plasma from young, highly magnetic neutron stars, or magnetars–may need to be rethought.

“The theory that FRBs come from magnetars was developed in part because the earlier FRB 121102 came from an active star-forming environment, where young magnetars can be formed in the supernovae of massive stars,” says Ravi. “But the host galaxy of FRB 190523 is more mellow in comparison. ”

Ultimately, to solve the mystery of FRBs, astronomers hope to uncover more examples of their host galaxies. “With the full Deep Synoptic Array, we are going to find and localize FRBs every few days,” says Gregg Hallinan, the director of OVRO and a professor of astronomy at Caltech. “This is an exciting time for FRB discoveries.”

The researchers also say that FRBs can be used to study the amount and distribution of matter in our universe, which will tell us more about the environments in which galaxies form and evolve. As radio waves from FRBs head toward Earth, intervening matter causes some of the wavelengths to travel faster than others; the wavelengths become dispersed in the same way that a prism spreads apart light into a rainbow. The amount of dispersion tells astronomers exactly how much matter there is between the FRB sources and Earth.

“Most matter in the universe is diffuse, hot, and outside of galaxies,” says Ravi. “This state of matter, although not ‘dark,’ is difficult to observe directly. However, its effects are clearly imprinted on every FRB, including the one we detected at such a great distance.”

“Something Unexpected Going On” –Astronomers Tune In to Fast Radio Bursts Cosmic Frequency

Getting back to the possibility of alien technology as the ultimate source of FRB’s the Breakthrough Listen team, in a totally separate project, is already looking beyond fast radio bursts, developing AI to analyze a wider range of similarly interesting signals coming from nearby stars and galaxies. AI’s broad pattern recognition abilities could prove especially helpful when nobody knows exactly what an alien signal might look like.

“If AI could flag things that don’t look right or don’t look natural, that might be an interesting thing to do,” said Seth Shostak, a senior astronomer at the SETI Institute in California who was not involved in the Breakthrough Listen study.

Eventually, AI could do much more than just filter radio signals. Shostak speculates that AI could someday automatically search telescope images for unusual visual features that might represent huge alien megastructures from either existing or bygone civilizations.

The Daily Galaxy, Max Goldberg, via Caltech, NBC MACH, and New York Times

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