Fast Radio Bursts (FRB's) From Sources Unknown Could Help Map Intergalactic Matter

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• published: 19 Feb 2014
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Brief and bright, fast and furious, uncommonly pure. Fast radio bursts have baffled astronomers since their discovery in 2007, but now they are revealing their true nature. Two new studies suggest that FRBs are as common as dirt, that they produce more energy in a millisecond than the sun does in a million years, and that their single, intense flash of radio waves may be created when a neutron star is severed from its magnetic field as it collapses into a black hole. This explanation has also led to a more evocative name -- blitzars -- after the German word blitz for lightning. In 2007, Duncan Lorimer and David Narkevic of West Virginia University in Morgantown discovered the first fast radio burst. (See: Extragalactic radio burst puzzles astronomers - http://www.newscientist.com/article/dn12699-extragalactic-radio-burst-puzzles-astronomers.html) Although many pulsars -- spinning magnetic stars -- give off brief periodic flashes of radio waves, the "Lorimer burst" was a singular event, lasting just a few milliseconds. What's more, it seemed to originate a few billion light years away, much more distant than the furthest pulsars that we can detect, suggesting that it must be exceptionally powerful. The plot thickened in 2012 when Evan Keane, now at the Max Planck Institute for Radio Astronomy in Bonn, Germany, and his colleague detected a similar event. (See: 'On the origin of a highly-dispersed coherent radio burst' - http://arxiv.org/abs/1206.4135) Their comparative analysis suggests that FRBs are frequent, with one being produced in every galaxy in the universe roughly every 1000 years. The fact that only six have been detected so far reflects their very short lifetime and the fact that astronomers can't keep an eye on the whole sky all the time. So what could give rise to an FRB? Several ideas have been put forward, including a collision between neutron stars -- the ultradense, magnetic remains of supernova explosions -- but most theories fail to explain why FRBs emit purely at radio wavelengths. Other energetic cosmic explosions shine across a much broader spectrum, including in visible light, x-rays and gamma rays.. But another study details a scenario that can account for this. Heino Falcke of Radboud University in Nijmegen, the Netherlands, and Luciano Rezzolla of the Max Planck Institute for Gravitational Physics in Potsdam, Germany, suggest that an FRB occurs when the supernova explosion of a giant star leaves behind a compact neutron star that is slightly overweight. The object's own gravity would cause it to collapse into a black hole, the researchers say, if not for the centrifugal effect of its fast rotation. But within a few million years, the interaction of the neutron star's magnetic field with the surrounding interstellar material slows the spin. Eventually, gravity wins and the star turns into a black hole after all. "When the black hole forms, the magnetic field will be cut off from the star and snap like rubber bands," explains Falcke. "This can produce the observed giant radio flashes." By contrast, other types of radiation, which would come from the star itself rather than around it, cannot escape the gravitational collapse. Thornton doesn't want to comment on Falcke and Rezzolla's idea before the paper has been accepted for publication in a refereed journal. "Our favourite explanation for FRBs is a giant burst from a magnetar -- a highly magnetised type of neutron star," he says. These explosions are expected to happen more or less as frequently as the mysterious radio bursts. But Falcke and The object's own gravity would cause it to collapse into a black hole, the researchers say, if not for the centrifugal effect of its fast rotation. But within a few million years, the interaction of the neutron star's magnetic field with the surrounding interstellar material slows the spin. Eventually, gravity wins and the star turns into a black hole after all. "When the black hole forms, the magnetic field will be cut off from the star and snap like rubber bands," explains Falcke. "This can produce the observed giant radio flashes." By contrast, other types of radiation, which would come from the star itself rather than around it, cannot escape the gravitational collapse. Thornton doesn't want to comment on Falcke and Rezzolla's idea before the paper has been accepted for publication in a refereed journal. "Our favourite explanation for FRBs is a giant burst from a magnetar -- a highly magnetised type of neutron star," he says. These explosions are expected to happen more or less as frequently as the mysterious radio bursts. But Falcke and Rezzolla have already coined the term "blitzar" to describe FRBs. have already coined the term "blitzar" to describe FRBs. A Brilliant Flash, Then Nothing: New "Fast Radio Bursts" Mystify Astronomers http://www.scientificamerican.com/article/a-brilliant-flash-then-nothing-new-fast-radio-bursts-mystify-astronomers/