A century ago, Albert Einstein hypothesised the existence of gravitational waves, small ripples in space and time that dash across the universe at the speed of light.
But scientists have been able to find only indirect evidence of their existence. On Thursday, at a news conference called by the US National Science Foundation, researchers may announce at long last direct observations of the elusive waves.
Such a discovery would represent a scientific landmark, opening the door to an entirely new way to observe the cosmos and unlock secrets about the early universe and mysterious objects like black holes and neutron stars.
Scientists from the California Institute of Technology, the Massachusetts Institute of Technology and the LIGO Scientific Collaboration are set to make what they bill as a “status report” on Thursday on the quest to detect gravitational waves. It is widely expected they will announce they have achieved their goal.
“Let’s say this: The first discovery of gravitational waves is a Nobel Prize-winning venture,” said physicist Bruce Allen of the Max Planck Institute for Gravitational Physics in Hannover, Germany.
Einstein in 1916 proposed the existence of these waves as an outgrowth of his ground-breaking general theory of relativity.
“Gravitational waves are literally ripples in the curvature of space-time that are caused by collisions of heavy and compact objects like black holes and neutron stars,” Ashtekar said.
‘MOVING MASSES’
“They’re waves, like light or any other kind of electromagnetic radiation, except here what’s ‘waving’ is space and time itself,” said NASA astrophysicist Ira Thorpe, with the Goddard Space Flight Center in Maryland. “You get radiation, basically light, when you move some sort of charged particle. When you’re moving masses, you get gravitational waves.”
Scientists have been trying to detect them using two large laser instruments in the United States, known together as the Laser Interferometer Gravitational-Wave Observatory (LIGO), as well as another in Italy.
The twin LIGO installations are located roughly 1,800 miles (3,000 km) apart in Livingston, Louisiana, and Hanford, Washington. Having two detectors is a way to sift out terrestrial rumblings, such as traffic and earthquakes, from the faint ripples of space itself.
The LIGO work is funded by the National Science Foundation, an independent agency of the US government.
All the current knowledge about the universe comes from electromagnetic waves like radio waves, visible light, infrared light, X-rays and gamma rays. But a lot of information remains hidden because such waves get scattered as they traverse the cosmos. That would not be the case with gravitational waves, making them an enticing potential source of new information.
Two types of very massive and dense celestial objects, neutron stars and black holes, have proven tough to study but could offer ideal subjects if observations of gravitational waves are possible.
“People don’t really know what’s going on inside neutron stars,” Allen said of these objects that weigh about 50 percent more than the sun but are extremely compact, only about the size of a city.
“It gives us a detailed picture of what’s happening inside or around the object that’s producing the waves. So, for example, if two black holes orbit each other, we can’t see it any way other than gravitational waves because black holes don’t emit any light, radio waves, X-rays or anything. The only way to see that is through their gravitational waves,” Allen said.
Gravitational waves also offer a way to study what the universe was like in its infancy. For the first roughly 200,000 years of its existence, light did not travel freely through the universe, Allen said, but “gravitational waves can travel freely, back to very early times.”
“So one cool thing is one day we’ll be able to see what the universe looked like in very early times using gravitational waves. That’s what actually got me interested in the field 25 years ago,” Allen said.
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