Bell witnesses supply KL lower bounds to local models that, when weighed against complexity costs, favor compact nonlocal descriptions over locality or overly flexible alternatives in CHSH data.
Schwarz, Estimating the dimension of a model, The Annals of Statistics 6, 461 (1978)
2 Pith papers cite this work. Polarity classification is still indexing.
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Interacting scalar fields coupled to Gauss-Bonnet gravity yield viable dark energy and dark matter models that match Pantheon+ and DES supernova data while preferring over LambdaCDM at high redshifts with Roman mocks.
citing papers explorer
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Complexity-Aware Theory Testing from Bell Witnesses
Bell witnesses supply KL lower bounds to local models that, when weighed against complexity costs, favor compact nonlocal descriptions over locality or overly flexible alternatives in CHSH data.
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Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity
Interacting scalar fields coupled to Gauss-Bonnet gravity yield viable dark energy and dark matter models that match Pantheon+ and DES supernova data while preferring over LambdaCDM at high redshifts with Roman mocks.