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CosmosUp | April 4, 2020

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Flat Universe Theory: What Does It Mean?

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Our universe have some peculiar properties, properties that couldn’t be explained by conventional Big Bang theory. For example, it’s flat, meaning it’s at just the right mass density that it will neither expand forever nor collapse back on itself. Why should it be flat? And completely opposite sides of the universe that haven’t had time to interact are at the same temperature. How can this possibly be?

These were two of the biggest questions in cosmology. It wasn’t until the 1980s, with the theory of cosmic inflation proposed by Alan Guth, that we found some answers. Inflation took us back to the beginning of the universe and, with exotic physics like repulsive gravity and false vacuums, answered the why and what of the Big Bang.

The first problem introduced by the old Big Bang theory was called the horizon problem.

Which is basically the problem of trying to understand how the universe got to be so uniform. Why does the universe look the same over there as it does if you look that way? And why was this a problem?

Guth said.

Well, think of a cup of tea. If you pour milk into your tea, it’ll take some time for the molecules to interact and eventually come to about the same temperature, but it won’t happen instantly. The same is true on a larger scale. The fastest any two objects can interact is as soon as light has had time to travel between them.

Well, according to conventional Big Bang theory, light hasn’t had time to travel from one side of the observable universe to the other, so why should they be at the same temperature?

Inflation gets around that in really a very simple way, is that if we trace back the universe that we’re looking at now to what it looked like before inflation, it was vastly smaller than anybody would have thought without the inflationary theory.

added Guth.

Vastly smaller is not an exaggeration. Before inflation, everything in our observable universe fit in a volume a billionth the size of a proton. Then the universe went through two expansions, inflation and after. Both expanded space by a factor of 1028, but the second expansion took 13.8 billion years. That first expansion, inflation, took 10 to the minus 38 seconds. It’s just an unfathomable rate.

Inflation theory infographic

Cosmic Inflation ©CosmosUp.com

And it was during the time before inflation, when the universe was incredibly tiny, that there was plenty of time for every piece of the universe to communicate with every other piece and plenty of time for it to come to essentially a uniform density of energy and uniform temperature.

explained Guth.

So now we know the universe was super tiny. Well, the true genius of Guth’s theory was not the incredibly tiny universe, but how it could have expanded so fast. Inflation provided the mechanism for expansion — repulsive gravity.

In Newton’s theory of gravity, gravity was always attractive. There just was no other option, but it turned out that the more complicated theory of general relativity actually allows for the possibility of a repulsive form of gravity.

added Guth.

Yes, in very specific circumstances, gravity can provide a push, not a pull. It comes from something called the false vacuum, a state of matter in the early universe that allows expansion of space while the mass density stays constant, and that understanding for the mechanism of inflation brought a solution to the horizon people.

The second obstacle The second problem was called the flatness problem. Why is the universe so flat, and what do I mean by flat? Well, the curvature of the universe is defined by the mass density of space, or the amount of energy and mass per volume. If there is a lot of matter, the universe is closed and collapses back in on itself.

 If there’s not much matter, the universe is open, and it will expand forever. If, however, the universe is in perfect balance and the density is exactly critical density, the universe will be flat, and it will continue to expand forever, but at an increasingly slower rate. So it will eventually stop, but when time reaches infinity.

The mass density we have measured so far appears to be exactly critical. Why is that? In fact, if it had started even slightly open or closed, it would have been pushed even further away from critical density over time by the expansion of the universe, just like the longer an arrow has to travel toward a target, the straighter you had to have initially shot the arrow. But we’re so close to hitting a bullseye. We’re so close to critical density. Why?

Inflation forces the universe toward critical density. How?

Well, in the conventional Big Bang theory, the universe gets larger, but as it gets larger, it gets much, much less dense. During inflation, the universe is getting larger and larger, and it’s flatter and flatter at a fixed mass density.

Guth explained.

General relativity implies a direct relationship between the mass density and the geometry of space or the flatness, so as space expands, the geometry gets flatter. Imagine space like the surface of a balloon. As you blow the balloon up, the surface gets flatter and flatter. Space does this in three dimensions.

And as space gets flatter, we go back to our relationship between geometry and mass density, and we find that the density is pushed toward critical density. In fact, it’s pushed very quickly toward critical density since the expansion of space during inflation is exponential, which explains why we’re so close to critical mass density.

And, boom, flatness problem solved. So you may be wondering, if inflation theory was so revolutionary and imaginative, why haven’t we heard more about it? Well, inflation is still a hot topic of debate. As we discussed, it solves many of the problems of conventional Big Bang theory and is widely accepted throughout the scientific community, but like all good theories, it has to make more predictions which we then observe.

We’re hoping for more observations that support inflationary theory, or whatever theory that might improve upon it. That’s what we’re working towards.

By: Dianna Cowern.



Comments


  1. Dennis torok

    Also I believe that the universe isn’t flat but rather more spiral like in shape much like our own galaxy due to the laws for the conservation of energy and angular monentum


  2. Dennis torok

    I believe that the universe goes through cycles. Everything in the universe will eventually end up in a black hole and black holes are nothing more than a group of quarks void of any electromagnetic energy. Any electromagnetic energy that does end up inside a black hole is readmitted as Hawking radiation or reject it in the form of gamma rays. Any and all electromagnetic energy that is ejected into the universe eventually slows down and pools in the voids in the cosmic web essentially inflating the universe because what we know to date is that the expansion of the universe is accelerating and we also know that more more black holes are being born everyday. but one thing you can’t get around in the universe is limits. everything has limits. There’s a limit as to how big a star can get, limits as to how big a planet can get in limits as to how far light can go we know this be due to redshift. Redshift is nothing more than a light wave slowing down and dissipating energy and sooner or later electromagnetic wavelength of light will lose enough energy that it will become trapped in a void of the cosmic web. So I believe that a black hole is nothing more then a group of quarks void of any electromagnetic energy. But sooner or later the quarks will be under so much stress that these fundamental particles will be ripped apart down to the rust form of energy an ejected throughout the cosmos. And anything that this energy comes into contact with will cause a chain reaction causing the same energy to be admitted. But once this chain reaction has come to completion this energy will then begin to slow and dissipate and once it has dissipated the electromagnetic energy will begin to pull back on the quarks and begin to call us back into hydrogen thus restarting universe.

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