What question did this study set out to answer?

The aim is to extend the Information Field dark matter model to dwarf irregular galaxies and analyze its performance.

March 4, 2026Open Access

Information Field Dark Matter III: Extreme Low-Mass Test on LITTLE THINGS Dwarf Galaxies

Key Points

The aim is to extend the Information Field dark matter model to dwarf irregular galaxies and analyze its performance.
Applied the Information Field framework to dwarf irregular galaxies from the LITTLE THINGS survey.
Measured metrics include Mean Absolute Error (MAE) and R² values to evaluate model performance.
Analyzed the effects of velocity limits on model accuracy and interpretation of quantum behaviors.
Achieved MAE of approximately 36.8% and R² of about 0.68, outperforming alternative models like emergent gravity.
Observed degradation of performance at velocities below 20 km/s, revealing critical quantum effects.
Probed deeper aspects of dark matter, suggesting it may represent the Cosmic Archive, which relates to spacetime's information.

Abstract

We extend the Information Field (IF) dark-matter framework to dwarf irregular galaxies from the LITTLE THINGS survey. IF achieves MAE ≈36. 8% and R² ≈0. 68 on dwarfs, outperforming Verlinde emergent gravity while remaining competitive with MOND. Degradation occurs only at vflat < 20 km/s, interpreted as the first observational signature of the IF quantum regime: qubit grid discretization, BEC coherence limits, and deep-MOND non-linearity of the information potential Uᵢnfo. Dwarfs do not falsify IF but probe its deepest layer, recasting dark matter as the Cosmic Archive—spacetime's informational substrate decoded via holographic entropy. This is Part III of the Information Field Dark Matter series. Part I (FhiemDien, 2026): https: //doi. org/10. 5281/zenodo. 18779541Part II (FhiemDien, 2026): https: //doi. org/10. 5281/zenodo. 18785473

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Cite This Study

Duy Bao (Fhiemdien) Le (Mon,) studied this question.

synapsesocial.com/papers/69a7cd1dd48f933b5eed9225 https://doi.org/https://doi.org/10.5281/zenodo.18830476

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