THE end of the universe is about to get interesting. Most data favours a slow fade into a silent, frozen oblivion. But a new analysis suggests the cosmos could gradually tear itself apart, galaxy from galaxy and atom from atom. Or at least, we canāt rule it out.
We know that the universe mostly consists of dark matter, which only interacts with regular matter via gravity, and dark energy, a mysterious, unseen force thought to be accelerating the expansion of the universe.
Now, it seems the distribution of dark energy favours a gradual rip as the eventual fate of our universe, says at the University of Beira Interior in Portugal.
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Depending on how dark energy behaves, there are a number of possible end-time scenarios. In the most popular, it causes expansion to accelerate steadily over time, until galaxies, stars and atoms grow too distant and cold to interact ā a Big Freeze.
But if dark energy behaves differently so that the acceleration rate is not constant and increases with time, it will eventually tear everything to bits in a kind of rip.
For that to happen, dark energy would have to take a mysterious āphantomā form, which gets denser as the universe grows. That flies in the face of everything else we observe ā density normally decreases as volume expands.
āWe donāt know of anything that behaves this way,ā says at Princeton University in New Jersey. āBut that doesnāt mean it canāt happen.ā
Bouhmadi-LĆ³pez and graduate students Imanol Albarran and JoĆ£o Morais studied three versions of this tear: the Big Rip, the Little Sibling of the Big Rip and the Little Rip. The main difference is the way in which things come undone: in a Big Rip, the universe abruptly rips itself to shreds at a fixed point in the future, but in the littler versions, it happens more gradually. āWhat they have in common is that our galaxy, and all galaxies, would be ripped apart,ā Bouhmadi-LĆ³pez says. āEverything goes wrong.ā
The way matter clumps can tell us which rip the universe might head for. Dark matter and regular matter are more concentrated in some areas of the universe. Those clusters lead to variations in gravity, which can make time run differently in those areas. That could mean that in some regions of the cosmos, dark energy acts at a faster or slower rate.
Bouhmadi-LĆ³pez and colleagues studied these differences using observations from the Wilkinson Microwave Anisotropy Probe and the higher-resolution Planck satellite, which released its latest map of the cosmos in 2015.
They concluded that the most likely scenario is the Little Rip, in which the universeās expansion slows down just enough that we experience a gradual unzipping, rather than a cataclysmic tear ().
āTheyāve been able to come up with some observational signatures that are different in these models, and in the future we will be able to use that,ā says at Vanderbilt University in Tennessee, who developed the Little Rip theory.
āOur galaxy, and all galaxies, would be ripped apart. Everything goes wrongā
But College in New Hampshire, who came up with the Big Rip theory, is sceptical. āRight now, we canāt distinguish between these cases,ā he says. āI donāt think they are justified in making any conclusion about one model over another.ā
Thereās still plenty of time to figure it all out. A Little Rip wouldnāt take place for another 100 billion years.
This article appeared in print under the headline āUniverse headed for āLittle Rip'ā
Update [November 11]: A previous version of this article gave the wrong affiliation for Mariam Bouhmadi-Lopez.
