Powered by

Map of all of universe's matter developed, could help understand its evolution better: Study

Sometimes to know what the matter is, you have to find it first

2171830161 Black hole sucking up the sun's matter in space | Shutterstock

A new analysis combined Dark Energy Survey and South Pole Telescope data to understand evolution of universe, according to a new study.

A group of scientists, including several with the University of Chicago, US, and Fermi National Accelerator Laboratory, US, have released one of the most precise measurements ever made of how matter is distributed across the universe today, according to the study.

Sometimes to know what the matter is, you have to find it first, said the study.

When the universe began, matter was flung outward and gradually formed the planets, stars and galaxies that we know and love today.

By carefully assembling a map of that matter today, scientists can try to understand the forces that shaped the evolution of the universe, the study said.

Combining data from two major telescope surveys of the universe, the Dark Energy Survey and the South Pole Telescope, the analysis involved more than 150 researchers and is published in the journal Physical Review D.

Among other findings, the analysis indicated that matter is not as "clumpy" as we would expect based on our current best model of the universe, which adds to a body of evidence that there may be something missing from our existing standard model of the universe.

After the Big Bang created all the matter in the universe in a very hot, intense few moments about 13 billion years ago, this matter has been spreading outward, cooling and clumping as it goes.

Scientists are very interested in tracing the path of this matter; by seeing where all the matter ended up, they can try to recreate what happened and what forces would have had to have been in play.

The first step is collecting enormous amounts of data with telescopes.

1697540665 Blue glowing deep space stream | Shutterstock

In this study, scientists combined data from two very different telescope surveys: The Dark Energy Survey, which surveyed the sky over six years from a mountaintop in Chile, and the South Pole Telescope, which looks for the faint traces of radiation that are still traveling across the sky from the first few moments of the universe.

Combining two different methods of looking at the sky reduces the chance that the results are thrown off by an error in one of the forms of measurement.

"It functions like a cross-check, so it becomes a much more robust measurement than if you just used one or the other," said University of Chicago astrophysicist Chihway Chang, one of the lead authors of the studies.

In both cases, the analysis looked at a phenomenon called gravitational lensing. As light travels across the universe, it can be slightly bent as it passes objects with lots of gravity, like galaxies.

This method catches both regular matter and dark matter - the mysterious form of matter that we have only detected due to its effects on regular matter - because both regular and dark matter exert gravity.

By rigorously analyzing these two sets of data, the scientists could infer where all the matter ended up in the universe. It is more precise than previous measurements - that is, it narrows down the possibilities for where this matter wound up - compared to previous analyses, the authors said.

The majority of the results fit perfectly with the currently accepted best theory of the universe, the study said.

But, according to the study, there are also signs of a crack - one that has been suggested in the past by other analyses, too.

"It seems like there are slightly less fluctuations in the current universe, than we would predict assuming our standard cosmological model anchored to the early universe," said analysis coauthor and University of Hawaii astrophysicist Eric Baxter.

That is, if you make a model incorporating all the currently accepted physical laws, then take the readings from the beginning of the universe and extrapolate it forward through time, the results look slightly different from what we actually measure around us today.

Specifically, today's readings find the universe is less "clumpy" - clustering in certain areas rather than evenly spread out - than the model would predict, the study said.

2115805886 Outer space cosmic landscape Nebula | Shutterstock

If other studies continue to find the same results, scientists say, it may mean there is something missing from our existing model of the universe, but the results are not yet to the statistical level that scientists consider to be ironclad. That will take further study, the study said.