This framework modifies Einstein gravity and introduces an information-driven scalar–tensor theory to address significant cosmological tensions.
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 (2026) studied this question.
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