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    Home»Physics»Decades-Old Dark Matter Explanation Fails Its Most Direct Test Yet
    Physics

    Decades-Old Dark Matter Explanation Fails Its Most Direct Test Yet

    By Yale UniversityJuly 12, 20263 Comments4 Mins Read
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    COSINE 100 Sodium Iodide Detector Array
    A decades-old dark matter claim is facing a decisive new challenge. The result clears the way for future searches to focus on unexplored signals and lower-mass dark matter candidates. Credit: Yale University

    Two experiments designed to detect signals directly found no evidence for the signal reported by an earlier experiment.

    For nearly three decades, one dark matter claim has refused to disappear. In 1997, the DAMA/NaI experiment detected a signal that changed with the seasons, a pattern that seemed to match what some physicists expected if Earth were moving through a halo of dark matter.

    The follow-up DAMA/LIBRA experiment reported a similar annual pattern, keeping the claim alive. But many physicists remained unconvinced because other direct detection experiments did not see the same signal.

    To test the result more directly, researchers built two sister experiments, ANAIS-112 and COSINE-100, using the same basic approach as DAMA/NaI and DAMA/LIBRA. In 2021, the first ANAIS-112 dataset showed no matching seasonal variation, weakening the case that dark matter caused the original DAMA signal.

    A new study published in Physical Review Letters combining data from ANAIS-112 and COSINE-100 now rules out the dark matter explanation with greater confidence.

    Same method tests the claim

    All four experiments were designed to look for signs of weakly interacting massive particles, a leading class of hypothetical dark matter particles, scattering off nuclei inside sodium iodide crystals.

    If dark matter were producing the signal, the rate should rise and fall slightly over the year. That is because Earth’s motion around the Sun changes the detector’s speed relative to the Milky Way’s dark matter halo.

    DAMA/NaI and DAMA/LIBRA reported this kind of annual modulation. The problem is that their results have remained difficult to reconcile with other direct detection experiments and with theoretical model predictions.

    Until recently, one major uncertainty remained. The DAMA signal had not been tested robustly using experiments with closely matched detector materials and methods.

    Combined data rejects modulation

    ANAIS-112 and COSINE-100 were designed to provide that comparison. Both used sodium iodide targets like DAMA, while adding features intended to reduce background noise and improve event detection.

    When researchers combined the new datasets and analyzed the relevant energy ranges, they found no significant evidence of annual modulation.

    The result effectively rules out dark matter as the source of the DAMA/LIBRA signal. It does not explain what caused the earlier observation, but it removes a long-standing obstacle for the field.

    The researchers say the finding allows future dark matter searches to move forward without being weighed down by an unresolved detection claim.

    Reference: “Combined Annual Modulation Dark Matter Search with COSINE-100 and ANAIS-112” by N. Carlin, J. Y. Cho, J. J. Choi, S. Choi, A. C. Ezeribe, L. E. França, C. Ha, I. S. Hahn, S. J. Hollick, I. S. Hahn, S. J. Hollick, S. B. Hong, E. J. Jeon, H. W. Joo, W. G. Kang, M. Kauer, B. H. Kim, H. J. Kim, J. Kim, K. W. Kim, S. H. Kim, S. K. Kim, W. K. Kim, Y. D. Kim, Y. H. Kim, Y. J. Ko, D. H. Lee, E. K. Lee, H. Lee, H. S. Lee, H. Y. Lee, I. S. Lee, J. Lee, J. Y. Lee, M. H. Lee, S. H. Lee, S. M. Lee, Y. J. Lee, D. S. Leonard, N. T. Luan, V. H. A. Machado, B. B. Manzato, R. H. Maruyama, R. J. Neal, S. L. Olsen, H. K. Park, H. S. Park, J. C. Park, J. S. Park, K. S. Park, K. Park, S. D. Park, R. L. C. Pitta, H. Prihtiadi, S. J. Ra, C. Rott, K. A. Shin, D. F. F. S. Cavalcante, M. K. Son, N. J. C. Spooner, L. T. Truc, L. Yang, G. H. Yu, J. Amaré, J. Apilluelo, S. Cebrián, D. Cintas, I. Coarasa, E. García, M. Martínez, Y. Ortigoza, A. Ortiz de Solórzano, T. Pardo, J. Puimedón, M. L. Sarsa and C. Seoane, 17 September 2025, Physical Review Letters.
    DOI: 10.1103/9j7w-qp1c

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    Astrophysics Cosmology Dark Matter Particle Physics Popular Yale University
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    3 Comments

    1. Jojo on July 13, 2026 12:07 am

      Can we retire the idea of dark matter being something real now?

      It will be difficult for all those “scientists” that have dedicated their lives and research to the belief that dark matter is real, though.

      Reply
      • Robert Welch on July 13, 2026 7:31 am

        Hard to let go of the notion your life’s work was for nothing.

        Reply
    2. Ralph Johnson on July 20, 2026 12:40 pm

      “Space is often treated as an empty vacuum because we look right through the darkness. However, it is actually an absolute soup packed with a continuous network of overlapping forces at all times. This includes cosmic rays, gamma rays, x-rays, ultraviolet light, visible photons, infrared thermal waves, microwaves, radio waves, and massive fields of neutrinos and magnetic flux lines.

      This background matrix acts exactly like a perfectly clean pane of glass: it is completely transparent to our eyes, but it still has a real physical density and a constant, built-in background pressure.

      The massive energy and torque we observe across galaxies aren’t coming from missing, invisible particles. Instead, they are the natural result of all these fields moving through the Torsion Hill—the massive macro-scale structural layout of the universe. The geometry of the Torsion Hill acts as a giant dimensional rift, bending and plumbing this pressurized, transparent medium into the spinning vortex structures we see throughout the cosmos.”

      Reply
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