Black hole superradiance efficiently produces ultralight axions with masses around 10⁻¹² eV, forming a gravitational atom and leading to the emission of nearly monochromatic gravitational waves. Unlike previous constraints based on measurements of individual black hole spins, this work performs a population analysis: it considers gravitational-wave signals from ~10⁸ black holes in the Milky Way and the stochastic background from axion clouds throughout the Universe. Taking into account systematic uncertainties in population properties, the potential sensitivity of detectors such as LIGO, Einstein Telescope, Cosmic Explorer, and a hypothetical high-frequency Weber bar has been computed. It is shown that LIGO can reliably probe axion masses from ~10⁻¹³ eV to 4·10⁻¹² eV. By extending the population to black holes with masses slightly below 5 M☉ — as hinted by LIGO observations — the sensitivity reaches 10⁻¹¹ eV, and future high-frequency instruments in optimistic scenarios could surpass the 10⁻¹⁰ eV threshold and approach the mass range accessible to direct axion dark matter experiments.
Black holes aren't silent abysses, but nature's tuning forks. Their rapid spin, predicted by Roger Penrose, makes spacetime itself sing, producing a stream of the lightest particles—axions. These accumulate around the hole, like sound in a concert hall, and begin to oscillate in unison. Thus a cloud forms, radiating gravitational waves of a single unchanging note—a cosmic tuning fork sounding for millions of years.
Previously, scientists tried to catch such a song from individual holes by monitoring their spin. Now they've taken into account that in our Milky Way alone there are about a hundred million such tuning forks. Their combined choir produces a hum that detectors built by Rainer Weiss (LIGO) can already pick up. The next generation of instruments, like the Einstein Telescope, will be able to distinguish notes from even lighter axions, bringing us closer to solving the dark matter puzzle.
🎯 The gravitational waves from axions are astonishingly pure—like a tuning fork note sounding for millions of years without a single flaw.
🎬 In 'Interstellar,' gravitational waves served as a bridge across time; here, we're catching the real melody sung by black holes.