In our Universe today, the light arriving from a distant galaxy is shifted into the red because the Universe is expanding. The expansion rate was greater in the past, and for this, more distant objects appear to be receding even more quickly than a naive extrapolation of the expansion rate would indicate: this is because our Universe doesn’t simply contain matter and radiation, but dark energy as well.
The way the expansion rate changes over time is determined by what your Universe is made up of. For the first few thousand years after the Big Bang, radiation dominated.
For billions of years after that, matter dominated. And today, it’s dark energy. But before the Big Bang, space expanded at an exponential, enormous rate, which stretched the Universe flat and gave it uniform properties everywhere. This was during the period of cosmic inflation.
Exponential expansion means that rather than having the expansion rate slow as time goes on, at having distant points recede from one another at ever slower speeds, the expansion rate doesn’t drop at all. As a result, distant locations — as time goes on incrementally — get twice as far away, then four times, eight, sixteen, thirty-two, etc.
Because the expansion is not just exponential but also incredibly rapid, “doubling” happens on timescale of around 10-35 seconds. Meaning, by time 10-34 seconds have passed, the Universe is around 1000 times its initial size; by time 10-33 seconds have passed, the Universe is around 1030 (or 100010) times its initial size; by time 10-32 seconds have passed, the Universe is around 10300 times its initial size, and so on. Exponential isn’t so powerful because it’s fast; it’s so powerful because it’s relentless.
![This diagram shows, to scale, how spacetime evolves/expands in equal time increments if your… [+]
Universe is dominated by matter, radiation, or the energy inherent to space itself, with the latter corresponding to cosmic inflation. Inflation causes space to expand exponentially, which can very quickly result in any pre-existing curved or non-smooth space appearing indistinguishable from flat, and drives any two non-coincident particles apart extraordinarily rapidly.]
If two particles are created very close to one another during this inflationary state, they still have to obey the laws of special relativity: they can only move relative to one another at speeds less than (or equal to, if they’re massless) the speed of light. But the space between them is free to expand at whatever rate the Universe dictates.
If that means you’d extrapolate their relative speed to be greater than the speed of light by combining the effects of relative motion (special relativity) with expanding space (general relativity), there’s nothing forbidding that. You’d simply be mistaken for attributing the entirety of the apparent cosmic motion to special relativity. And you don’t even need to go to an inflationary state to run into that problem.
In a region just 1/32,000,000th of the sky, we’ve found 5,500 identifiable galaxies, all owing to the Hubble Space Telescope. Hundreds of the most distant ones seen here are already unreachable, even at the speed of light, due to the relentless expansion of space.]
If you take a look at the galaxies in our Universe today, the ones that lie beyond about 15 billion light years already appear to be receding from us faster than the speed of light. If you got into a spaceship today and took off towards them at the speed of light, you’d never reach them.
The expansion of the Universe teaches us that the rate that the fabric of space is stretching is greater than the distance we can cover even at light speed; the distance between us and them increases by more than a light year with each year that goes by. Beyond a critical distance in the Universe, all the galaxies that reside there are already forever out of reach.
There is no theoretical bound on the expansion rate because it itself isn’t a speed, but rather a property of the Universe that’s determined by the amount of energy in it. Today, that rate is around 70 km/s/Mpc, but during inflation, it was likely some 1050 times higher.
Within the observable Universe (yellow circle), there are approximately 2 trillion galaxies… [+]
WIKIMEDIA COMMONS USERS AZCOLVIN 429 AND FRÉDÉRIC MICHEL / E. SIEGEL
In an inflationary Universe, any two particles, beyond a tiny fraction of a second, will see the other one recede from them at speeds appearing to be faster-than-light. But the reason for this isn’t because the particles themselves are moving, but rather because the space between them is expanding.
Once the particles are no longer at the same location in both space and time, they can start to experience the general relativistic effects of an expanding Universe, which — during inflation — quickly dominates the special relativistic effects of their individual motions.
It’s only when we forget about general relativity and the expansion of space, and instead attribute the entirety of a distant particle’s motion to special relativity, that we trick ourselves into believing it travels faster-than-light. The Universe itself, however, is not static. Realizing that is easy. Understanding how that works is the hard part.