5. Discussion
The proposed theoretical framework presents several key distinctions from existing approaches, particularly from Modified Newtonian Dynamics (MOND), while also offering deeper insights into the nature of gravity and its connection to geometry.
First, unlike MOND—whose original formulation is based on an empirical ansatz designed to fit galactic rotation curves without a rigorous theoretical foundation—our model is derived from a consistent physical and mathematical framework. MOND, in its initial form, lacks a clear derivation from fundamental principles and violates standard conservation laws such as energy and momentum in isolated systems. In contrast, the present theory provides a complete and self-consistent derivation rooted in classical gravitational dynamics within specific geometric configurations. Crucially, it unifies both Newtonian gravity and MOND-like behavior under a single formalism: in appropriate limits (e.g., spherical symmetry or point-mass approximations), it recovers standard inverse-square law behavior; in disk-like or extended planar systems with fixed height, it naturally yields a∝1/r, reproducing the core prediction of MOND without introducing ad hoc modifications to gravity or inertia.
Second, this model reveals a profound link between gravity and geometry. Specifically, it demonstrates that gravitational effects depend not only on mass and distance but also on the surface area associated with the mass distribution—particularly the effective cross-sectional or bounding surface through which field lines pass. Since surface area is inherently a geometric quantity, this suggests that gravity exhibits intrinsic geometric dependence. This finding resonates strongly with the geometric interpretation of gravity in general relativity, where gravitation arises from the curvature of spacetime. While our model operates within a classical context, the emergence of geometric sensitivity supports the broader idea that gravity is fundamentally tied to the shape and topology of matter distributions, reinforcing the notion that geometric principles may underlie gravitational phenomena across scales.
Third, the role of the gravitational constant G must be re-evaluated in light of this theory. Traditionally, G is determined experimentally in systems with approximate spherical symmetry (e.g., Cavendish-type experiments). However, our results suggest that what we measure as “G” may in fact be a shape-dependent effective parameter, denoted here as G′, whose value depends on the global geometry of the mass distribution. In other words, G′may not be a universal constant across all configurations, but rather a coefficient that varies with system morphology—constant only within certain symmetric classes (spherical, cylindrical, etc.). This implies that apparent discrepancies in gravitational measurements at different scales could partially stem from unaccounted geometric effects, rather than requiring new physics or dark components.
Finally, extending this framework to more complex systems—such as triaxial ellipsoids—reveals even richer dynamical behavior. Unlike spherical systems characterized by a single parameter (radius) or axisymmetric bodies like cylinders and disks (two parameters), ellipsoids are defined by three principal axes, all of which can vary with position in a non-uniform medium. This increased degree of freedom leads to highly anisotropic and potentially chaotic orbital dynamics, where accelerations and forces lack simple radial symmetry. Such complexity may explain the irregular velocity dispersions and non-Keplerian motions observed in elliptical galaxies and galaxy clusters, suggesting that geometric diversity alone can contribute significantly to observed gravitational anomalies.
In summary, this theory not only accounts for both Newtonian and MOND-like regimes within a unified, physically grounded framework but also highlights the critical role of geometry in shaping gravitational interactions. It challenges the universality of G as a constant and opens new avenues for interpreting gravitational phenomena through the lens of system morphology—potentially reducing the need for dark matter or modified dynamics in certain astrophysical contexts.