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March 19, 2026Open Access

Dark Matter as Thermodynamic Informational Residue of Scalar-Field-Driven Cosmic Expansion

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Authors

JPJ. Adam Perry

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Overview

This proposal reveals dark matter as entropic residue from scalar-field-driven cosmic expansion, implying a novel understanding of cosmic structure.

Key Points

  • To explore the concept that dark matter is an informational residue from scalar-field-driven cosmic expansion rather than a particle.
  • Develop a theoretical model involving a minimally coupled scalar information field.
  • Analyze irreversible quantum-to-classical transitions causing the formation of a pressureless fluid.
  • Determine the energy density equation relevant to dark matter.
  • Predict the behavior of dark matter fraction at different redshifts.
  • Established dark matter as a cold fluid with energy density scaling as a^(-3).
  • Showed that the model aligns with current cold dark matter observations.
  • Predicted that the current dark matter fraction should converge to approximately 0.38 at higher redshifts.

Cite This Study

J. Adam Perry (2026) studied this question.

synapsesocial.com/papers/69bb9357496e729e62981663https://doi.org/10.5281/zenodo.19066061
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