We present a scalar field framework in which the chronon field χ, governed by the Lagrangian L= P(X)−V(χ) + βχρbar, addresses five observational domains through distinct sectors of a single action. Holographic derivation. Enforcing the Bekenstein–Hawking entropy bound restricts the effective thermodynamic dimensionality of the field to d= 2 in the weak-acceleration regime. The resulting scale-invariant equation of state p= ρ/2 uniquely determines the kinetic Lagrangian P(X) ∝X3/2. The composite form P(X) = X + αX3/2 admits an exact algebraic solution in spherical symmetry, yielding the standard MOND in- terpolation function ν(y) = (1 + 1 + 4/y)/2, with ν(1) = φ = (1 + √5)/2 (golden ratio). Galactic dynamics. We fit this model to 171 SPARC galaxies with one free param- eter per galaxy (Υ⋆) and a globally fixed a0. At optimized a0 = 1.0 ×10−10 m/s2 we obtain χ2/dof = 6.48 and reproduce the Radial Acceleration Relation with 0.144 dex scatter. A double-counting theorem establishes that on galactic scales the field acts exclusively as a metric modifier. Galaxy clusters. A running acceleration scale a0,eff(M) = a01+ΞmaxM/(M+Msat), activated by the potential sector V(χ), reduces the MOND cluster mass deficit from ∼2.1×to∼1.07×across five clusters (RMS: 0.303 →0.089 dex) with two global parameters. Gravitational waves. Extending the potential with a χ6/M2 HL term from Hoˇrava- Lifshitz UV completion produces a first-order cosmological phase transition at Tc ≈ 0.4 MeV. The predicted gravitational wave spectrum peaks at f = 5.1 nHz with h2Ω = 3 ×10−10, coinciding with the NANOGrav 15-year signal. One field, one Lagrangian, four free dark-sector parameters, five observational do- mains.
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Anton Karpov
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Anton Karpov (Tue,) studied this question.
www.synapsesocial.com/papers/69be37aa6e48c4981c6777cf — DOI: https://doi.org/10.5281/zenodo.19073054
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