Some of the brightest flashes in the universe may be coming into focus. So-called fast radio bursts are enigmatic, ultra-brief, ultra-powerful bursts of energy coming from distant galaxies. They last for only a fraction of a second, but in that time they emit the energy of perhaps 500 million suns.
James Cordes, an astronomer at Cornell University, thinks he can help explain not only the power of these repeating bursts, but also the seeming irregularity of their eruptions.
He has found that clouds of charged gas, or plasma, in an FRB’s host galaxy could magnify the burst by as much as a factor of 100.
The gas would not always magnify the source; at times, there may be no lensing at all. At these times, the source would appear to be dormant. “It is possible that FRB sources are always active but appear to fluctuate greatly in the brightness of their bursts because of dynamic lensing,” Cordes said.
The plasma just needs to be in the right configuration to focus the light reaching us.
Brian Metzger, an astronomer at Columbia University, said that if we could confirm that plasma lenses are responsible for the repeating FRB’s erratic on-off blast cycle, “this would be telling us something important about the environment through which the FRB is passing and thus a strong hint as to their origin.”
Astronomers have seen similar activity in other situations, said Robert Main, an astronomer at the University of Toronto. “Several pulsars have now shown the effects of plasma lensing, which Jim proposes could be happening in FRBs,” he said. When this tail passes in front of the pulsar (as seen from Earth), the plasma focuses the pulsar’s light, causing its radio emission to appear as much as 30 times brighter. The effect was first observed in 2011 by Anna Bilous, an astronomer at the University of Amsterdam.
“The light rays from the two copies of the FRB would constructively interfere with each other in a way that could help us peer at the FRB with super high resolution.” Plasma lenses might even provide us with a tool allowing us to see the source of a burst.
Yet well-studied magentas close to home are nowhere near as energetic as the distant repeater. Even if the source is amplified, FRBs would still be more energetic than any known magentas.