Gravitational waves refine cosmic expansion rate экспресс

Оригинал: "First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis"
arXiv:2601.04774v1 · 2026-01-08 · CC BY 4.0 · 1 мин
Combining gravitational wave signals with galaxy surveys yields a more precise measurement of how fast the universe is growing.

Measuring the universe’s expansion is like timing a race when the track stretches. Neutron star mergers act as standard sirens: their gravitational waves ring out with a known “volume,” so fainter signals mean greater distance.

A new study paired the siren from merger GW170817 with a galaxy map tracing matter, including dark matter (invisible mass first detected by Vera Rubin). The result: the Hubble constant (named after Edwin Hubble) is 67.9 km/s per megaparsec — so a galaxy 3.26 million light-years away recedes at that speed — with just 6.4% uncertainty.

This value eases a cosmic dispute: the early universe’s afterglow suggests slower expansion, while nearby exploding stars point to faster. The new number falls between them, highlighting the strength of cross-checking methods. Remarkably, the spacetime ripples from GW170817 jiggled our detectors by less than a proton’s width, yet clocked the universe’s growth.

The term 'standard siren' echoes 'standard candle,' but while candles use light, sirens use gravitational waves — a clever twist on an old cosmic yardstick.

Учёные
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Понятия
измерение постоянной Хаббла стандартная сирена постоянная Хаббла лиза детектирование гравитационных волн корень герца gw170817 сигма усреднение сигнала закон хаббла космический исследователь космологические параметры LIGO снижение шума детектора гравитационных волн измерение космических расстояний космический телескоп Джеймса Уэбба пять сигм стандартная свеча телескоп Эйнштейна событие