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How The Universe Will End

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by Clara Moskowitz, written originally for SPACE.com

This vision is the most likely future for our universe, scientists say, because the best observations of the young, distant universe to date suggest that the strength of dark energy has remained steady throughout time.

This is in fitting with a theory that dark energy is what Einstein called the cosmological constant, a term he added to his general theory of relativity.

"Today, to the best of my knowledge, all the best data we have are consistent with a cosmological constant, consistent with dark energy being constant over time," Allen said. "If people had to bet on anything, they would bet on that."

Big Rip

But a Big Freeze isn't inevitable. If dark energy isn't a constant and instead increases over time, we could be facing what scientists call a Big Rip.

The current strength of dark energy is not thought to be enough to overcome gravity on small, local scales. However, if dark energy gets stronger, it may be enough to counteract even that, expanding not just the space between galaxies but the space within them.

"At some point galaxies themselves could be ripped apart," said Martin Bojowald, a physicist at Pennsylvania State University. "The Milky Way would be ripped apart. The question is whether it goes down even to the solar system."

Big Crunch

Another, equally dire possibility is that the strength of dark energy diminishes over time. In that case, the expansion of the universe will stop accelerating and eventually slow down.























If dark energy became weak enough, gravity might ultimately win the tug of war and pull the universe back in on itself. The result would be the Big Crunch.

"The collapse initially would just be very harmless; the density of the universe would increase, but very slowly," Bojowald said. "But at some time the collapse would lead to densities of the same size as the Big Bang."

According to general relativity, at the moment of the Big Bang the universe was as small as a single point, and infinitely dense. However, most physicists think this theory is incomplete and cannot fully describe the quantum and gravitational forces going on at that time.

Thus, if the universe did crunch back in on itself, it's unclear whether it would stop once it got down to its smallest, densest state, or if some kind of repellant force would kick in, forcing space back outward and beginning the cycle all over again.

Unraveling the mystery

If scientists have any hope of solving the mystery of the universe's fate, they must get a better handle on dark energy.

"Our biggest question is, what is the dark energy?" said astrophysicist Alexey Vikhlinin of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. "All these answers sensitively depend on the physical nature of dark energy."

It's a question researchers on which do have hope of making headway, as they continue to look farther and farther away, taking more and more precise measurements of the expansion rate of the universe over time. In the next decade or so, scientists expect to be able to say with significantly more confidence whether dark energy has been constant or has changed over the 14 billion years since the Big Bang.

It's a challenge scientists relish.

"The universe is kind of humbling when you look at it and start to appreciate its scale," Allen said. "It feels like a privilege to be able to ask these questions."











































































































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