Gravitational Waves

In 2017, the Nobel Prize for physics was awarded to Kip Thorne, Rainer Weiss and Barry Barish for their work towards the first-ever detection of gravitational waves by conceptualizing the Laser Interferometer Gravitational Wave-Observatory (LIGO) in the early 1970s. Gravitational waves are simply defined as invisible "ripples" in space that squeeze and stretch everything in their path at the speed of light, much like the ripples in a pond when a stone is tossed in. 

Einstein hypothesized this in his theory of general relativity, which, in simple terms, states that space and time are two aspects of space-time, which curves when there is gravity, matter, energy, and momentum. He predicted that two large bodies (Such as black holes or stars) orbiting or colliding into each other could cause gravitational waves in space-time. 

Two stars orbit each other, creating 'ripples' also known as gravitational waves
Both observatories work in unison and are highly sensitive. The detection of gravitational waves cannot be confirmed with only one observatory, as there are massive amounts of data being received from all over the universe at any given time. So, when both observatories receive the same specific signal, it can be verified that the signal is indeed a gravitational wave.

LIGO
So how do we detect them? This is where LIGO comes in. LIGO has the ability to detect gravitational waves from a whopping 1 BILLION cubic light-years of space, all the while receiving massive amounts of data. To be able to detect these gravitational waves, two observatories on opposite sides of the USA were made, with each observatory working in the following way: A laser beam is split down two 4-kilometer long arms containing a mirror at the end. The laser beams reflect back off of the mirrors and come back to converge at the base of the arms. Both beams cancel each other out, and no light is detected. The passage of a gravitational wave would alter the length of the arms by extremely small distances, causing the light beams to travel minutely different distances. This mismatch would be measurable with a light detector. 


Cool right!? If you're fascinated by this, I suggest you take the time to learn some more from these sites:


What do you think about gravitational waves? Please leave any feedback (or praise :) ) in the comments!

Email me at: bparth@tisb.ac.in



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