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Spokane, Washington  Est. May 19, 1883

Einstein got it right: Gravitational waves exist in spacetime

A visual of gravitational waves from two converging black holes is displayed on a monitor behind Laser Interferometer Gravitational-Wave Observatory (LIGO) Co-Founder Kip Thorne during a news conference at the National Press Club in Washington, D.C., Thursday. (Andrew Harnik / Associated Press)
Nicholas K. Geranios Associated Press

More than a billion years ago, in a galaxy far away, two black holes surrendered to one another’s inexorable attraction and collided with such force that it disturbed the very fabric of the universe.

On Thursday, scientists announced to the world that they had detected the ripple-like gravitational waves that still course from this violent event and simultaneously confirmed a prediction made by Albert Einstein a century ago.

The detection, made with the Laser Interferometer Gravitational-Wave Observatory, known as LIGO, is the culmination of a decadeslong search for signs of this elusive phenomenon – and an achievement some said was on par with the discovery of the Higgs boson, which earned its theorists a Nobel Prize in 2013.

The discovery, described in a paper in Physical Review Letters, will open a new window onto the universe, said David Reitze, executive director of LIGO, which was designed and built by researchers at the California Institute of Technology and the Massachusetts Institute of Technology.

“This was truly, I think, a scientific moonshot,” Reitze said at a news briefing at the National Press Club in Washington. “I really believe that. And we did it. We landed on the moon.”

Since humans first gazed skyward, they have relied on light of all wavelengths to describe their universe. Visible light first revealed the starry heavens, while infrared allowed us to peer further back in time and see older, more distant stars. Radio waves revealed the afterglow of the universe’s violent birth, as X-rays showcased the supernova deaths of massive stars.

But now, researchers will be able to sense the universe in a whole new way: with their “ears.”

“We can hear gravitational waves. We can hear the universe,” Gabriela Gonzalez, LIGO’s spokeswoman at Louisiana State University, said at the briefing. “That’s one of the beautiful things about this: We are not only going to be seeing the universe, we are going to be listening to it.”

The telltale ripples were picked up just before 2:51 a.m. PDT on Sept. 14 by the twin LIGO detectors – one in Hanford, Washington, and the other in Livingston, Louisiana – a mere three days after the detectors had gone live following a five-year upgrade.

“Nature was kind,” said Mustafa Amin, a cosmologist at Rice University who was not involved in the work.

The twin detectors are shaped like Ls with legs of equal length, 2.5 miles long. At the L’s corner, a laser beam is split and sent into both legs, then reflected back to the corner once it reaches mirrors in each leg. If both arrive at the same time – which they should – they’ll cancel each other out.

However, if a gravitational wave passes through, it will squeeze one leg and stretch the other, causing the distance to change and thus creating slight differences in timing that push the light waves out of phase, and the lasers will reach the photo detector. The detector is able to pick up discrepancies between the two beams that are a ten-thousandth the width of a proton.

Gravitational waves, which Einstein predicted as part of his general theory of relativity, occur as objects accelerate or decelerate through space, much the way a boat moving on a lake sends ripples across the water’s surface. But they’re so tiny that until now it’s been nearly impossible to detect them, even those caused by something as large as a planet moving around the sun.

So to pick up this signal, scientists have to look for massive, violent events in the universe. This particular signal appears to have been caused by a collision that occurred about 1.3 billion years ago between two black holes, holding 29 and 36 solar masses.

During the smash-up, the two black holes combined into one, and turned about three suns’ worth of mass into gravitational waves. Although the event lasted only 20 milliseconds, the peak power output was about 50 times the output of all the stars in the visible universe, said Caltech physicist Kip Thorne, one of LIGO’s three founders along with Caltech colleague Ronald Drever and MIT’s Rainer Weiss.

“This is amazing. Spectacular,” said Marc Kamionkowski, an astrophysicist at Johns Hopkins University who was not involved in the work. “It’s a major, major triumph for experimental physics.”

In its previous incarnation, LIGO ran from 2002 until 2010 without making any detections. That the National Science Foundation-funded project was able to make a detection just days after starting up was thanks to a much-needed five-year upgrade.

Kamionkowski guessed that hundreds of new events will be found over the next few years, allowing scientists to perform a range of different types of studies, including population surveys of these phenomena.

The LIGO result is also the first observation of a black-hole merger, and it offers a preview of the other high-energy phenomena in the universe that gravitational wave astronomy might reveal to star-gazing scientists.

“There’s probably even events we haven’t dreamed of,” said Fiona Harrison, chair of Caltech’s division of physics, mathematics and astronomy. “This is just the beginning.”

LIGO can get better

At best, LIGO in its current state is at a third of its maximum sensitivity, Weiss said. “Over years, the noise level will be brought down, and LIGO will be three times better and see three times farther,” Weiss said.

Scientists all over the world are working on developing laser detectors like LIGO. Virgo, an interferometer like LIGO in Europe, is expected to be ready to join LIGO in measuring waves later this year, Gonzalez said.

Researchers in Japan are working on Kagra, another interferometer, and the LIGO laboratory is working to establish another LIGO detector in India, which should be operational in 2022, according to a National Science Foundation news release.

“It took a worldwide village to do this,” Gonzalez said. The more interferometers there are across the world measuring gravitational waves, the easier it will be to find the black holes or other astronomical disturbances in the universe, Gonzalez said. As of now, researchers have only a general idea where the black holes collided.

Despite the growing understanding of how warped spacetime behaves, Thorne said, scientists aren’t dabbling in the realm of science fiction yet. “I don’t think (LIGO) is going to bring us any closer to time travel,” Thorne said with a chuckle. “LIGO is heading in a different direction.”

Scientists have been working on detecting gravitational waves for 40 years, largely with the support of national science grants. Reitze thanked “U.S. taxpayers and Congress, who supported this research.”

“We’re seeing our universe through new eyes in an entirely new way,” said France Cordova, National Science Foundation director. “Einstein would’ve been beaming.”