The Cosmic Top That Brakes Too Fast express

Original: "Search for continuous gravitational waves from the pulsar J0435+3233"
arXiv:2607.18219 · 2026-07-20 · CC BY 4.0 · 2 min
Pulsar J0435+3233 spins like crazy but slows down at a record rate, and that's our chance to hear its gravitational song.

A spinning top that makes a hundred turns per second suddenly starts losing speed dramatically — much faster than any known top. That's exactly what pulsar J0435+3233 is doing. It's a dead star, crushed to the size of a city, but whirling at a furious rate. Its period is less than 10 milliseconds, and it has set a record: never before have we seen such a fast pulsar slow down so much (its spin-down exceeds $10^{-12}$ Hz/s).

Such a sharp slowdown is like the screech of brakes on a speeding car. But instead of sound, it could create ripples in spacetime — gravitational waves. Scientists from the LIGO collaboration analyzed observational data and tried to catch this "whisper" from J0435+3233. They looked for a signal at exactly twice the pulsar's spin frequency, in a narrow band around it, and at frequencies corresponding to special oscillations of stellar matter — the so-called r-modes.

The pulsar is 1.2 kiloparsecs away — about 4000 light-years. If it were emitting gravitational waves, only a tiny fraction of that energy would reach Earth, comparable to the trembling of a blade of grass caused by a truck passing a kilometer away.

The detectors picked up nothing. But the silence is also a result. It allowed setting an upper limit on the gravitational wave amplitude: $h_0 = 5.8 \times 10^{-27}$. That's ten times stricter than the limit you could get from the spin-down alone. In other words, if the pulsar were slowing down only due to gravitational wave emission, its "oblateness" (deviation from a perfect sphere) would be no more than $1.6 \times 10^{-8}$. That's in a physically very interesting range, like having a perfectly smooth billiard ball the size of Earth with no bump taller than a couple of centimeters.

If the observed slowdown is really caused by internal processes rather than gravitational radiation, then J0435+3233 becomes the first pulsar where the "braking limit" is beaten by more than an order of magnitude. That means nature has a surprise in store: perhaps some other mechanism is at work inside the star, unrelated to gravitational waves.

So, the top isn't just slowing down: it's doing so mysteriously. We didn't hear its gravitational screech, but we did get a glimpse into the very heart of the physics of ultra-dense objects. And who knows, maybe next time, when LIGO becomes even more sensitive, we'll finally catch that cosmic rhythm.

If pulsar J0435+3233 were a perfectly smooth sphere, its rotation wouldn't produce gravitational waves. You need at least a tiny "bump" on the surface — a deviation from sphericity. The upper limit on such a bump for this pulsar is less than the thickness of a human hair on an object the size of Manhattan.

In Carl Sagan's novel "Contact," a signal from an alien civilization is hidden in the pulsations of a neutron star — maybe someday we'll find something more than just gravitational waves in such data.

h_0 = 5.8 \times 10^{-27}
Upper limit on the gravitational wave amplitude from pulsar J0435+3233 at a frequency of 216 Hz. This is 10 times lower than the limit derived from the spin-down rate.
Scientists
Wolfgang PauliEmmy NoetherDavid CharbonneauIsaac NewtonJohannes KeplerWilliam Borucki
Concepts
high frequency gravitational waves continuous gravitational wave gw190814 cosmic explorer virgo gw170817 nanograv spin wave pulsar glitch radio pulsar taiji lisa tianqin kagra black hole ringdown overtones jwst red sources gwtc standard siren ligo virgo kagra wormhole resonance