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Two lenses on the same evidence. Source weight and the primary source ratio show what each rests on.
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Investigated
Image: nature.com
Collapse models are tested by looking for departures from ordinary quantum predictions: loss of interference, anomalous force noise, heating, or other decoherence-like signals as systems become larger or more massive. Key platforms include matter-wave interferometers, mechanical and optomechanical resonators, superconducting circuits, ultracold cantilevers, gravitational-wave detectors, and Bell experiments designed to probe localized collapse assumptions. So far, results mainly bound model parameters rather than decisively establish or exclude every collapse theory.
Two lenses on the same evidence. Source weight and the primary source ratio show what each rests on.
A serious dissenting emphasis is that null results do not eliminate collapse theories as a class. Different models predict different signatures and parameter scales, and environmental decoherence can mimic collapse. Some proposals therefore shift toward less conventional tests—such as spacelike-separated collapse conditions in Bell experiments, dissipative collapse models, or hybrid electromechanical measurements—rather than treating existing bounds as a final verdict.
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