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February 14, 20260 citationsOpen Access

Deriving MOND from Complexity Binding Theory: Field Equation Solutions and Falsifiable Predictions

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DDDavid Dudaš

Key Points

  • The research aims to derive Modified Newtonian Dynamics (MOND) from Complexity Binding Theory (CBT) and validate its predictions.
  • Derived MOND from the scalar binding field of CBT without prior assumptions.
  • Solved static field equilibrium equations to obtain an interpolation function.
  • Tested the theory on 22 SPARC galaxies with observed declining rotation curves.
  • Utilized the CLASS Boltzmann code for cosmological scale validation.
  • CBT predicts declining rotation curves, contrasting MOND's flat curves.
  • Outperformed MOND in explaining observations across all 22 SPARC galaxies (mean χ² ratio 24:1).
  • Matched cosmological data with a fixed dark matter density ω_cdm = 0.1216, comparable to ΛCDM results.

Abstract

This paper derives Modified Newtonian Dynamics (MOND) directly from the scalar binding field of Complexity Binding Theory (CBT), without assuming MOND a priori. Solving the static field equilibrium equation yields an interpolation function that differs from standard MOND in the deep regime (x < 0. 1): CBT predicts declining outer rotation curves where MOND predicts flat curves. Testing on 22 SPARC galaxies with observed declining rotation curves confirms this prediction, with CBT outperforming MOND on all 22 galaxies (mean χ² ratio 24: 1). The theory is further validated at cosmological scales using the CLASS Boltzmann code, with the CBT-predicted dark matter density ωcdm = ωb × 2e = 0. 1216 (fixed, not fitted) matching Planck 2018 TT+TE+EE power spectra at χ²/dof = 1. 09 — comparable to ΛCDM's 1. 10 with one fewer free parameter. This is Paper III of the CBT program; Paper I established empirical success on 175 SPARC galaxies, and Paper II provided the theoretical foundations.

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Cite This Study

David Dudaš (2026) studied this question.

synapsesocial.com/papers/699011932ccff479cfe58509https://doi.org/10.5281/zenodo.18616671
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