New Light on Dark Energy

Jan 30, 2008
Large-scale structures
Snapshot from a computer simulation of the formation of large-scale structures in the Universe, showing a patch of 100 million light-years and the resulting coherent motions of galaxies flowing towards the highest mass concentration in the centre. The snapshot refers to an epoch about 10 billion years back in time. The colour scale represents the mass density, with the highest density regions painted in red and the lowest in black. The tiny yellow lines describe the intensity and direction of the galaxy´s velocities. Like compass needles, they map the infall pattern and measure the rate of growth of the central structure. This depends on the subtle balance between dark matter, dark energy and the expansion of the Universe. Astronomers can measure this effect using large survey of galaxies at different epochs in time, as shown by the new research. Credit: Klaus Dolag and the VVDS team.

Astronomers have used ESO’s Very Large Telescope to measure the distribution and motions of thousands of galaxies in the distant Universe. This opens fascinating perspectives to better understand what drives the acceleration of the cosmic expansion and sheds new light on the mysterious dark energy that is thought to permeate the Universe.

“Explaining why the expansion of the Universe is currently accelerating is certainly the most fascinating question in modern cosmology,” says Luigi Guzzo, lead author of a paper in this week’s issue of Nature, in which the new results are presented. “We have been able to show that large surveys that measure the positions and velocities of distant galaxies provide us with a new powerful way to solve this mystery.”

Ten years ago, astronomers made the stunning discovery that the Universe is expanding at a faster pace today than it did in the past.

“This implies that one of two very different possibilities must hold true,” explains Enzo Branchini, member of the team. “Either the Universe is filled with a mysterious dark energy which produces a repulsive force that fights the gravitational brake from all the matter present in the Universe, or, our current theory of gravitation is not correct and needs to be modified, for example by adding extra dimensions to space.”

Current observations of the expansion rate of the Universe cannot distinguish between these two options, but the international team of 51 scientists from 24 institutions found a way that could help in tackling this problem. The technique is based on a well-known phenomenon, namely the fact that the apparent motion of distant galaxies results from two effects: the global expansion of the Universe that pushes the galaxies away from each other and the gravitational attraction of matter present in the galaxies’ neighbourhood that pulls them together, creating the cosmic web of large-scale structures.

“By measuring the apparent velocities of large samples of galaxies over the last thirty years, astronomers have been able to reconstruct a three-dimensional map of the distribution of galaxies over large volumes of the Universe. This map revealed large-scale structures such as clusters of galaxies and filamentary superclusters ”, says Olivier Le Fèvre, member of the team. “But the measured velocities also contain information about the local motions of galaxies; these introduce small but significant distortions in the reconstructed maps of the Universe. We have shown that measuring this distortion at different epochs of the Universe’s history is a way to test the nature of dark energy.”

Guzzo and his collaborators have been able to measure this effect by using the VIMOS spectrograph on Melipal, one of the four 8.2-m telescopes that is part of ESO’s VLT. As part of the VIMOS-VLT Deep Survey (VVDS), of which Le Fèvre is the Principal Investigator, spectra of several thousands of galaxies in a 4-square-degree field (or 20 times the size of the full Moon) at epochs corresponding to about half the current age of the Universe (about 7 billion years ago) were obtained and analysed.

“This is the largest field ever covered homogeneously by means of spectroscopy to this depth,” says Le Fèvre. “We have now collected more than 13,000 spectra in this field and the total volume sampled by the survey is more than 25 million cubic light-years.”

The astronomers compared their result with that of the 2dFGRS survey that probed the local Universe, i.e. measures the distortion at the present time.

Within current uncertainties, the measurement of this effect provides an independent indication of the need for an unknown extra energy ingredient in the ‘cosmic soup’, supporting the simplest form of dark energy, the so-called cosmological constant, introduced originally by Albert Einstein. The large uncertainties do not yet exclude the other scenarios, though.

“We have also shown that by extending our measurements over volumes about ten times larger than the VVDS, this technique should be able to tell us whether cosmic acceleration originates from a dark energy component of exotic origin or requires a modification of the laws of gravity,” said Guzzo.

“VIMOS on the VLT would certainly be a wonderful tool to perform this future survey and help us answer this fundamental question. This strongly encourages our team to proceed with even more ambitious surveys of the distant Universe,” says Le Fèvre.

Source: ESO

Explore further: Physicist's Nobel Prize up for auction; $325,000 minimum bid (Update)

Related Stories

Supernova ignition surprises scientists

May 20, 2015

Scientists have captured the early death throes of supernovae for the first time and found that the universe's benchmark explosions are much more varied than expected.

Fresh theories about dark matter

May 15, 2015

Tom Broadhurst, the Ikerbasque researcher in the Department of Theoretical Physics of the UPV/EHU, together with Sandor Molnar of the National Taiwan University and visiting Ikerbasque researcher at the UPV/EHU ...

Scientists discover the fluffiest galaxies

May 14, 2015

An international team of researchers led by Pieter van Dokkum at Yale University have used the W. M. Keck Observatory to confirm the existence of the most diffuse class of galaxies known in the universe. ...

VLT discovers new kind of globular star cluster

May 13, 2015

Observations with ESO's Very Large Telescope in Chile have discovered a new class of 'dark' globular star clusters around the giant galaxy Centaurus A. These mysterious objects look similar to normal clusters, ...

Recommended for you

On-demand X-rays at synchrotron light sources

15 hours ago

Consumers are now in the era of "on-demand" entertainment, in which they have access to the books, music and movies they want thanks to the internet. Likewise, scientists who use synchrotron light sources ...

New model sheds light on 'flocking' behaviour

23 hours ago

Understanding how turbulence can alter the shape and course of a flock of birds, a swarm of insects or even an algal bloom could help us to better predict their impact on the environment.

User comments : 5

Adjust slider to filter visible comments by rank

Display comments: newest first

earls
1 / 5 (2) Jan 30, 2008
"Either the Universe is filled with a mysterious dark energy which produces a repulsive force that fights the gravitational brake from all the matter present in the Universe, or, our current theory of gravitation is not correct and needs to be modified"

Hmmmmm... Hmm.... Coin toss?
Noumenon
3 / 5 (2) Jan 30, 2008
So, locally, galaxies spin and behave as if there is more gravitational force than what is accounted for visually,... and yet considered in relation to other galaxies and clusters on a larger scale, they accelerate as if there is less gravitational force with time than what is accounted for? Poor cosmologist. :)
out7x
1 / 5 (1) Jan 31, 2008
This is very important work. Turning 2D into a 3D universe. Onward!! I have little faith in dark energy. Go 10D superstrings!
LearmSceince
not rated yet Feb 11, 2008
Hmmmmm... Hmm.... Coin toss?


No. Design experiments that would distinguish between the candidates.
marlowg
not rated yet Mar 01, 2008
If matter contains an energy component with a wavelength equal to the size of the universe, it would explain why gravity started out stronger in the beginning and got weaker with time. If you do the math for 14 BLY, you will also see that this wavelength's relative energy compared to the rest energy of an electron is on the order of gravity's relative strength compared to the strength of the electric force.

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.