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Physics 2016

Observation of Gravitational Waves from a Binary Black Hole Merger

B. P. Abbott et al. (LIGO Scientific Collaboration & Virgo)

Two black holes collided a billion years ago, and we heard spacetime itself ring.

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In depth · the introduction

Scientists directly detected gravitational waves for the first time — ripples in spacetime set off when two black holes crashed together over a billion years ago.

The idea, unpacked

A century ago, Einstein predicted that violent events in space — like two black holes colliding — should send ripples through spacetime itself, stretching and squashing space as they spread outward, like waves on a pond. But the ripples reaching Earth would be fantastically faint, and for a hundred years no one could measure something so small.

Where it came from

LIGO is the machine built to catch them: two enormous L-shaped detectors with arms four kilometres long, using laser beams to measure those arms' lengths to almost impossible precision. When a gravitational wave rolls past, it lengthens one arm and shortens the other by a hair's breadth — far less, actually, than the width of an atom. On 14 September 2015, both detectors, far apart, twitched in exactly the same way at almost the same instant. They had felt the tremor from two black holes merging more than a billion light-years away — a century, almost to the year, after Einstein's prediction.

Why it mattered

This confirmed the last untested major prediction of Einstein's general relativity, a hundred years after he made it. More than that, it gave astronomy a brand-new sense: until now we'd only ever “seen” the universe with light. Now we can “hear” it through gravity, letting us detect things — like colliding black holes — that give off no light at all.

Why it's called a “chirp”

As the two black holes spiral closer, they whirl around each other faster and faster, and the gravitational wave they send out climbs in pitch and volume — exactly like a bird's rising chirp. Turn the signal into sound and that's what you hear: a swoop upward, then a thump as they merge. How fast the pitch rises gives away how heavy the black holes are. Set their masses below and watch the chirp change shape.

A gravitational-wave strain plotted against time: an oscillation whose frequency and amplitude both rise — the chirp — ending in a brief merger spike and a quickly fading ringdown. Two sliders set the black-hole masses; lighter masses stretch the chirp out over more cycles, heavier masses make it short and end at a lower frequency.

What came next

GW150914 was just the first. LIGO and its partner detectors have now caught dozens more black-hole collisions, and in 2017 they heard two neutron stars merge — an event telescopes also saw as a burst of light, revealing it as a cosmic forge where gold and platinum are made. Each detection is a note in a kind of music from the dark side of the universe, the part that gives off no light at all.

The original document
Original source text
B. P. Abbott et al. (LIGO Scientific Collaboration and Virgo Collaboration) · Phys. Rev. Lett. 116, 061102 (2016)
Detection
On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal.
The signal
The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0 × 10⁻²¹. It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole.
The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater than 5.1σ.
The source
The source lies at a luminosity distance of 410 (+160 −180) Mpc … The initial black hole masses are 36 and 29 solar masses, and the final black hole mass is 62 solar masses, with 3.0 solar masses radiated in gravitational waves.
This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.
The full Letter — with the strain time-series from both detectors, the time-frequency “chirp” spectrograms, the residuals against the general-relativity template, and the parameter-estimation tables — is available at the source below.
Detected 14 September 2015 · published 11 February 2016