Q.  Scientists made the landmark announcement about the discovery of gravitational waves. What are they and what relevance have they got.

What are gravitational waves?

Gravitational waves are small ripples in space-time that are believed to travel across the universe at the speed of light. They are like tiny waves on a lake — from far away, the lake’s surface looks glassy smooth; only up very close can the details of the surface be seen. They were predicted to exist by Albert Einstein in 1916 as a consequence of his General Theory of Relativity.

Scientists spot elusive space-time ripples

The highly elusive ‘gravitational waves’ have finally been detected. Understandably, and justifiably, there is great elation within the global physics community, astrophysicists and cosmologists in particular.  

What does Einstein say about gravity?

While Sir Isaac Newton visualised gravitational force as a pulling force between objects, Albert Einstein opined it to be a pushing force due to the curvature of four dimensional spacetime fabric. The curvature of spacetime stems from the dent heavy objects produce on spacetime fabric, which can be compared to the dent one could see on a plastic sheet when a massive ball is placed.

How are these waves detected?

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 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 U.S. government.

What is LIGO?

The Laser Interferometer Gravitational-Wave Observatory is a large-scale physics experiment aiming to directly detect gravitational waves.

LIGO operates two gravitational wave observatories in unison: the LIGO Livingston Observatory in Livingston, Louisiana, and the LIGO Hanford Observatory, on the DOE Hanford Site, located near Richland, Washington. These sites are separated by 3,002 kilometers. Since gravitational waves are expected to travel at the speed of light, this distance corresponds to a difference in gravitational wave arrival times of up to ten milliseconds.

Why is the study important?

Discovery of gravitational waves 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.

Did scientists ever detect gravitational waves?

Although, physics supports the existence of gravitational waves, the strength of such waves even due to astronomically heavy bodies is awfully weak to be detected.On March 17, 2014, Harvard-Smithsonian Centre for Astrophysics erroneously claimed discovery of gravitational waves. The Harvard group, working at BICEP2 (Background Imaging of Cosmic Extragalactic Polarisation) telescope, had reported that they had observed a twist in the polarisation of ancient light that goes back to the time of the big bang. But within a month, studies pointed out flaws in the study.

Gravitational Waves: What Their Discovery Means for Science and Humanity

With this new sensory view of the universe, here are some of the things scientists hope to discover.

New windows on the universe

LIGO is particularly sensitive to gravitational waves that come from violent cosmic events, such as two massive objects colliding or a star exploding. The observatory has the potential to locate these objects or events before light-based telescopes can do so, and in some cases, gravitational-wave observations could be the only way to find and study such events.

For example, in yesterday's announcement, scientists reported that LIGO had identified two black holes spinning around each other and merging together in a final, energetic collision. As their name suggests, black holes don't radiate light, which means they are invisible to telescopes that collect and study electromagnetic radiation. Some black holes are visible with light-based telescopes, because material in their immediate vicinity radiates, but scientists haven't seen examples of merging black holes with radiating material around them.

In addition, the black holes spotted by LIGO are 29 and 36 times the mass of the sun, respectively. But Reitze said that as LIGO's sensitivity continues to improve, the instrument could be sensitive to black holes that are 100, 200 or even 500 times the mass of the sun that are further away from Earth. "There could be a really nice discovery space that opens up once we get out there," he said.

Scientists already know that studying the sky in different wavelengths of light can reveal new data about the cosmos. For many centuries, astronomers could only work with optical light. But relatively recently, researchers built instruments allowing them to study the universe using X-rays, radio waves, ultraviolet waves and gamma-rays. Each time, scientists got a new view of the universe.

In the same way, gravitational waves have the potential to show scientists totally new features of cosmic objects, LIGO team members said. 

"If we're ever lucky enough to have a supernova in our own galaxy, or maybe in a nearby galaxy, we will be able to look at the actual dynamics of what goes on inside the supernova," said LIGO co-founder Rainer Weiss of MIT, who spoke at the announcement ceremony. While light is often blocked by dust and gas, "gravitational waves come right out [of the supernova], boldly unimpeded," Weiss said. "As a consequence, you really find out what's going on inside of these things."

