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Showing posts with label Dark energy. Show all posts
Showing posts with label Dark energy. Show all posts

Can Gravity Beat Dark Energy?

Although it might not seem obvious when you look at the night sky, but we live in a universe that is expanding faster by the instant. Every day, stars fall over the horizon of what we can see, as the space between us stretches faster than their light can reach us. And we can never know what exists past that horizon. So you might imagine or you might have heard about, a far-off future, where space is stretching faster and faster and where all of the stars and galaxies are over that edge. A future where Earth will be left with a dark, empty sky. But luckily for us, or, at least, for hypothetical future earthlings, that’s not actually the case. Because the universe is expanding but not all of it.

We have known that the universe is expanding since the 1920s, but we only discovered that the expansion is accelerating in the 1990s, thanks to the Hubble Space Telescope. Hubble was the first tool to measure really precise distances to supernovas out near the edge of the observable universe. And it showed us that out there, ancient galaxies and the supernovas in them are zooming away from us faster than anywhere else. In fact, astronomers realized that they were flying away even faster than expected. Which, at first, didn’t make sense.


At the time, we thought the universe was dominated by gravity, which pulls things together. So seeing everything accelerate apart was weird. It would kind of be like if you kicked a ball uphill and saw it speed up instead of coming back down to you. Because of this, scientists concluded that there had to be something else going on, something pushing these galaxies apart. They came to call that thing dark energy. Decades later, dark energy is still really mysterious and there is a lot we don’t understand about it.

One explanation is that it’s a property of empty space. This means that space itself, with no stuff in it at all, has dark energy. And that energy pushes space apart, creating new space, which in turn has dark energy, which pushes space apart, creating new space, which in turn has dark energy, which You get it. If dark energy is a property of space, that also means you can’t dilute it. Its density will always be the same, no matter how much space expands.


Of course, that density is also pretty small. If you borrow Einstein’s “E=mc2” trick and express energy as mass, it is equivalent to about one grain of sand in a space the size of the entire Earth. But if you average that over the whole universe, which is mostly empty space, there is more dark energy than anything else. So it dominates and the universe as a whole expands. That’s why the most ancient galaxies are also moving away faster than before.

It has taken a long time for their light to reach us, so the universe has had more time to stretch. Now, this might all make dark energy seem super strong. After all, it makes up more than two-thirds of all the stuff in the universe and it’s pushing apart entire galaxies. But it is only powerful because there is a lot of it.


Within small spaces, especially those full of planets and stars, dark energy is actually pretty weak. Like, the gravity between the Sun and the Earth or the Earth and the Moon is more than enough to overpower the repulsive dark energy between them. In fact, most of the universe’s mass is concentrated in galaxy clusters and these pockets of matter are completely immune to dark energy. They are simply not expanding. 

It doesn’t mean the expansion is negligible, like how technically your gravity pulls ever-so-slightly on Earth but it is not enough to actually notice. It means that, as far as we know, dark energy is truly not stretching our galaxy at all. This is because it’s not a force like gravity, so it works a little differently.


To understand how, think about pushing on a heavy door. If you push lightly, it won’t open. Push a little harder and it still won’t. But if you push hard enough, once you cross a certain threshold of pushing, it will open. That door is gravity and within a galaxy, there’s just not enough dark energy to push it open. 

In other words, gravity is too strong. So our galaxy will never expand, because if it can’t stretch even a little, then it can’t create more space. And that means the amount of dark energy inside will never grow. Of course, this isn’t something we have been able to directly observe, like by looking at other galaxies. But multiple observations have shown us what dark energy is like and they all suggest this should be true.


Eventually, in the really distant future, fewer and fewer galaxies will be visible from Earth. And in 100 billion years or so deep space will be almost empty. But if Earth were still around by then, which, admittedly, is pretty unlikely, we would still have a beautiful night sky. Even as the universe stretches, the glow of our galaxy will still be overhead and we will have stars, constellations and even a handful of galaxies bound by gravity to ours. All because dark energy just can’t get a foothold around here. Of course, this will only last until the heat death of the universe but that’s another story.



The Big Rip Due To Dark Energy

Even though nobody else will be around to see it, scientists are fascinated by the end of the universe. It is kind of like the Big Bang there's just something so interesting about knowing where your atoms came from and where they are ultimately going to go in billions of years. Right now, there are a few ideas about how everything could end, where everything is spread so thin that activity basically stops.

Except, based on the results from a paper published in Nature Astronomy, that might not actually be true. Instead, there is a chance that everything in existence will eventually be ripped apart. And it would all be thanks to dark energy. Scientists think it makes up about 70% of the stuff in the universe and that it is the reason the expansion of the universe is accelerating. But there is a lot they are still figuring out.


Some of their research into dark energy has involved tools called standard candles. Standard candles are objects or events of known brightness that are used to measure distance in the far-off universe. Essentially, if you know how bright something should be up close, then how bright it actually looks indicates how far away it is.

For decades, the most important standard candle has been a special kind of exploding star called a type a supernova. These events always have the same brightness and in the 1990s, they allowed scientists to discover that the universe’s rate of expansion was accelerating. But what is really important for this recent study is that all the estimates provided by type 1a supernovas also indicate that the density of dark energy is fixed.



There is a lot of math involved, but this fact is a big reason they believe the Big Freeze is most likely. The problem is, you can only see so far with any given candle before it gets too dim and type 1a can’t take us back to the beginning of the universe. Because light can only move so fast, looking deep into space is like looking back in time. And these supernovas only allow us to see what things were like 4.5 billion years or so after the Big Bang.

Admittedly, there are some data sources like one called the Cosmic Microwave Background, that can tell us what things were like around 400 thousand years after the Big Bang. But that Background actually seems to disagree with what supernovas say about the expansion rate, which has had astronomers debating different options for years. There is also been a 4-billion-year gap between the two data sources, so it has been hard to figure out what’s going on.



That’s where last week’s news comes in. In their paper, a pair of astronomers proposed a new kind of standard candle, one that can let us peer back to that sweet spot just 1-2 billion years after the Big Bang. Their idea relies on quasars, rapidly-growing black holes that are among the universe’s brightest objects. Although quasars vary a lot in brightness, the authors claim that the ratio of ultraviolet brightness to X-ray brightness is not only more predictable but also reliable enough to indicate a quasar’s distance.

They point out that, at distances where both type 1a supernovas and quasars are visible, they provide comparable results, too. But the key is, farther from Earth, and further back in time, only quasars are visible. And after looking at some of those super-distant objects, the authors claim to have made a surprising observation: In the first couple billion years after the Big Bang, the growth rate of the universe didn’t match the predictions made by the supernova-based models. Back then, things seemed to be getting bigger more slowly than expected.



That implies that the amount of dark energy driving that expansion hasn’t been constant after all. Instead, it has been increasing over time. It sounds like a wild idea, but it would help explain why there isn’t a perfect match between the expansion rate we see from supernovas and that of Cosmic Microwave Background. So it is not like there is no foundation for it. But still, before they rewrite your Astronomy textbook, it is important to remember two things. One, these results will need a lot of confirmation before they are accepted into the mainstream theory. And two, scientists have effectively no clue what dark energy actually is.

So it is not even worth asking questions like what would be generating more and more of it, because we don’t even know what IT is. But if these results are true, there is one thing we do know, instead of ending in the Big Freeze, the universe would eventually end in the so-called Big Rip, where ever-increasing dark energy tears apart every particle until there’s nothing left and no one to see it. But the assumption is that it’s not such a big deal, because there is no way we would be around by then.

Reference:- Quasars as standard candles
Also Read:- Let's Understand Wormholes


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