The Universe is full of tantalising mysteries. They include bizarre fast radio bursts that flash out of the sky in less time than some supercomputers can do a single calculation. They’ve found a way to confound astronomers and simply delight space fans. Let’s explore the cosmos, and investigate these intergalactic enigmas when they emit a cosmic spray of energy – bursts from the fast radio burst enigma.
A fast radio burst is an extremely short, very intense flash of radio-frequency radiation that puts out as much energy as the sun does in days. Roughly 30 of these bursts have been observed to date, coming from all over the cosmos; they appear and disappear in a blink of a cosmic eye, which is why they have become a major current topic of astronomy – an erupting fad.
For the first time, we have a tool to change the way we think about these cosmic explosions The team analysed polarised light from the FRB to study how the bursts are produced, their birth environments and how they travelled through the vast cosmos to reach us. To analyse the polarised light, the team looked at the angle of the electromagnetic waves as they vibrate, which provides clues about where the burst was emitted from and the cosmic environment the burst traversed to get here.
The identity of the source of the FRBs remains a huge mystery; is it something cataclysmic that destroys its source, or is it from something that survives the cosmic explosion? The difference between repeating and non-repeating FRBs might point to the answer. Some of the sources show multiple bursts, while others seem to make a single, dramatic fireworks show before quietly disappearing.
Some of the more common bursts have been linked to magnetars, or strongly magnetised neutron stars. But the extremely rare, non-repeating bursts might be produced by blitzars, a fireworks-like ending of a neutron star’s life, in which it collapses into a black hole, triggering a fast radio burst as it does.
Today, the emergence of the Canadian Hydrogen Intensity Mapping Experiment (CHIME) has pushed FRB research into a wholly new phase. Designed to scan the whole visible sky through all the year using a technique pioneered by Anderson’s team, it will enable us to discover non-repeating FRBs more quickly and effectively than ever before. This leads to opportunities to probe the environments in which these bursts originate in unprecedented detail by looking at the polarisation of light from an FRB as it transforms between the burst’s emission and reception.
In the case of CHIME, an analysis of the detections is leading to another surprising conclusion: non-repeating FRBs probably are not the same as repeating ones, or are possibly evolved versions that originated in less extreme environments. We already know that FRBs are a diverse class of phenomena, and that there are different cosmic theatres from which they emerge. But, from their predominant transport properties, it is possible they’re each bursting forth with their own stories to tell.
The search to understand FRBs is a story of a puzzle being pieced together, or a mosaic being made, one piece at a time. We’ve come a long way, but we still have a long way to go. We’ve got the CHIMEs and the appetite for innovative research strategies to get us there. But we still don’t know what we’re searching for. But understanding FRBs is almost tangential to what we’ll learn once we find them. What we’ll learn is less about these bursts themselves than our incredible tools and what those tools can tell us about the cosmos. What we’ll begin to understand is our seemingly insignificant place in the footnotes of the universe.
FRBs are beacons not only in that they help us explore space and time, but because they showcase the endless human urge to understand the Universe, even as it expands and evolves far beyond our ability to comprehend it.
Understanding the FRB sprint, and the possibilities attached to it, is just the beginning. After all, if advances in astronomy are propelled by bursts, then peeling back the layers on these temporal surprises holds the potential to help answer some of the oldest questions about our Universe.
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