It’s been almost two years since the first human brain was born.
And now the world’s scientists are looking into what might happen if we can harness the power of the singularity, a time when matter becomes so powerful that it destroys the fundamental laws of nature.
But if we’re lucky, there will be no singularity at all, because it’s impossible to predict the future.
That’s what a team of physicists and engineers from the University of Manchester and the University College London have been thinking about for decades.
They want to understand what happens when matter and energy collide at the edge of the universe, when we’re just a speck in the cosmic crowd, when the very fabric of reality becomes bent in ways that make no sense.
If the singularities don’t occur, how can we predict what happens?
It’s a question that has puzzled physicists since the universe began.
But the new work by scientists from the universities and universities in the UK and the US shows that we can do some pretty good work predicting the future of the cosmos, at least in some ways.
The scientists looked at the way the universe is currently behaving and at the possibility that matter and space can come to a physical end.
This means we have to go into the future and look at the conditions that existed before the singular events of the Big Bang, the Big Crunch and the Big Freeze.
What we know now We have a good idea about how the universe will look like in the coming two or three billion years, and we know that we are heading towards a new kind of singularity.
The Big Crunch A big bang occurred when the universe was about 8,000 years old.
It was a time of great energy and mass, when everything was made of matter.
There were no supernovas, no stars and no galaxies.
There was only the big bang.
The universe is now about 3.5 billion years old, and it’s already gone through several large bangs.
This is the most massive expansion of the Universe ever seen.
The energy involved was so great that it created a black hole, a kind of vacuum that sucked everything around it in.
But as it cooled down, it created new stars.
These are the first stars to form in the Universe.
They form stars with a mass of a million billion times that of the Sun, so they have about the same mass as our Sun.
These stars formed in a blackhole.
There are so many stars that they would have formed stars that would have been 10 billion times more massive than our Sun, and the mass of all these stars combined would have given the Universe its current radius of 2.8 billion kilometres.
The big bang itself happened in a supermassive black hole about 3 billion kilometres in diameter.
As the Universe cooled, this black hole cooled down to about 20 kilometres in mass.
The gravitational force between the Universe and the black hole created the current density of the material in the cosmos.
This density is called the singular density, and there is a huge amount of it.
This material is called a singularity and it will continue to exist even if there are no more black holes around.
What happens when the Universe collapses When the Universe is still in a state of collapse, the singular-density density drops by 50 per cent.
This drops to 20 per cent, so we have a drop in density of 100 per cent in just a matter of milliseconds.
In other words, the density drops so fast that it’s a lot like the light of the sun being scattered by the wind in the sky.
In a black box It takes a lot of energy to collapse a black-hole into a black state.
The Universe’s gravity has to do more work than the sun, but that doesn’t mean that there’s nothing there to collapse into.
As gravity falls away, it creates a pocket of matter called the cosmological constant.
The cosmology constant is the average density of matter in the universe that has ever existed.
When the universe collapsed into a singular state, it was compressed by the cosnological constant to just about one percent of the density of its universe.
This allowed the gravity of the black-body to push the cosmetically constant down by a factor of about 10, which is a lot more than the amount of energy that was being used to collapse the Universe into the singular state.
This meant that matter was moving from one location in space to another in space, so gravity was pushing the cosmic constant down in one direction.
What this means is that matter has accelerated to a very high rate of speed.
If matter was just a bit heavier, it would be pushed a lot slower.
That would explain why the Universe was expanding so fast.
However, when matter is more massive, it gets pushed even further.
When matter is denser, gravity gets pushed a little bit harder, so it’s pushed by the same amount.
This causes the cosmology constant to get compressed again, which leads to a decrease in the cosmere