4 CASES WHEN THINGS TRAVEL FASTER THAN THE SPEED OF LIGHT
When Albert Einstein first foretold that light travels the same speed everywhere in our cosmos, he basically imprinted a speed limit on it: 670,616,629 miles per hour — fast enough to circle the complete Earth eight times every second.
This warping is what we colloquially call a “wormhole,” which theoretically would let something travel vast distances rapidly, fundamentally enabling us to break the cosmic speed limit by travelling unlimited distances in a very short amount of time.
But that’s not the complete story. Actually, it’s just the start.
Before Einstein, mass — the atoms that make up you, me, and everything we perceive — and energy were treated as separate objects. But in 1905, Einstein forever altered the way physicists view the cosmos. Einstein’s Special Theory of Relativity forever tied mass and energy together in the simple yet fundamental equation E=mc2. This little equation forecasts that nothing with mass can move as fast as light, or faster.
The closest humankind has ever come to reaching the speed of light is inside of powerful particle accelerators like the Large Hadron Collider and the Tevatron. These huge machines accelerate subatomic particles to more than 99.99% the speed of light, but as Physics Nobel laureate David Gross explains, these particles will never reach the cosmic speed limit. To do so would need an infinite amount of energy and, in the process, the object’s mass would become infinite, which is impossible. (The reason particles of light, called photons, travel at light speeds is since they have no mass.)
Since Einstein, physicists have discovered that certain entities can reach superluminal (that means “faster-than-light”) speeds and still follow the cosmic rules laid down by special relativity. While these do not contradict Einstein’s theory, they give us insight into the peculiar behavior of light and the quantum realm.
The light equivalent of a sonic boom
When objects travel faster than the speed of sound, they produce a sonic boom. So, in theory, if something travels quicker than the speed of light, it should yield something like a “luminal boom.”
In fact, this light boom occurs on a daily basis in facilities around the world — you can see it with your own eyes. It’s called Cherenkov radiation, and it shows up as a blue glow inside of nuclear reactors, like in the Advanced Test Reactor at the Idaho National Laboratory in the image to the right. Cherenkov radiation is named for Soviet researcher Pavel Alekseyevich Cherenkov, who first measured it in 1934 and was awarded the Nobel Physics Prize in 1958 for his discovery.
Cherenkov radiation glows as the core of the Advanced Test Reactor is submerged in water to keep it cool. In water, light travels at 75 % the speed it would in the vacuum of outer space, but the electrons produced by the reaction inside of the core travel through the water faster than the light does.
Particles, like these electrons, that exceed the speed of light in water, or some other medium such as glass, create a shock wave like to the shock wave from a sonic boom. When a rocket, for example, travels through air, it produces pressure waves in front that move away from it at the speed of sound, and the nearer the rocket reaches that sound barrier, the less time the waves have to move out of the object’s path. Once it extents to the speed of sound, the waves bunch up generating a shock front that forms a loud sonic boom.
Likewise, when electrons travel through water at speeds faster than light speed in water, they produce a shock wave of light that sometimes shines as blue light, but can also shine in ultraviolet. While these particles are roaming faster than light does in water, they’re not really breaking the cosmic speed limit of 670,616,629 miles per hour.
When the rules don’t apply
Cosmic web 3d map
Casey Stark (UC Berkeley) and Khee-Gan Lee (MPIA)
A 3D map of the cosmic web at a distance of 10.8 billion light years from Earth.
Keep in mind that Einstein’s Special Theory of Relativity states that nothing with mass can go faster than the speed of light, and as far as physicists can tell, the cosmos follow by that rule. But what about something without mass?
Photons, by their very nature, cannot surpass the speed of light, but particles of light are not the only massless entity in the cosmos. Empty space comprises of no material substance and consequently, by definition, has no mass.
Since nothing is just empty space or vacuum, it can enlarge faster than light speed since no material object is breaking the light barrier,” said theoretical astrophysicist Michio Kaku on Big Think. “Therefore, empty space can surely expand faster than light.”
This is precisely what physicists think occurred instantaneously after the Big Bang during the epoch called inflation, which was first hypothesized by physicists Alan Guth and Andrei Linde in the 1980s. Within a trillionth of a trillionth of a second, the cosmos constantly doubled in size and as a result, the outer edge of the cosmos expanded very quickly, much faster than the speed of light.
Quantum entanglement makes the cut
Quantum entanglement sounds complex and scary but at a rudimentary level entanglement is just the way subatomic particles communicate with each other.
If I have two electrons close together, they can vibrate in unison, according to the quantum theory,” Kaku explains on Big Think.
Now, isolate those two electrons so that they’re hundreds or even thousands of light years apart, and they will keep this instant communication bridge open.
- “If I jiggle one electron, the other electron ‘senses’ this vibration instantaneously, faster than the speed of light. Einstein believed that this therefore negated the quantum theory, since nothing can go faster than light,” Kaku wrote.
In fact, in 1935, Einstein, Boris Podolsky and Nathan Rosen, tried to disprove quantum theory with a thought experiment on what Einstein referred to as “spooky actions at a distance.”
Ironically, their paper laid the foundation for what today is called the EPR (Einstein-Podolsky-Rosen) paradox, a paradox that defines this immediate communication of quantum entanglement — an integral part of some of the world’s most cutting-edge technologies, like quantum cryptography.
Dreaming of wormholes
Wormhole in ‘Interstellar’ film
Since nothing with mass can travel faster than light, you can kiss interstellar travel goodbye — at least, in the classical sense of rocket ships and flying.
However, Einstein trampled over our aspirations of deep-space road trips with his Theory of Special Relativity, he gave us a new hope for intergalactic travel with his General Theory of Relativity in 1915. While Special Relativity wed mass and energy, General Relativity knitted space and time together.
The only viable way of breaking the light barrier may be through General Relativity and the warping of space time,” Kaku writes.
This warping is what we colloquially call a “wormhole,” which theoretically would let something travel vast distances rapidly, fundamentally enabling us to break the cosmic speed limit by travelling unlimited distances in a very short amount of time.
In 1988, theoretical physicist Kip Thorne — the science consultant and executive producer for the recent film “Interstellar” — used Einstein’s equations of General Relativity to forecast the likelihood of wormholes that would forever be open for space travel. But in order to be traversable, these wormholes need some strange, exotic matter holding them open.
“Now it is an amazing fact that exotic matter can exist, thanks to weirdnesses in the laws of quantum physics,” Thorne writes in his book “The Science of Interstellar.”
And this exotic matter has even been prepared in laboratories here on Earth, but in very tiny amounts. When Thorne proposed his theory of stable wormholes in 1988 he called upon the physics community to help him define if enough exotic matter could exist in the cosmos to support the likelihood of a wormhole.
This generated a lot of research by a lot of physicists; but today, nearly thirty years later, the answer is still unknown.” Thorne writes. At the moment, it’s not looking good, “But we are still far from a final answer,” he concludes.
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