That makes sense, though, if the glitch marked a starquake also released charged particles in a brief blast of wind. That wind would have robbed the star of its spin almost as quickly as it had gained it.
Then, with all of those particles hanging around in an uber-powerful magnetic field — which is far stronger than any we can make on Earth — the conditions were right for an extreme scenario. Particles (specifically, electrons and their antimatter partners, positrons) are born in pairs from the magnetic field's energy, resulting in what Hu calls an “avalanche.”
“One electron makes a pair, and then each child makes several more, and so on for several generations, until there are thousands of progenies per electron,” he says. These electron-positron pairs could ultimately be responsible for the sudden burst of radio emission in a “laser-like process,” Hu adds.