We introduce an information-driven scalar–tensor theory of gravity in which spacetime curvature couples to a fundamental information density field. The framework modifies Einstein gravity in the weak-field and cosmological regimes while remaining screened in high-density environments via a chameleon mechanism. An early dark energy (EDE) component emerges naturally from the information potential, altering pre-recombination dynamics.
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Brian Cobham
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Brian Cobham (Sun,) studied this question.
www.synapsesocial.com/papers/695d85543483e917927a4acd — DOI: https://doi.org/10.5281/zenodo.18146324