We Discovered That Life May Be Billions of Times More Common in the Multiverse

Why is there life in our universe? The existence of galaxies, stars, planets, and ultimately life seem to depend on a small number of finely tuned fundamental physical constants. Had the laws of physics been different, we would not have been around to debate the question. So how come the laws of our universe just happen to be the way they are—is it all a lucky coincidence?

In the last few decades, an increasingly popular theory has come to the fore. The multiverse theory suggests that our universe is just one of many in an infinite multiverse where new universes are constantly being born. It seems likely that baby universes are produced with a wide range of physical laws and fundamental constants, but that only a tiny fraction of these are hospitable for life. It would therefore make sense that there is a universe with the strange fundamental constants we see, finely tuned to be hospitable for life.

But now our new discovery, published in the Monthly Notices of the Royal Astronomical Society, complicates things by suggesting that life may actually be a lot more common in parallel universes than we had thought.

While there is no physical evidence that parallel universes exist (at the moment), the theories that explain how our universe came to be seem to suggest that they are inevitable. Our universe started with a Big Bang, followed by a period of very rapid expansion, known as inflation. However, according to modern physics, inflation is unlikely to have been a single event. Instead, many different patches of the cosmos could suddenly start inflating and expand to huge volumes—each bubble creating a universe in its own right.

Some believe that we may one day be able to witness imprints of collisions with parallel universes in the cosmic microwave background, which is the radiation left over from the birth of the universe. Others, however, believe the multiverse is a mathematical quirk rather than a reality.

Dark Energy

One hugely important constant in the universe is a mysterious, unknown force dubbed dark energy. At the present day, this makes up 70% of our universe. Rather than our universe slowing down as it expands, dark energy causes its expansion to accelerate.

But many current theories suggest that dark energy should be much more plentiful than this across the multiverse. Most universes should have an abundance of dark energy that is around a million, billion, billion, billion, billion, billion, billion times larger than in our universe. But if dark energy were this abundant, the universe would rip itself apart before gravity could bring together matter to form galaxies, stars, planets or people.

While our universe has a strangely low value of dark energy, it is this low value that makes our universe hospitable to life. The multiverse theory can help us explain why it is so low—there will always be some universes with unlikely values in an infinite multiverse.

However, the theory nevertheless requires that our universe’s value for the abundance of dark energy is close to the maximum allowed for intelligent life to exist. This is because larger values of dark energy should be more common in the multiverse than lower values. At the same time, we expect life to exist only in a small group of universes with a value below a certain maximum—those in which matter can still clump together to form stars and galaxies. This means that universes with a comparatively high value of dark energy (close to maximum) that are hospitable to life should be more numerous than universes with low values (close to minimum), meaning they are more likely.

So do we live in such a universe? Through our study, we set out to find out what this maximum level is and whether we are close to it.

Computer Simulations

Our computer model of the universe, the EAGLE project, has been successful at explaining the observed properties of galaxies in our universe. The simulations take the laws of physics and follow the formation of stars and galaxies as the universe expands after the Big Bang. The galaxies that emerge in our model look remarkably like those seen in the night sky through telescopes.

Each simulation led to a universe with specific structure.

This success makes it possible to convincingly investigate how the formation of stars and galaxies would proceed in other parts of the multiverse. We created a series of computer-generated universes that were identical apart from having different amounts of dark energy. Initially, the universes all expanded at similar rates but, as the energy left over from the Big Bang dissipated, the power of dark energy became important. The universes with abundant dark energy accelerated vigorously.

To our surprise, however, we discovered that baby universes with ten or even 100 times more abundant dark energy (compared to our own) produce almost as many stars and planets as our own universe. That means our own universe does not have a value of dark energy that is close to the maximum for life to exist. The effects of gravity are much more robust than we had previously thought. Life, it seems, would be rather common throughout the multiverse, perhaps a million, billion, billion, billion, billion more common that we previously thought.

Our discovery puts the idea that an infinite multiverse can explain the low abundance of dark energy on very rocky ground. Interestingly, in his last published paper, Stephen Hawking argued that the multiverse is far from infinite, and that it is more likely to contain a finite number of rather similar parallel universes.

We are forced to an uncomfortable conclusion. The value of dark energy we observe is far too unlikely for the multiverse to explain why we are here. It seems that a new physical law, or a new approach to understanding dark energy, is needed to account for the deeply puzzling properties of our universe. But the good news is that we are one step closer to cracking it.

This article was originally published on The Conversation. Read the original article.

Image Credit: Jaime Salcido/EAGLE Collaboration/Durham University

Richard Bower
Richard Bowerhttps://www.dur.ac.uk/physics/staff/profiles/?id=527
A long time ago, Richard Bower grew up in a small Cornish village where the sky was dark, and it was warm enough to sit outside and wonder where they came from. Today, he is Professor of Cosmology at Durham University. He works at the ICC, the Institute for Computational Cosmology, creating a virtual universe with some of the world’s largest computers. This is clearly an almost impossible task, yet recently his simulations have taken a major step forward and are able to reproduce galaxies in the observed universe in remarkable detail. Professor Bower’s interests span observational and theoretical studies of galaxy formation. His research time is shared between observational and theoretical cosmology. In particular, he works on the formation and evolution of galaxies and clusters of galaxies. He is fascinated by the existence of galaxies and the ways in which they formed. Why is the night sky so full of stars? What has made the different types of galaxies so different from each other? He likes to speculate about what it would be like to live in a galaxy cluster. After graduating with a First in Physics at Oxford, he completed his PhD thesis at the University of Durham and went on hold research positions in Munich and Edinburgh before returning to Durham as a lecturer. As well as teaching courses on Cosmology and Computing, he has lectured on topics as diverse as the Physics of Motorsport and, now, on Robert Grosseteste’s 13th century vision of the creation of the Universe, “De Luce”. Professor Bower leads the Intel Parallel Computing Centre at Durham, developing SWIFT, a revolutionary new approach to high-performance computing.
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