Other exotic objects scientists hope to study with gravitational waves are neutron stars, which are mind-bogglingly dense, burned-out stellar corpses: A teaspoon of neutron-star material would weigh about a billion tons on Earth. Scientists aren't sure what happens to regular matter under such extreme conditions, but gravitational waves could provide extremely helpful clues, because these waves should carry information about the interior of the neutron star all the way to Earth, LIGO scientists said.

LIGO also has a system set up to alert light-based telescopes when the detector seems to have spotted a gravitational wave. Some of the astronomical events that LIGO will study, such as colliding neutron stars, may produce light in all wavelengths, from gamma-rays to radio waves. With LIGO's alert system in place, it's possible that scientists could observe some astronomical events or objects in various wavelengths of light, plus gravitational waves, which would provide a "very complete picture" of those events, Reitze said.

"When that happens, that'll be, I think, the next big thing in this field," he said. 


Gravitational waves were first predicted by Einstein's theory of general relativity, which was published in 1916. That famous theory has stood up to all kinds of physical tests, but there are some aspects that scientists haven't been able to study in the real world, because they require very extreme circumstances. The extreme warping of space-time is one example of this.

"Until now, we have only seen warped space-time when it is very calm — as though we had only seen the surface of the ocean on a very calm day, when it's quite glassy," Kip Thorne of Caltech, another founding member of LIGO and an expert on warped space-time, said at yesterday's ceremony. "We had never seen the ocean roiled in a storm, with crashing waves. All that changed on Sept. 14. The colliding black holes that produced these gravitational waves created a violent storm in the fabric of space and time." 

"This observation tests that regime beautifully, very strongly," Thorne continued. "And Einstein comes out with beaming success."

But the study of general relativity via gravitational waves is far from over. Questions remain about the nature of the graviton, the particle believed to carry the gravitational force (just like the photon is the particle that carries the electromagnetic force). And scientists have many questions about the inner workings of black holes, which gravitational waves may help illuminate (so to speak). But all of that, the scientists said, will be revealed slowly, over the course of many years, as LIGO and related instruments collect more data on more events.

A legacy for the future

Looking toward the next three years, Reitze said the collaboration is focused on increasing LIGO's sensitivity to its full potential. This will make the observatory — which consists of two big detectors, one in Louisiana and the other in Washington state — more sensitive to gravitational waves. But scientists don't know how many events LIGO will see, because they don't know how often many of these events occur in the universe.

LIGO detected the binary black hole merger even before the instrument began its first official observation campaign after its recent upgrade, but it's possible that this was a lucky break. To get the gravitational astronomy train rolling, LIGO simply needs more data.

When asked to comment on LIGO's impact on the world beyond the scientific community, and about how gravitational-wave science might influence people's daily lives, Reitze simply said, "Who knows?"

"When Einstein predicted general relativity, who would have predicted that we'd use it every day when we use our cellphones?" he said. (General relativity provides an understanding how gravity influences the passing of time, and this information is necessary for GPS technology, which uses satellites that orbit further away from the gravitational pull of the Earth than people on the surface).

LIGO is "the most sensitive instrument ever built," said Reitze, and the technological advances that have been made while building the observatory may feed into technologies that will be used in ways people can't yet predict.

Thorne said he sees the larger contribution of LIGO slightly differently.

"When we look back on the era of the Renaissance, and we ask ourselves, 'What did the humans of that era give to us that's important to us today?' I think we would all agree it's great art, great architecture, great music," he said.

"Similarly, when our descendants look back on this era, and they ask themselves, 'What great things came to us?' … I believe there will be an understanding of the fundamental laws of the universe and an understanding of what those laws do in the universe, and an exploration of the universe," Thorne added. "LIGO is a big part of that. The rest of astronomy is a big part of that. And I think that cultural gift to our future generations is really much bigger than any kind of technological spin-off, than the ultimate development of technology of any kind. I think we should be proud of what we give to our descendants culturally."




Dr Khan

Dr. Khan began his career of teaching in 1988 as lecturer in a college of University of Delhi. He later taught at Delhi School of Economics, University of Delhi. He has several research papers and books to his credit.

Dr. Khan has been teaching General Studies since February 1992 to IAS aspirants and is very proud of the fact that almost every State and Union Territory in India has some civil servants who personally associate with him.



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