The Nobel Prize in Physics - What are Gravitational Waves?

by kyle batra

The past couple weeks have been filled with news from Puerto Rico and Nevada so you might have missed the other important news of the week- the Nobel Prize. The Nobel Prize, named after Alfred Nobel who was famous for inventing dynamite, is a yearly award in many scientific categories and also peace and literature that honor the greatest achievements in those fields.

This year’s Nobel Prize in physics was awarded to three scientists, Kip Thorne, Rainer Weiss, and Barry Barish for their contributions in discovering gravitational waves, a concept that had been theorized by Einstein but never proven until very recently.

So what are these gravitational waves? Gravitational waves are very similar to other waves- light, radio waves, gamma rays… Yet they are a lot fainter and harder to detect (gravity is the weakest force compared to electromagnetic forces and the strong and weak nuclear force). Because of this, as Einstein theorized, we would only be able to detect massive gravitational ripples in spacetime, for example, when two black holes collide. Just a few weeks ago, just this occurred. Two black holes each about solar masses ended up merging far away in space, sending out huge ripples, gravitational waves, out in spacetime. We were able to detect these waves on earth, confirming that gravitational w

aves exist, which is a major discovery in physics and proves that Einstein was correct. This gives scientists a new way to observe the hardest observable object in the universe, black holes, and allows astronomers to look at other high mass objects like galaxies as stellar clusters as well.

In the photo above, one can see the large dip in spacetime that the supermassive black hole causes in spacetime. When multiple black hole’s collide, it causes the reverberations in spacetime which is what scientists look for and is what is known as gravitational waves.

How were the gravitational waves detected? Scientists constructed these two large-scale detectors named the LIGO interferometers which use a complicated set of angled mirrors to send two powerful lasers through miles of tubes. At the end, a detector is able to measure the exact wavelength of the laser, including where the bals and troughs are in the light wave. By looking at the variability between the two lasers, it can detect if a gravitational wave impacted the light waves. The tubes are very isolated so that nothing other than the gravitational waves could impact them. There has now been a third interferometer constructed in Italy, which was also able to confirm the previous detection of gravitational waves. By now having three detectors, astronomers can triangulate where in the sky the gravitational event is coming from. The final detector, named VIRGO, is smaller than the LIGO interferometers but is just as useful because of its ability to help triangulate the location of the event.