Gravitational Waves Leave an Eternal Imprint ⚡ экспресс
The gravitational-wave memory effect — a nonlinear prediction of general relativity — manifests as a residual displacement of initially comoving observers after a burst of radiation passes. To search for it in LIGO–Virgo–KAGRA data, the GWTC-5.0 catalog of binary black hole mergers was used. Unlike previous works relying on Bayesian factors, this study employs hierarchical Bayesian inference, free of their shortcomings. The estimated memory amplification factor — the constant multiplying the contribution from the supermomentum flux to the strain — is 0.26^{+4.09}_{-4.08} (68% confidence interval), consistent with the theoretical value of 1. It is predicted that to constrain this parameter away from zero at the 1σ level, about 2000 gravitational-wave detections will be needed.
Gravitational waves are the very trembling of space, born when black holes or other massive bodies collide. Their main oddity isn't that they pass through us, but that they permanently alter the curvature of spacetime and the distances between everything they touch. Just like a footprint remains on wet sand even after the wave has receded, a gravitational wave leaves an indelible trace—a minuscule but eternal shift.
This memory effect was predicted by Einstein, but catching a single such "dent" in space is impossible—it's billions of times fainter than what detectors like LIGO pick up. So scientists got clever: they stacked data from a hundred mergers and, using careful statistical analysis, teased out the collective contribution. It turned out the effect's magnitude matches theory exactly, though the uncertainty is still large, and to nail it, we need to wait for roughly 2000 events.
From a single black hole merger, the distance between Earth and the Sun would change by less than a proton's diameter. Yet, accumulating thousands of such "footsteps," the cosmos will retain their cumulative imprint—and we will see not just ripples, but the very memory of the universe for the first time.
🎯 From a single black hole merger, the memory effect would change the distance between Earth and the Sun by less than the diameter of a proton.