Lightning in the Heart of a Galaxy ✛ ✎

Original: "Fast radio bursts as cosmic lightning"
· Parsa Kafashi, Sohrab Rahvar
arXiv:2508.03620 · 2025-08-05 · arXiv non-exclusive · independent analysis · 2 min
A fast radio burst is a discharge of a cosmic capacitor hidden in a black hole's accretion disk.

A radio telescope catches a signal lasting a few milliseconds, and in that instant, energy comparable to what the Sun emits over days is released. This is a fast radio burst, a millisecond radio pulse from a distant galaxy. Since their discovery in 2007, astrophysicists have debated what causes them. A new model offers an unexpected answer: a capacitor discharge.

Around a black hole or neutron star spins an accretion disk, a rotating disk of gas and dust around a compact object. X-ray photons from its inner regions scatter off free electrons, pushing them outward. This creates a charge separation: electrons move to the outer layers, while positive ions remain inside. Thus, a cosmic capacitor is born. The balance between radiation pressure and electrostatic attraction holds the accumulated charge. But if the radiation wavers, a breakdown occurs.

The accumulated charge is comparable to that carried by a terrestrial lightning bolt, but concentrated in an area the size of a city.

The discharge is described as a simple RC circuit: current flows, charge decays, and the radio pulse fades exponentially. For the burst FRB20180725A, the model gives a characteristic decay time of 5.88 milliseconds. The system's dipole moment reaches 1.3×10³⁰ C·m. The theoretical estimate of the accumulated charge for a stellar-mass black hole at Eddington luminosity, the maximum luminosity when radiation and gravity are in equilibrium, is about 10²⁰ C. A combined analysis of observational data and theory allows determining the electron density in the disk, on the order of 10¹⁸ m⁻³, and the energy of X-ray photons, about 10 keV.

The idea of a "cosmic capacitor" has been quantitatively tested against real data for the first time. Previously, fast radio bursts were mainly linked to magnetic processes: magnetars, magnetic reconnection. The new work shows that ordinary accretion of matter onto a compact object is sufficient. This paves the way for a unified explanation of a wide class of bursts. Further refinements to the model, such as accounting for disk rotation, magnetic fields, and turbulence, will help understand why some bursts repeat and others are one-offs. Predictions can be tested through coordinated observations with radio telescopes and X-ray observatories.

A cosmic lightning bolt, flashing at the edge of a black hole, reaches Earth billions of years later. Now we have a tool to read its traces.

The accumulated charge in the model is comparable to the charge carried by a lightning bolt on Earth, but concentrated in a region the size of a city.

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