‘Cosmic whistle’ releases lots of energy in gamma rays

(Credit: Getty Images)

Astronomers have discovered that the mysterious “cosmic whistles” known as fast radio bursts can pack a serious punch, in some cases releasing a billion times more energy in gamma rays than they do in radio waves.

They can even rival the stellar cataclysms known as supernovae in their explosive power.

The discovery, the first-ever finding of non-radio emission from any fast radio burst, drastically raises the stakes for models of fast radio bursts and is expected to further energize efforts by astronomers to chase down and identify long-lived counterparts to fast radio bursts using X-ray, optical, and radio telescopes.

Fast radio bursts, which astronomers refer to as FRBs, were first discovered in 2007, and in the years since radio astronomers have detected a few dozen of these events. Although they last mere milliseconds at any single frequency, their great distances from Earth—and large quantities of intervening plasma—delay their arrival at lower frequencies, spreading the signal out over a second or more and yielding a distinctive downward-swooping “whistle” across the typical radio receiver band.

Listen to the “cosmic whistle:”

“This discovery revolutionizes our picture of FRBs, some of which apparently manifest as both a whistle and a bang,” says coauthor Derek Fox, a professor of astronomy and astrophysics at Penn State. The radio whistle can be detected by ground-based radio telescopes, while the gamma-ray bang can be picked up by high-energy satellites like NASA’s Swift mission.

“Rate and distance estimates for FRBs suggest that, whatever they are, they are a relatively common phenomenon, occurring somewhere in the universe more than 2,000 times a day.”

To test general relativity, use fast radio bursts

Efforts to identify FRB counterparts began soon after their discovery but have all come up empty until now. In a paper published in Astrophysical Journal Letters the team, led by physics graduate student James DeLaunay, reports bright gamma-ray emission from the fast radio burst FRB 131104, named after the date it occurred, November 4, 2013.

“I started this search for FRB counterparts without expecting to find anything,” says DeLaunay. “This burst was the first that even had useful data to analyze. When I saw that it showed a possible gamma-ray counterpart, I couldn’t believe my luck!”

FRB 131104
Discovery of the gamma-ray counterpart to FRB 131104, in wide-angle and zoomed-in views of Swift gamma-ray data. The black circle indicates the area of the sky that Parkes Observatory was observing when it detected FRB 131104. Within the circle there is a single prominent red peak, the signal of the gamma-ray counterpart. Colors in the image indicate the signal-to-noise level at each position; the counterpart’s signal-to-noise level is 4.2. The Swift exposure was taken over 300 seconds starting 7 seconds before FRB 131104. While the wide-field image is only a small portion of Swift’s very large field of view, it is large enough to fit eight full moons lined up from top to bottom of the image. (Credit: J. J. DeLaunay/Penn State)

Discovery of the gamma-ray “bang” from FRB 131104, the first non-radio counterpart to any FRB, was made possible by NASA’s Earth-orbiting Swift satellite, which was observing the exact part of the sky where FRB 131104 occurred as the burst was detected by the Parkes Observatory radio telescope in Parkes, Australia.

“Swift is always watching the sky for bursts of X-rays and gamma rays,” says Neil Gehrels, the mission’s Principal Investigator and chief of the Astroparticle Physics Laboratory at NASA’s Goddard Space Flight Center. “What a delight it was to catch this flash from one of the mysterious fast radio bursts.”

Can fast radio bursts root out dark matter?

“Although theorists had anticipated that FRBs might be accompanied by gamma rays, the gamma-ray emission we see from FRB 131104 is surprisingly long-lasting and bright,” Fox says. The duration of the gamma-ray emission, at two to six minutes, is many times the millisecond duration of the radio emission. And the gamma-ray emission from FRB 131104 outshines its radio emissions by more than a billion times, dramatically raising estimates of the burst’s energy requirements and suggesting severe consequences for the burst’s surroundings and host galaxy.

Two common models for gamma-ray emission from FRBs exist: one invoking magnetic flare events from magnetars—highly magnetized neutron stars that are the dense remnants of collapsed stars—and another invoking the catastrophic merger of two neutron stars, colliding to form a black hole.

According to coauthor Kohta Murase, a Penn State professor and theorist, “The energy release we see is challenging for the magnetar model unless the burst is relatively nearby. The long timescale of the gamma-ray emission, while unexpected in both models, might be possible in a merger event if we observe the merger from the side, in an off-axis scenario.”

“In fact, the energy and timescale of the gamma-ray emission is a better match to some types of supernovae, or to some of the supermassive black hole accretion events that Swift has seen,” Fox says. “The problem is that no existing models predict that we would see an FRB in these cases.”

The bright gamma-ray emission from FRB 131104 suggests that the burst, and others like it, might be accompanied by long-lived X-ray, optical, or radio emissions. Such counterparts are dependably seen in the wake of comparably energetic cosmic explosions, including both stellar-scale cataclysms—supernovae, magnetar flares, and gamma-ray bursts—and episodic or continuous accretion activity of the supermassive black holes that commonly lurk in the centers of galaxies.

In fact, Swift X-ray and optical observations were carried out two days after FRB 131104, thanks to prompt analysis by radio astronomers (who were not aware of the gamma-ray counterpart) and a nimble response from the Swift mission operations team, headquartered at Penn State. In spite of this relatively well-coordinated response, no long-lived X-ray, ultraviolet, or optical counterpart was seen.

The authors hope to participate in future campaigns aimed at discovering more FRB counterparts, and in this way, finally revealing the sources responsible for these ubiquitous and mysterious events. “Ideally, these campaigns would begin soon after the burst and would continue for several weeks afterward to make sure nothing gets missed. Maybe we’ll get even luckier next time,” DeLaunay says.

The research effort received financial support from Penn State’s Office of the Senior Vice President for Research, Penn State’s Eberly College of Science, and the Penn State Institute for Gravitation and the Cosmos. Members of the research team also received support from the US National Science Foundation and NASA.

Source: Penn State