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RACHEL MARTIN, HOST:
Albert Einstein predicted that some cosmic smashups would be so powerful, they'd create ripples1 in the very fabric2 of the universe. A century later, physicists4 proved him right when they detected the ripples created by the collision of two black holes. The massive detectors6 used to make that discovery have now gotten an upgrade, and they are just about to start back up. NPR's Nell Greenfieldboyce reports.
NELL GREENFIELDBOYCE, BYLINE7: Gabby Gonzalez is a physicist3 at Louisiana State University who has spent years, decades, working with a team that was trying to detect something that had never been detected before.
GABRIELA GONZALEZ: I have lots of friends that, now, they tell me, I felt so worried about your career because you were working on such a difficult thing that I thought it was never going to happen. And now, I'm so jealous (laughter).
GREENFIELDBOYCE: They're jealous because in 2015, it did happen - the first-ever detection of gravitational waves. You can't see them. You can't feel them. But Albert Einstein had it right. Space and time is a kind of jiggly matrix. And when two big things out in the universe collide, they can send shockwaves through spacetime that are like the ripples you make when you toss a pebble8 into a pond. Being able to sense these waves is brand new for astronomy, which has spent centuries studying light.
GONZALEZ: Galileo invented the telescope or used the telescope for the first time to do astronomy 400 years ago. And today, we're still building better telescopes. I think this decade has been the beginning of gravitational wave astronomy.
GREENFIELDBOYCE: And she thinks it should just keep getting better and better. The United States has two facilities for detecting gravitational waves - one in Washington state and one in Louisiana. Together, they're called LIGO for the Laser Interferometer Gravitational-Wave Observatory9. I drove about an hour and a half north of New Orleans to see the one in rural Louisiana. The head of the observatory, Joe Giaime, took me over to a display case to see a gold medal.
JOSEPH GIAIME: People who win Nobel prizes can pay a little extra money, and check a box and get a duplicate.
GREENFIELDBOYCE: Each site has one of these since the first detection of gravitational waves was such a big deal that the Nobel Committee, pretty much instantly, honored three American physicists for their work on this project. We walk out onto a bridge that goes over a big concrete pipe. From here, we see the pipe going off into the distance, and we can also see another pipe as well. Giaime says each is more than two miles long. They come together in a shape that, from above, looks like a capital L.
GIAIME: I've spoken with pilots who fly over this. And they wonder why there's a pipeline10 that starts nowhere, travels, you know, a couple miles, turns right and then goes also nowhere.
GREENFIELDBOYCE: Inside each stretch of pipe is a powerful laser beam that bounces back and forth11 between mirrors. Scientists use this laser to precisely12 measure the length of each arm of the L. When a gravitational wave passes through and distorts space, the lengths change by a tiny, tiny bit like a fraction of the width of a subatomic particle.
GIAIME: We're in the control room now, and this is where all of the activities of both the site and the detector5 are monitored and controlled.
GREENFIELDBOYCE: It's a windowless room with people sitting at dozens of computer monitors. Since the first historic detection 3 1/2 years ago, this place has registered 10 more gravitational wave events. Nine were black hole collisions, and one was a pair of neutron13 stars smashing together. But the science has been shut down for more than a year. That was to let researchers install new hardware and other upgrades. The workers in here, now, are testing them out. On April 1, everything officially comes back online. Giaime says the U.S. detectors plus another one in Italy will all be more sensitive.
GIAIME: So, so far, we've seen 11 things. Maybe we'll see twice that many this year.
GREENFIELDBOYCE: And they'll be better able to locate the source of the waves in the sky. The team will send out public alerts so that anyone can point their telescopes at the right spot. In case, like the neutron star collision, the event sends out cosmic fireworks. Thousands of astronomers14 and physicists around the world are now involved in studying gravitational waves because these offer the only way to explore some of the most powerful, exotic events in the universe. And that's the fun of it. Nergis Mavalvala is a physicist at MIT.
NERGIS MAVALVALA: We've only seen this handful of black holes of all the possible ones that are out there. There are many, many questions we still don't know how to answer.
GREENFIELDBOYCE: Plus, maybe something completely unexpected will go boom.
MAVALVALA: That's how discovery happens. As you turn on a new instrument, you point it out at the sky and you see something that you had no idea existed.
GREENFIELDBOYCE: She says that's happened time and time again in astronomy, and she bets it'll happen for gravitational waves as well. Nell Greenfieldboyce, NPR News.
1 ripples | |
逐渐扩散的感觉( ripple的名词复数 ) | |
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2 fabric | |
n.织物,织品,布;构造,结构,组织 | |
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3 physicist | |
n.物理学家,研究物理学的人 | |
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4 physicists | |
物理学家( physicist的名词复数 ) | |
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5 detector | |
n.发觉者,探测器 | |
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6 detectors | |
探测器( detector的名词复数 ) | |
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7 byline | |
n.署名;v.署名 | |
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8 pebble | |
n.卵石,小圆石 | |
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9 observatory | |
n.天文台,气象台,瞭望台,观测台 | |
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10 pipeline | |
n.管道,管线 | |
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11 forth | |
adv.向前;向外,往外 | |
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12 precisely | |
adv.恰好,正好,精确地,细致地 | |
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13 neutron | |
n.中子 | |
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14 astronomers | |
n.天文学者,天文学家( astronomer的名词复数 ) | |
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