Tue. Mar 10th, 2026

Why cosmology seems to be caught in a vibe shift

SEI 2875670181


Dark Matter Core Defies Explanation NASA ID: GSFC_20171208_Archive_e001774 NASA image release March 2, 2012 This composite image shows the distribution of dark matter, galaxies, and hot gas in the core of the merging galaxy cluster Abell 520, formed from a violent collision of massive galaxy clusters. The natural-color image of the galaxies was taken with NASA's Hubble Space Telescope and with the Canada-France-Hawaii Telescope in Hawaii. Superimposed on the image are "false-colored" maps showing the concentration of starlight, hot gas, and dark matter in the cluster. Starlight from galaxies, derived from observations by the Canada-France-Hawaii Telescope, is colored orange. The green-tinted regions show hot gas, as detected by NASA's Chandra X-ray Observatory. The gas is evidence that a collision took place. The blue-colored areas pinpoint the location of most of the mass in the cluster, which is dominated by dark matter. Dark matter is an invisible substance that makes up most of the universe's mass. The dark-matter map was derived from the Hubble Wide Field Planetary Camera 2 observations, by detecting how light from distant objects is distorted by the cluster galaxies, an effect called gravitational lensing. The blend of blue and green in the center of the image reveals that a clump of dark matter resides near most of the hot gas, where very few galaxies are found. This finding confirms previous observations of a dark-matter core in the cluster. The result could present a challenge to basic theories of dark matter, which predict that galaxies should be anchored to dark matter, even during the shock of a collision. Abell 520 resides 2.4 billion light-years away. To read more go to: www.nasa.gov/mission_pages/hubble/science/dark-matter-cor... Credit: NASA, ESA, CFHT, CXO, M.J. Jee (University of California, Davis), and A. Mahdavi (San Francisco State University)

NASA, ESA, CFHT, CXO, M.J. Jee (University of California, Davis), and A. Mahdavi (San Francisco State University)

A few years ago, the internet caught alight with talk of a “vibe shift” in what counts as cool. Skinny jeans and minimalism were out; baggy trousers and messy hair were in. Cue a minor panic for ageing millennials everywhere as it dawned on them that they were suddenly out of touch.

Now, something similar is happening in cosmology. For years, physicists thought they had a neat understanding of how the universe works, a simple and elegant framework called the standard model of cosmology that gave an excellent account of how it began and evolved. At the heart of the model is dark energy, a force we admittedly can’t identify but behaves predictably to force the universe to expand.

Then, last year, explosive results from a telescope survey seemed to show the unthinkable: dark energy has been getting weaker over the history of the universe. If that is true, then the standard model of cosmology will need to be rewritten. In a package of three special features, we delve into the beauty of the standard model, reveal how endangered it really is and explore what might replace it.


Where the attachment to the old model is motivated by fear or nostalgia, that won’t do

It must be said, though, that many physicists are still reluctant to abandon their cherished model. To some extent, this is fair enough. As with so many apparently convincing results in modern physics, the dark energy findings may not stand the test of time. But where the attachment to the old model is motivated by fear of the unknown or nostalgia for simpler times, that won’t do.

Scientists tend not to talk of vibe shifts, but of paradigm shifts – periods when our lens of understanding fundamentally changes. History teaches us that paradigm shifts are a good thing. They are discombobulating, no question, but allow us to see reality more clearly. We aren’t yet sure if the challenge to dark energy really will amount to a paradigm shift akin to the quantum or Copernican revolutions – but if it does, we will look back on this period of cosmology as a thrilling time to be alive. Bring on the new vibe.

By uttu

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