Japan is also leading on mineral-based detection. The third "Mineral Detection of Neutrinos and Dark Matter" (MDνDM'25) meeting was held in Yokohama in May 2025, hosted by JAMSTEC, focused on using mineral deposits as natural, long-exposure particle detectors .
Modified Newtonian Dynamics (MOND) proposes that gravity behaves differently at low accelerations, eliminating the need for invisible dark matter . It successfully predicts galaxy rotation curves, but recent evidence has significantly challenged it:
The prevailing scientific consensus remains that dark matter is favored over modified gravity as an explanation for the full range of cosmological and astrophysical data .
In April 2026, the German Research Foundation (DFG) approved €5.3 million in funding for the DELight experiment—a direct search for light dark matter using superfluid helium-4 as the target material . The consortium is led by Heidelberg University, with partners at KIT (Karlsruhe) and the University of Freiburg
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DELight focuses on particles with very low mass as candidates for dark matter, explained Professor Kathrin Valerius . The detector uses ultra-cold superfluid helium instrumented with large-area magnetic microcalorimeters (LAMCALs), optimized to detect very low-mass dark matter particles that would produce tiny energy depositions
. Helium offers several advantages: its low nuclear mass and intrinsic radiopurity make it ideal for low-threshold experiments, and it enables scalable detector designs
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The OMNIA research group at the Max Planck Institute for Nuclear Physics (MPIK) in Heidelberg is also active in dark matter searches through microlensing and astroparticle experiments .
The FASER (Forward Search Experiment) at the Large Hadron Collider continues to produce results. In April 2026, it reported new searches for dark photons using 177 fb⁻¹ of proton-proton collision data from LHC Run 3 . Dark photons are hypothetical mediators of a hidden "dark sector" that could explain dark matter
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FASER's new search uses data collected between 2022 and 2024, corresponding to an integrated luminosity of 177 fb⁻¹ at a centre-of-mass energy of 13.6 TeV . The observed limit excludes dark photons with masses between about 10 and 150 MeV and couplings of around 10⁻⁵–10⁻⁴, ruling out part of the cosmologically viable parameter space
. CERN's EP-News highlighted in June 2026 that FASER has opened new windows into both dark sectors and TeV-scale neutrino physics
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The field is moving on multiple fronts—Earth-scale natural detectors (Japan), new dedicated cryogenic experiments (DELight in Heidelberg), collider-based dark sector searches (FASER at CERN), and continued tension between the dark matter paradigm and modified gravity alternatives. Direct detection has not yet found dark matter, but the sensitivity of experiments is improving rapidly . Next-generation detectors such as DarkSide-20k, DARWIN/XLZD, and PandaX-xT are in design, R&D, or construction phases
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