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- The universe\u2019s expansion has already begun to slow,<\/strong> says a new study from Yonsei University. This challenges the long-held belief that the universe is rapidly accelerating due to dark energy.<\/li>\n
- Researchers found that type Ia supernovas<\/strong> \u2013 the \u201cstandard candles\u201d used to measure cosmic expansion \u2013 are affected by the age of their progenitor stars. Thus, previous evidence for acceleration may be faulty.<\/li>\n
- After correcting for this bias,<\/strong> the data no longer fit the standard Lambda-CDM cosmological model. Now, it aligns with newer evidence that dark energy weakens and evolves over time. This would mark a huge paradigm shift in cosmology.<\/li>\n<\/ul>\n
The Royal Astronomical Society published this original story at 00:01 GMT on November 6, 2025. Edits by EarthSky.<\/p>\n
Universe\u2019s expansion is slowing down, not speeding up<\/h3>\n
The universe\u2019s expansion may actually have started to slow rather than accelerating at an ever-increasing rate as previously thought, a new study suggests.<\/p>\n
The \u201cremarkable\u201d findings published November 6, 2025, in Monthly Notices of the Royal Astronomical Society<\/em> cast doubt on the long-standing theory that a mysterious force known as dark energy is driving distant galaxies away increasingly faster.<\/p>\n
Instead, they show no evidence of an accelerating universe.<\/p>\n
If the results are confirmed, it could open an entirely new chapter in scientists\u2019 quest to uncover the true nature of dark energy, resolve the Hubble tension, and understand the past and future of the universe.<\/p>\n
The universe is in a phase of decelerated expansion<\/h3>\n
Lead researcher Young-Wook Lee of Yonsei University in South Korea said: <\/p>\n
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Our study shows that the universe has already entered a phase of decelerated expansion at the present epoch and that dark energy evolves with time much more rapidly than previously thought.<\/p>\n
If these results are confirmed, it would mark a major paradigm shift in cosmology since the discovery of dark energy 27 years ago.<\/p>\n<\/blockquote>\n
For the past three decades, astronomers have widely believed that the universe is expanding at an ever-increasing rate, driven by an unseen phenomenon called dark energy that acts as a kind of anti-gravity.<\/p>\n
This conclusion, based on distance measurements to faraway galaxies using type Ia supernovas, earned the 2011 Nobel Prize in Physics.<\/p>\n
A new look at type 1a supernovas as standard candles<\/h3>\n
However, a team of astronomers at Yonsei University have now put forward new evidence that type Ia supernovas, long regarded as the universe\u2019s standard candles, are in fact strongly affected by the age of their progenitor stars.<\/p>\n
Even after luminosity standardization, supernovas from younger stellar populations appear systematically fainter, while those from older populations appear brighter.<\/p>\n
Based on a much larger host-galaxy sample of 300 galaxies, the new study confirmed this effect at extremely high significance (99.999% confidence). This suggests that the dimming of distant supernovas arises not only from cosmological effects but also from stellar astrophysics effects.<\/p>\n
When this systematic bias was corrected, the supernova data no longer matched the standard Lambda-CDM cosmological model with a cosmological constant, researchers said.<\/p>\n
Instead, it aligned far better with a new model favored by the Dark Energy Spectroscopic Instrument (DESI) project, derived from baryonic acoustic oscillations (BAO) \u2013 effectively the sound of the Big Bang \u2013 and cosmic microwave background (CMB) data.<\/p>\n
The corrected supernova data and the BAO+CMB-only results both indicate that dark energy weakens and evolves significantly with time.<\/p>\n
More importantly, when the corrected supernova data were combined with BAO and CMB results, the standard Lambda-CDM model was ruled out with overwhelming significance, the researchers said.<\/p>\n
![\"A](\"https:\/\/earthsky.org\/upl\/2025\/11\/DESI-instrument-Berkeley-Lab-CC-BY-40-scaled-e1762278455738.jpeg\")
DESI is a state-of-the-art instrument which maps distant objects to study dark energy. Image via Marilyn Sargent\/ Berkeley Lab\/ RAS\/ CC BY 4.0.<\/figcaption><\/figure>\n A look at the data<\/h3>\n
![\"Two](\"https:\/\/earthsky.org\/upl\/2025\/11\/Graph-on-slowing-universe-RAS-Son-et-al-e1762278188462.jpg\")
