A century after Albert Einstein rewrote our understanding of space and time, physicists have confirmed one of the most elusive predictions of his general theory of relativity.
In another galaxy, a billion or so light-years away, two black holes
collided, shaking the fabric of spacetime. Here on Earth, two giant
detectors on opposite sides of the United States quivered as
gravitational waves washed over them. After decades trying to directly
detect the waves, the recently upgraded Laser Interferometer
Gravitational-Wave Observatory, now known as Advanced LIGO, appears to
have succeeded, ushering in a new era of astronomy.
What are gravitational waves?
Colossal
cosmic collisions and stellar explosions can rattle spacetime itself.
General relativity predicts that ripples in the fabric of spacetime
radiate energy away from such catastrophes. The ripples are subtle; by
the time they reach Earth, some compress spacetime by as little as one
ten-thousandth the width of a proton.
How are they detected?
To spot a signal, LIGO uses a special
mirror to split a beam of laser light and sends the beams down two
4-kilometer-long arms, at a 90 degree angle to each other. After
ricocheting back and forth 400 times, turning each beam’s journey into a
1,600 kilometer round-trip, the light recombines near its source.
The experiment is designed so that, in normal
conditions, the light waves cancel one another out when they recombine,
sending no light signal to the nearby detector.
But
a gravitational wave stretches one tube while squeezing the other,
altering the distance the two beams travel relative to each other.
Because of this difference in distance, the recombining waves are no
longer perfectly aligned and therefore don’t cancel out. The detector
picks up a faint glow, signaling a passing wave.
LIGO has
one detector in Louisiana and another in Washington to ensure the wave
is not a local phenomenon and to help locate its source.
What are other sources of gravitational waves?
By
studying computer simulations of astrophysical phenomena, scientists
can figure out what type of signals to expect from various gravitational
wave sources.