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World's largest particle smasher halts for upgrade to boost hunt for dark matter
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World's largest particle smasher halts for upgrade to boost hunt for dark matter

The world's most powerful particle accelerator will shutter operations Monday for four years of renovations to dramatically boost its collision capacity and the potential for.

Original source cited and editorially framed by Cosmos Week. Phys. org Physics
Editorial signatureCosmos Week Editorial Desk
Published27 Jun 2026 19: 29 UTC
Updated2026-06-27
Coverage typeScience journalism
Evidence levelJournalistic coverage
Read time4 min read

Key points

  • Focus: The world's most powerful particle accelerator will shutter operations Monday for four years of renovations to dramatically boost its collision
  • Detail: Science reporting: verify primary technical documentation
  • Editorial reading: science reporting; whenever possible, verify the cited primary source.
Full story

The world's most powerful particle accelerator will shutter operations Monday for four years of renovations to dramatically boost its collision capacity and the potential for unlocking one of the greatest mysteries of the universe: dark. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

This matters because cosmology operates at the edge of what current instruments can measure, where systematic errors and model assumptions are never trivial. Small discrepancies between independent measurements have historically pointed toward missing physics rather than simple calibration errors, and the ongoing tension in the Hubble constant is a live example of how a persistent disagreement between methods can reshape the theoretical landscape. Each new dataset that approaches this territory with independent systematics adds real information to a problem that has resisted easy resolution for more than a decade. This article has been reviewed according to Science X's editorial process and policies. Once completed, the enhanced particle smasher, bearing the new name High Luminosity LHC (HL-LHC), is scheduled to begin operations in June 2030 and to run for about a decade.

From Monday, we will be entering a new phase," HL-LHC project chief Markus Zerlauth told reporters. There are still many discoveries to be made. " The goal is to increase the "luminosity"—that is, the total number of collisions produced over a given period, by a factor of 10.

The total cost of the upgrade is expected to come in at 1.2 billion Swiss francs ($1.5 billion). That will be covered by CERN membership fees, along with in-kind contributions making up 10, 15 percent of the total, including from the United States, Japan, Canada and China.

The upgrade will require fully replacing the components in 1.2 kilometers (0.75 miles) of the 27-kilometer (17-mile) tunnel. Once operational, between 140 and 200 collisions will occur each time two packets of particles meet inside detectors in the tunnel, up from 60 currently.

The relevance goes beyond one dataset because even small shifts in measured parameters can matter when the field is testing the limits of the standard cosmological model. The Lambda-CDM framework describes the observable universe with remarkable economy, but its success rests on two components, dark matter and dark energy, whose physical nature remains entirely unknown. Any credible measurement that tightens or loosens the constraints on those components moves the entire theoretical enterprise forward, regardless of whether the immediate result looks dramatic on its own terms.

Overall, "the increased number of collisions will allow us to collect up to 100 times more data," Zerlauth said. But "AI does not replace physicists," insisted Nedaa-Alexandra Asbah, a research physicist at CERN's ATLAS experiment, which helped discover the Higgs boson using the LHC.

Because this item comes through Phys. org Physics as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to see whether the effect survives when independent surveys, different calibration strategies and tighter control of systematic uncertainties enter the picture. Programmes such as Euclid, DESI and the Rubin Observatory will deliver datasets over the next several years that cover the same parameter space with largely independent methods. If the current signal persists through those tests, its theoretical implications will become impossible to set aside.

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