The Hubble residual diagram before (top) and after (bottom) the age-bias correction. Corrections are applied to supernova data from the Dark Energy Survey project. After correction, the dataset no longer supports the Lambda-CDM model (red line) with a cosmological constant. But instead it more closely fits with a time-varying dark energy model favored by a combined analysis using only baryonic acoustic oscillations and cosmic microwave background data (blue line). Image via Son et al.\/ RAS\/ CC BY 4.0.<\/figcaption><\/figure>\n ![\"Line](\"https:\/\/earthsky.org\/upl\/2025\/11\/Line-graph-for-slowing-universe-RAS-Son-et-al-e1762278326604.jpg\")
This diagram shows how the universe appears to be in a state of decelerated expansion (red line). The dotted vertical line marks the present epoch, while the black line shows the Lambda-CDM prediction. The green and red lines represent the new study\u2019s model before (green) and after (red) age-bias correction, consistent with baryonic acoustic oscillations and cosmic microwave background data (blue line). Image via RAS\/ Son et al.\/ CC BY 4.0.<\/figcaption><\/figure>\n The universe\u2019s expansion is not rapidly accelerating<\/h3>\n
Most surprising of all, this combined analysis indicates the universe is not accelerating today as previously thought. Instead, it has already transitioned into a state of decelerated expansion.<\/p>\n
Professor Lee said: <\/p>\n
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In the DESI project, the key results were obtained by combining uncorrected supernova data with baryonic acoustic oscillations measurements, leading to the conclusion that while the universe will decelerate in the future, it is still accelerating at present.<\/p>\n
By contrast, our analysis \u2014 which applies the age-bias correction \u2014 shows that the universe has already entered a decelerating phase today. Remarkably, this agrees with what is independently predicted from BAO-only or BAO+CMB analyses, though this fact has received little attention so far.<\/p>\n<\/blockquote>\n
To further confirm their results, the Yonsei team are now carrying out an \u201cevolution-free test.\u201d It uses only supernovas from young, coeval host galaxies across the full redshift range. The first results already support their main conclusion.<\/p>\n
Co-author Chul Chung said:<\/p>\n
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Within the next five years, with the Vera C. Rubin Observatory discovering more than 20,000 new supernova host galaxies, precise age measurements will allow for a far more robust and definitive test of supernova cosmology.<\/p>\n<\/blockquote>\n
The Vera C. Rubin Observatory, which sits on a mountain in the Chilean Andes, is home to the world\u2019s most powerful digital camera. It began scientific operations this year and could answer vital questions about our own solar system and the wider universe.<\/p>\n
![\"A](\"https:\/\/earthsky.org\/upl\/2025\/11\/Vera-C.-Rubin-Observatory-RAS-e1762278552375.jpeg\")
The Vera C. Rubin Observatory began scientific operations this year and could answer vital questions about our own solar system and the wider universe. Image via RubinObs\/ NOIRLab\/ SLAC\/ NSF\/ DOE\/ AURA\/ RAS.<\/figcaption><\/figure>\n Dark energy is still mysterious<\/h3>\n
After the Big Bang and the rapid expansion of the universe some 13.8 billion years ago, gravity slowed it down. But in 1998, it was established that 9 billion years after the universe began, its expansion had started to speed up again, driven by a mysterious force.<\/p>\n
Astronomers dubbed this dark energy, but despite it making up about 70% of the universe, it is still considered to be one of the greatest mysteries in science.<\/p>\n
Last year, data from DESI in Tucson, Arizona, suggested that the force exerted by dark energy had changed over time. And more evidence for that has been growing ever since.<\/p>\n
The hope is that with these new tools in their arsenal, astronomers will now be better equipped to find clues about what exactly dark energy is and how it influences the universe.<\/p>\n
Bottom line: New research suggests that we don\u2019t live in an rapidly accelerating, expanding universe after all. DESI data suggest the universe\u2019s expansion is already slowing.<\/p>\n
Source: Strong Progenitor Age-bias in Supernova Cosmology. II. Alignment with DESI BAO and Signs of a Non-Accelerating Universe<\/p>\n
Via Royal Astronomical Society<\/p>\n
Read more: A new data release hints dark energy may be weakening<\/p>\n
- Researchers found that type Ia supernovas<\/strong> \u2013 the \u201cstandard candles\u201d used to measure cosmic expansion \u2013 are affected by the age of their progenitor stars. Thus, previous evidence for acceleration may be faulty.<\/li>\n