The Cosmic Capacitor: Unraveling Fast Radio Bursts ✛ ✎

Original: "Fast radio bursts as cosmic lightning"
· Parsa Kafashi, Sohrab Rahvar
arXiv:2508.03620 · 2025-08-05 · arXiv non-exclusive · independent analysis · 1 min
A new model explains fast radio bursts as electrical discharges in disks around black holes.

Fast radio bursts are flashes of radio waves lasting mere milliseconds, yet they pack as much energy as the Sun produces in a day. Their nature long remained a mystery. Now astrophysicists have a simple idea: these signals are nothing more than giant electrical sparks in the disks around black holes.

A searing-hot gas disk whirls around the black hole. Intense radiation acts like a gusty wind, blowing lightweight electrons outward while the heavier nuclei stay put. The disk becomes something like a thundercloud — except the electrical voltage builds up not for lightning, but for a radio burst.

A millisecond discharge unleashes as much energy as thousands of earthly lightning strikes, packed into an area no bigger than a major city.

When the voltage breaks down, the accumulated charge is released in an instant, and we detect a fast radio burst.

Scientists tested the model on a known burst and found an exact match with its spectral portrait — the way energy is distributed across frequencies. This allowed them to calculate densities and charges. A similar mechanism likely operates for neutron stars — the ultra-dense remnants of exploded stars.

In the radio band, such a flash momentarily outshines an entire galaxy, though you can't see it with the naked eye.

The energy released in one millisecond of a fast radio burst can exceed the energy the Sun radiates over several days.

S_0(t) = \frac{Q^2 l^2}{32\pi^2 T^4 \epsilon_0 c^3} \frac{\sin^2\theta}{d_L^2} e^{-2t/T} \left(1+\frac{r}{3tc}\right)^3
Dependence of the received flux on time, charge, distance, and cosmological expansion
Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesAdam Riess
Concepts
black hole outburst fast radio burst radio loud quasar black hole accretion winds quasi periodic eruptions flare outburst Accretion disk debris disk starburst x ray burst hawking radiation mechanism gravitational wave frequency central engine stellar flares microquasar nuclear reaction mass gap solar eruption ultra fast outflow iron k alpha reverberation