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Home»Science»The enlargement of our universe could also be slowing down. What does that imply for darkish power?
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The enlargement of our universe could also be slowing down. What does that imply for darkish power?

VernoNewsBy VernoNewsNovember 6, 2025No Comments5 Mins Read
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The enlargement of our universe could also be slowing down. What does that imply for darkish power?
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As if darkish power weren’t already mysterious and baffling sufficient, new analysis means that this unknown pressure will not be driving galaxies aside at an accelerating fee anymore.

This exceptional end result comes from analysis that implies that the enlargement of the universe has already begun to sluggish, opposite to the at the moment favored perception that darkish power remains to be accelerating the enlargement of the cosmos. The invention additionally follows outcomes from the Darkish Power Spectroscopic Instrument (DESI) that final 12 months indicated that darkish power is weakening.

This analysis couldn’t solely revolutionize our understanding of the universe as it’s in the present day, but additionally provide clues about how our cosmos will finish. If darkish power has already misplaced the battle towards gravity, the following step after slowing cosmic enlargement may very well be the contraction of house, and that might counsel the universe will finish in a “Large Crunch” state of affairs akin to the Large Bang taking part in in reverse.


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The researchers behind this discovery are already hailing it as a attainable paradigm shift in how we take into consideration the very nature of the universe. “Our research reveals that the universe has already entered a section of decelerated enlargement at this time epoch and that darkish power evolves with time far more quickly than beforehand thought,” Younger-Wook Lee, group chief and researcher at Yonsei College in South Korea, mentioned in a press release. “If these outcomes are confirmed, it could mark a serious paradigm shift in cosmology for the reason that discovery of darkish power 27 years in the past.”

Darkish power evolves

The existence of darkish power was first urged in 1998 when two separate groups of astronomers noticed distant Kind Ia supernovas, additionally known as “commonplace candles” because of the truth that their uniform mild output can be utilized to measure cosmic distances. This revealed that the additional away a galaxy was, the sooner it was receding away. This indicated to the 2 groups, who obtained the 2011 Nobel Prize in Physics for the invention, that the velocity at which the universe expands is growing. Darkish power was launched as a placeholder pressure to elucidate this accelerating enlargement.

Over the next three a long time, whereas scientists have been unable to conclusively decide what darkish power is, they’ve discovered that this pressure is dominant, accounting for roughly 68% of the universe’s whole energy-matter funds. Researchers additionally found that darkish power had not all the time been dominant, showing to start its rule and begin rushing up the enlargement of the universe round 5 billion years in the past, or roughly 9 billion years after the Large Bang.

The primary indication that darkish power will not be as dominant as beforehand thought emerged courtesy of the primary outcomes from DESI in Spring 2024. This new chink within the armor of darkish power resulted from Lee and colleagues from Yonsei College discovering that Kind Ia supernova will not be fairly so commonplace in any case. That’s as a result of their brightness could also be strongly affected by the age of the progenitor stars of those explosive occasions. The truth is, this group discovered that even after the sunshine from Kind Ia supernovas was standardized, Kind Ia supernovas from populations of youthful stars had been fainter than these belonging to older stellar populations.

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A NASA/ESA Hubble Area Telescope view of SN UDS10Wil, a supernova that exploded greater than 10 billion years in the past — probably the most distant Kind Ia supernova ever detected. (Picture credit score: NASA, ESA, and Z. Levay (STScI))

Utilizing a pattern of 300 galaxies, the analysis urged a significance of 99.99% that the dimming of distant Kind Ia supernovas can come up not simply from cosmological results just like the enlargement of house, but additionally from stellar results. Correcting for bias, the group discovered that their outcomes rule out the at the moment favored mannequin of cosmic evolution, the usual mannequin of cosmology, or the Lambda Chilly Darkish Matter (LCDM) mannequin, and its recipe of darkish power.

Nevertheless, the main end result rising from this analysis is the implication that the universe isn’t increasing at an accelerating fee, however has already transitioned right into a state of decelerating enlargement. That goes even additional than DESI’s hints at weakening darkish power.

“Within the DESI mission, the important thing outcomes had been obtained by combining uncorrected supernova information with baryonic acoustic oscillations measurements, resulting in the conclusion that whereas the universe will decelerate sooner or later, it’s nonetheless accelerating at current,” Lee defined. “In contrast, our evaluation — which applies the age-bias correction — reveals that the universe has already entered a decelerating section in the present day.”

The subsequent step for the group will likely be to verify these outcomes by conducting an “evolution-free check” using solely younger Kind Ia supernovas from younger galaxies at a variety of distances. The Vera C. Rubin Observatory, which has simply begun observing the cosmos with the world’s largest digital digital camera from its place atop Cerro Pachón in Chile, is poised to play a serious function on this investigation.

“Throughout the subsequent 5 years, with the Vera C. Rubin Observatory discovering greater than 20,000 new supernova host galaxies, exact age measurements will enable for a much more strong and definitive check of supernova cosmology,” Chul Chung, group member and Yonsei College researcher, mentioned.

The group’s analysis was revealed on Wednesday (Nov. 5) within the journal Month-to-month Notices of the Royal Astronomical Society.

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