In space, near neutron stars, the ultra-dense remnants of dead stars, an ocean of incredible force crashes. Its 'water' is a magnetic field trillions of times stronger than Earth's, and its 'waves' are electromagnetic oscillations. Charged particles here are like surfers: some drift helplessly, but others catch the crest and accelerate to near light speed.
For a long time, it was thought that such 'surfing' required a wave as strong as the star's own magnetic field. But computer simulations revealed that chaos and those coveted crests arise at just a quarter of that strength. Then a small group of particles surges ahead, leaving the rest far behind.
It's these accelerated lucky few that likely generate fast radio bursts — dazzling signals whose energy in an instant outshines the Sun's daily output. Such bursts were first detected by Jocelyn Bell Burnell in 1967 while she was studying pulsars — rotating neutron stars. The idea of dead stars with strong fields was proposed back in the 1930s by Fritz Zwicky. Thus, the invisible cosmic surf reveals the universe's secrets.
In a single millisecond, a fast radio burst emits more energy than our Sun does in an entire day.