CTIO / NOIRLab / DOE / NSF / AURA
The astronomers behind the Darkish Power Survey have measured the properties of the mysteriously repulsive darkish vitality extra exactly than ever earlier than. Their work brings collectively six years of information, greater than half a billion galaxies, and 1000’s of supernovae to make clear essential questions in cosmology.
Since 1998, astronomers have identified that the enlargement of the universe is accelerating. They aren’t certain why, but it surely’s normally put right down to the existence of a repulsive property of empty area, labeled darkish vitality. However the nature of darkish vitality — whether or not it evolves over time or expands area in a extra fixed trend — has remained an open query.
Again in 2013, astronomers began utilizing the Darkish Power Digital camera hooked up to the Víctor M. Blanco telescope in Chile to start the Darkish Power Survey (DES) to attempt to reply that query. Over the following six years, DES astronomers noticed an eighth of the sky throughout a complete of 758 nights, cataloguing 669 million galaxies. The total set of findings is posted on the collaboration’s web site and can seem in Bodily Evaluation D.
“These outcomes from the Darkish Power Survey shine new gentle on our understanding of the universe and its enlargement,” says Regina Rameika (U.S. Division of Power).

Jessie Muir / DES Collaboration
One of many methods astronomers used DES to measure darkish vitality is thru an impact referred to as weak lensing. On this impact, the gravity of intervening matter, most of it darkish matter, barely bends gentle from distant galaxies, subtly distorting their shapes. Astronomers should observe many galaxies to measure the impact.
Measuring weak lensing with DES allowed astronomers to chart the distribution of darkish matter during the last 6 billion years. If darkish vitality is ramping up the enlargement of the universe, it ought to gradual the expansion of large-scale construction, equivalent to galaxy clusters, in a while in cosmic evolution.
Darkish vitality additionally has a silent, guiding hand in shaping the distribution of galaxies. So analyzing the statistical sample of their clustering is one other manner astronomers measure the repulsive pressure’s altering affect.
The DES staff mixed six years’ price of weak lensing and galaxy distribution knowledge with different datasets (primarily based on baryon acoustic oscillations and Sort Ia supernovae). It’s the primary time all 4 strategies for measuring darkish vitality have been mixed on this manner.
“This was one thing I might have solely dared to dream about when DES began gathering knowledge,” says DES staff member Yuanyuan Zhang (NSF NOIRLab). “Now the dream has come true.”
The outcomes are intriguing.
Whereas in keeping with findings from earlier releases of DES knowledge, the brand new findings widen the doable explanations for darkish vitality. In the usual mannequin of cosmology, the density of darkish vitality is fixed. Whereas these new knowledge match that image, they fail to rule out the choice idea, during which darkish vitality evolves over time.
However each theories face a deeper drawback: They fail to precisely predict how matter has clustered in current astronomical historical past. Observations of the early universe recommend that cosmic construction should be clumpy. But pictures of our cosmic neighborhood present that galaxies are extra easily distributed than anticipated. The brand new DES knowledge solely widen this hole.
“This stress has beforehand been noticed by a number of impartial surveys and stays probably the most intriguing open questions in cosmology,” says Edward Macaulay (Queen Mary College of London), who was not concerned within the analysis.
Macaulay thinks the DES outcomes are an incredible treasure trove, however he additionally thinks that is simply the beginning of one thing larger. “Though this paper represents the tip of observations with DES, it is simply the beginning of a complete new golden age of cosmology,” he says. New observations from the Darkish Power Spectroscopic Instrument (DESI), the Euclid spacecraft, and the 8.4-meter Simonyi Survey Telescope on the Vera Rubin Observatory symbolize a step-change in our efforts to pin down the character of darkish vitality.
“With this new technology of telescopes,” Macaulay says, “we now have a unprecedented alternative to find extra in regards to the largest questions in cosmology.”
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