Verlinde–Bose–Einstein Emergent Gravity: Supplementary Code and Data

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Main Author: Morris, Christian W.
Format: Recurso digital
Language:English
Published: Zenodo 2026
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author Morris, Christian W.
author_facet Morris, Christian W.
contents <div>Supplementary analysis code and figures for a three-paper series on emergent gravity without dark matter. The codebase accompanies: (1) Morris (2026), "The Radial Acceleration Relation as a Bose-Einstein Identity in Verlinde's Emergent Gravity" — galactic rotation curve analysis using SPARC data; (2) Morris (2026), "Galaxy Cluster Radial Acceleration Relation from Verlinde-Bose-Einstein Framework with NFW Potential Ratio Geometric Correction" — extension to cluster scales; (3) Morris (2026), "Cosmological Constraints on the Verlinde-Bose-Einstein Framework: Structure Formation, CMB, and the Hybrid Interpretation" — cosmological tests including structure formation, CMB acoustic scale, pre-recombination strain dynamics, Bullet Cluster analysis, and a hybrid model reducing required dark matter by 47%. All scripts are self-contained Python 3 with NumPy/SciPy/Matplotlib dependencies.</div> <div><br><br> <div> <div>Requirements</div> <br> <div>- Python 3.8+</div> <div>- NumPy</div> <div>- Matplotlib</div> <div>- SPARC rotation curve data (Lelli, McGaugh & Schombert 2017; available at https://astroweb.case.edu/SPARC/)<br><br><br> <div> <div>Relationship: is a supplement to https://doi.org/10.5281/zenodo.18881878</div> </div> </div> </div> </div>
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language eng
publishDate 2026
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record_format zenodo
spellingShingle Verlinde–Bose–Einstein Emergent Gravity: Supplementary Code and Data
Morris, Christian W.
modified gravity
emergent gravity
MOND
radial acceleration relation
Bose-Einstein statistics
horizon thermodynamics
SPARC
galaxy rotation curves
dark matter
Verlinde gravity
galaxy clusters
cosmology
CMB
structure formation
Bullet Cluster
Python
<div>Supplementary analysis code and figures for a three-paper series on emergent gravity without dark matter. The codebase accompanies: (1) Morris (2026), "The Radial Acceleration Relation as a Bose-Einstein Identity in Verlinde's Emergent Gravity" — galactic rotation curve analysis using SPARC data; (2) Morris (2026), "Galaxy Cluster Radial Acceleration Relation from Verlinde-Bose-Einstein Framework with NFW Potential Ratio Geometric Correction" — extension to cluster scales; (3) Morris (2026), "Cosmological Constraints on the Verlinde-Bose-Einstein Framework: Structure Formation, CMB, and the Hybrid Interpretation" — cosmological tests including structure formation, CMB acoustic scale, pre-recombination strain dynamics, Bullet Cluster analysis, and a hybrid model reducing required dark matter by 47%. All scripts are self-contained Python 3 with NumPy/SciPy/Matplotlib dependencies.</div> <div><br><br> <div> <div>Requirements</div> <br> <div>- Python 3.8+</div> <div>- NumPy</div> <div>- Matplotlib</div> <div>- SPARC rotation curve data (Lelli, McGaugh & Schombert 2017; available at https://astroweb.case.edu/SPARC/)<br><br><br> <div> <div>Relationship: is a supplement to https://doi.org/10.5281/zenodo.18881878</div> </div> </div> </div> </div>
title Verlinde–Bose–Einstein Emergent Gravity: Supplementary Code and Data
topic modified gravity
emergent gravity
MOND
radial acceleration relation
Bose-Einstein statistics
horizon thermodynamics
SPARC
galaxy rotation curves
dark matter
Verlinde gravity
galaxy clusters
cosmology
CMB
structure formation
Bullet Cluster
Python
url https://doi.org/10.5281/zenodo.18881795