Randomized trial reveals temporal kernel effects on gravitational waves, suggesting implications for understanding fundamental physics.
This is Paper XIV in the History-Dependent Gravity (HDG) series. Building on the dynamical relaxation framework of HDG XIII, we derive the observational consequences of the scale-free temporal kernel K(t) ∝ 1/t that emerges from the relaxation dynamics. Main results:(1) The kernel is uniquely selected by scale invariance of the relaxation equation (Appendix C).(2) Fourier transform yields a universal logarithmic response K̃(ω) ∼ -log(iω) (Appendix A).(3) Two distinct observable signatures: - Source-level: GW phase drift δΨ(f) ∝ f^(-13/3) log f in compact binary inspirals (Section 3) - Propagation-level: logarithmic dispersion during cosmological travel (Section 4)(4) Fisher matrix analysis shows LISA can probe the fundamental coupling λ₀ down to ~10⁻³ through hierarchical population analysis (Appendix B). The logarithmic phase drift is irreducible — it cannot be absorbed into standard waveform parameters (masses, spins, distance) — and provides a direct, falsifiable test of directional time geometry. All observable effects are controlled by the same fundamental parameter λ₀, with λ_eff encoding its history-dependent realization. Part of the series "Temporal Nonlocality and Fundamental Physics" (Zenodo community).
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Alik Gimranov (2026) studied this question.
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