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| Format: | Recurso digital |
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Zenodo
2026
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| Online Access: | https://doi.org/10.5281/zenodo.18214550 |
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Table of Contents:
- <p>This work investigates a density-screened modification of gravity characterized by a universal power-law contribution with exponent n \approx 1.8. Across a wide range of astrophysical systems, from dwarf and low-surface-brightness galaxies to massive galaxy clusters, this value consistently reproduces observed kinematics without system-dependent retuning. The framework explores an alternative phenomenological approach in which a universal power-law gravitational contribution operates in low-density environments and becomes suppressed in high-density regions." </p>