Observational exploration derives constraints on dark matter parameters using weak-lensing in galaxy clusters, suggesting future testing methods.
This companion article provides a first observational exploration of the infrared vacuum-response framework through weak-lensing bridges between galaxy clusters. It uses published bridge detections and non-detections to derive preliminary constraints on the coherence parameters of the model and to define a likelihood-based strategy for future empirical tests with larger weak-lensing samples.
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Daniel Bensaid (2026) studied this question.
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