Gravity of the Situation

Originally published in the Informanté newspaper on Thursday, 25 February, 2016.


A few weeks ago, scientists revealed an amazing discovery. 100 years after Albert Einstein had formulated his General Theory of Relativity, an experiment had confirmed the existence of one of the predictions of his theory – gravitational waves. Prof Karsten Danzmann, from the Max Planck Institute for Gravitational Physics and Leibniz University in Hannover, Germany said that "It is the first ever direct detection of gravitational waves; it's the first ever direct detection of black holes and it is a confirmation of General Relativity because the property of these black holes agrees exactly with what Einstein predicted almost exactly 100 years ago."

Of course, all this seems rather esoteric to the average man, whose only recollection of Einstein is his famous equation E = mc2 and his letter to Franklin Delano Roosevelt concerning the atomic bomb. Few know the implications of his work, and perhaps that is why the confirmation of his theories even a 100 years later don’t quite shake up the world as much as it should.

And while we may wonder what effect this could have on the average person, consider the following – in most cellphones these days, you have a GPS transceiver. This transceiver receives precise time signals for the up to 24 GPS satellites around earth, each with an atomic clock accurate to 1 nanosecond (1 billionth of a second). To determine your position, the transceiver compares the time signals from 4 different satellites, and trilaterates your position from the time difference in the satellite signals, and their known positions above the earth. 

These satellites are 20 000 km above the ground, orbiting the earth at 14 000 km/h. Special Relativity predicts that due to their speed, they’ll be slower than your clock by 7 microseconds per day. General Relativity predicts that because they’re further from a gravitational object, they’ll be faster than our clocks by 45 microseconds per day. For the navigational calculations to work, the clocks on all our devices should remain accurate within 30 nanoseconds. A microsecond is 1000 times longer than a nanosecond – if Einstein’s theories were not taken into account, the GPS system would be inaccurate in about 2 minutes, and off by 10km in a day. 

Because E = mc2 is only the start of the story. It is part of a solution to a paradox Einstein encountered in formulating his Special Theory of Relativity. Einstein’s Special Theory of Relativity was originally proposed to reconcile the Laws of Motion of Isaac Newton with electromagnetism as described by James Clerk Maxwell. 

Einstein started from the proposition the speed of light was constant regardless of the motion of the observer, and from that, a lot of what sounds counter-intuitive flowed. Einstein’s work on Special Relativity showed not only that mass and energy are equivalent (E = mc2), but also that space and time cannot be separated from one another – that time was a dimension just like any other. From this, a few other strange features emerged. 

Since the speed of light in a vacuum had to remain constant, something else happened when objects started travelling close to the speed of light. In order for light observed by such an object to remain at constant speed, time had to slow for such objects, since light could not. This is commonly known as time dilation. And in order for the speed of light to be constant, those observing an object travelling close to the speed of light would see its length shorten in the direction of travel. This is called a Lorentz contraction. 

But Einstein’s Special Theory of Relativity only explained motion in bodies without the effect of gravity, hence the term ‘special.’ Even so, up to today, it is still the most accurate model of motion tested. But ultimately, all bodies are under the influence of gravity. And thus Einstein worked for 8 more years, and in 1915, he published his General Theory of Relativity. 

This General Theory of Relativity combined the Special Theory of Relativity with Newton’s Law of Universal Gravitation, describing gravity as a property of the curvature of space and time, or spacetime. Einstein postulated that heavy objects curved spacetime in much the same way a heavy iron ball on a bed curves the surface of a bed. And in the same way a smaller ball would fall into the curve created by the heavy one, so too do all objects in space curve toward the heavier one. In fact, Einstein showed gravity bends even light. It predicts gravitational time dilation, to allow the speed of light to remain constant as it goes deeper into and then out of gravity (i.e. time passes slower the stronger gravity is), it predicts gravity can be used as a lens to focus light (gravitational lensing), it predicts gravity can be too strong for even light to escape (black holes), and then also predicts that when two spinning black holes collide, they’ll set off waves in spacetime similar to the effect that waves have on a puddle if you drop a stone in them.


This all sounds very counter intuitive, which is why Einstein’s theories have always been the subject of extensive testing. Thus, when on September 14, 2015 at 09:51 UTC, the Laser Interferometer Gravitational-wave Observatory (LIGO) detectors, located in Livingston, Louisiana, and Hanford, Washington, went off, the scientific community cheered. Einstein’s theories had their reliability to predict confirmed. 

As our technology advances, we become more and more dependent on them being built to model and anticipate the universe as it is, not as one wishes it would be. The confirmation of scientific theories not only provides us certainty about the universe we live in now, it also gives us hope that we can find answers in the future. After all, if simple theories on the progression of time was capable of providing us pinpoint navigation to the entire human race a mere few decades later, who knows where this one will take us?

No comments:

Post a Comment