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February 19, 20260 citationsOpen Access

Logarithmic Velocity Correction in Galaxy Rotation Curves: An Empirical Test with 151 SPARC Galaxies

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YFYanush FeshterRSRSI Multi-Agent Suite

Key Points

  • To assess a logarithmic velocity correction model's effectiveness using galaxy rotation curves from the SPARC database.
  • Analyzed rotation curves from 151 galaxies in the SPARC database
  • Fitted model using Nelder-Mead minimization and Gaussian priors on mass-to-light ratios
  • Employed bootstrap resampling for statistical analysis
  • Compared performance to MOND using AIC and data residuals
  • Logarithmic model achieved median data residuals of 0.54, while MOND had 0.14
  • 60% sample favored MOND based on data residuals, 85% preferred by AIC
  • Coupling parameter γ showed a scaling relation with baryonic mass, α = 0.485 ± 0.030
  • No significant correlation was found for the fitted scale length r₀ with baryonic mass or galaxy extent

Abstract

We present an empirical test of a logarithmic velocity correction model using 151 galaxy rotation curves from the SPARC database (Lelli, McGaugh by AIC (ΔAIC = +2. 6), MOND is preferred in 85%. The logarithmic model's contribution is not superior goodness-of-fit but a confirmed scaling prediction and consistency with stellar population constraints. 2. Scaling relation. Using baryonic masses computed with fixed mass-to-light ratios (Υdisk = 0. 5, Υbulge = 0. 7) independent of the fitting procedure, the coupling parameter scales as γ ∝ Mbar^α with α = 0. 485 ± 0. 030, consistent with the geometric prediction α = 0. 50 within 0. 5σ. Bootstrap resampling (10⁴ iterations) yields 68% CI = 0. 457, 0. 512 and 95% CI = 0. 431, 0. 540, both containing the predicted value. The result is stable across mass-to-light ratio assumptions (α ∈ 0. 467, 0. 504 for Υdisk ∈ 0. 3, 0. 8). 3. Scale length. The fitted r₀ ≈ 0. 6 kpc shows no significant correlation with baryonic mass (Spearman ρ = 0. 149), galaxy extent (ρ = 0. 108), or outer acceleration (ρ = −0. 083), suggesting it represents a structural property of the velocity correction rather than a scaling of the baryonic distribution. 4. Limitations. Individual gas-dominated dwarf galaxies (e. g. , DDO 154) remain challenging. The high-mass regime shows a flattened local slope (αₗocal ≈ 0. 37), consistent with a mass-dependent deviation from the global scaling. No comparison with NFW halo fits is included. Methodology. Fitting uses Nelder-Mead minimization with Gaussian priors on stellar mass-to-light ratios. Quality cuts require ≥5 data points, successful convergence, and γ > 10 km²/s². MOND comparison uses the RAR interpolation function with free a₀. All analysis code is in Python (NumPy, SciPy). Multi-agent analysis. The analysis was independently cross-checked using multiple large language model systems to detect logical inconsistencies, pipeline errors, and methodological issues. Related work: - TKWC Nodes 734–735: doi: 10. 5281/zenodo. 18650668 - Topological Screening of Dark Energy: doi: 10. 5281/zenodo. 18422868 The Entropy Sink: doi: 10. 5281/zenodo. 18479788

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Cite This Study

Feshter et al. (2026) studied this question.

synapsesocial.com/papers/6996a8d4ecb39a600b3eff3bhttps://doi.org/10.5281/zenodo.18670862
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