How can gravity be repulsive, when our everyday experience shows it’s attractive?
To explain it, we need dark energy.
What goes up must come down… right?
How do we think about something we can't see and don’t experience in our everyday lives, but seems to be pushing our universe apart ever faster?
The nature of dark energy is one of the most important unsolved problems in all of science.
But what, exactly, is dark energy, and why do we even believe that it exists?
Step back a minute and consider a more familiar experience: what happens when you toss a ball
straight up into the air?
It gradually slows down as gravity tugs on it, finally stopping in mid-air
and falling back to the ground. Of course, if you threw the ball hard enough (about 25,000 miles
per hour) it would actually escape from the Earth entirely and shoot into space, never to return.
But even in that case, gravity would continue to pull feebly on the ball, slowing its speed as it escaped the clutches of the Earth.
But now imagine something completely different.
Suppose that you tossed a ball into the air, and instead of being attracted back to the ground, the ball was repelled by the Earth and blasted faster and faster into the sky.
This would be an astonishing event, but it’s exactly what astronomers have observed happening to the
entire universe!
Scientists have known for almost a century that the universe is expanding, with all of the galaxies
flying apart from each other. And until recently, scientists believed that there were only two possible options for the universe in the future. It could expand forever (like the ball that you tossed upward at 25,000 miles an hour), but with the expansion slowing down as gravity
pulled all of the galaxies toward each other.
Or gravity might win out in the end and bring the expansion of the universe to a halt, finally collapsing it back down in a “big crunch,” just
like your ball plunging back to the ground.
This illustration shows abstracted ‘slices’ of space at different points in time as the universe expands.
So imagine scientists’ surprise when two different teams of astronomers discovered, back in 1998, that neither of these behaviors was
correct.
These astronomers were measuring how fast the universe was expanding when it was much younger than today.
But how could they do this without building a time machine?
Luckily, a telescope is a time machine.
When you look up at the stars at night, you aren’t seeing what they look like today – you’re seeing light
that left the stars a long time ago – often many hundreds of years.
By looking at distant supernovae, which are tremendously bright
exploding stars, astronomers can look back hundreds of millions of years. They can then measure the expansion rate back then by
comparing the distance to these far-off supernovae with the speed at which they are flying away from us.
And by comparing how fast the universe was expanding hundreds of millions of years ago to its rate of expansion today, these astronomers discovered that the expansion is
actually speeding up instead of slowing down as everyone had expected.
What pushes galaxies like these in the Hubble deep field apart?
Instead of pulling the galaxies in the universe together, gravity seems to be driving them apart.
But how can gravity be repulsive, when our everyday experience shows that it’s attractive?
Einstein’s theory of gravity in fact predicts that gravity can repel as well as attract, but only under very special circumstances.
Repulsive gravity requires a new form of energy, dubbed “dark energy,” with very weird properties.
Unlike ordinary matter, dark energy has negative pressure, and it’s this negative pressure that makes gravity repulsive. (For ordinary matter, gravity is always attractive).
Dark energy appears to be smoothly smeared out through the entire universe, and it interacts with ordinary matter only through the action of gravity, making it nearly impossible to test in the laboratory.
Scientists used to think that the expansion of the universe was described by the yellow,
green, or blue curves. But surprise, it’s actually the red curve instead.
The simplest form of dark energy goes by two different names: a cosmological constant or
vacuum energy. Vacuum energy has another strange property. Imagine a box that expands as the universe expands. The amount of matter in
the box stays the same as the box expands, but the volume of the box goes up, so the density of matter in the box goes down. In fact, the density of everything goes down as the universe expands.
Except for vacuum energy – its density stays exactly the same. (Yes, that’s as bizarre as it sounds. It’s like stretching a string of taffy
and discovering that it never gets any thinner).
Astronomers continue to probe the skies, looking for finer details that can build on what we suspect about dark energy.
Since dark energy can’t be isolated or probed in the laboratory, how can we hope to understand exactly what it’s made of?
Different theories for dark energy predict small differences in the way
that the expansion of the universe changes with time.
Credit: www.earthsky.org
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