Modeling Orbital Dynamics without Mass Attraction
Binary stars, such as the PSR B1913+16 pulsar system (two neutron stars, ~1.4 \( M_\odot \) each, orbital period ~7.75 hours, semi-major axis ~2 light-seconds), exhibit apparent mutual attraction traditionally explained by gravity. In the Kinetiverse framework, this attraction is modeled as a spatial force driven by \( F = ma \), rejecting Newtonian gravity (\( F = G \frac{m_1 m_2}{R^2} \)) and Einsteinian spacetime (\( E = mc^2 \)).
The Kinetiverse uses \( F = ma \) for spatial dynamics and \( E = mc \) for temporal energy, per Essen’s critique. Tides result from orbital (Keplerian) and axial motions reducing centrifugal force, and clock motion alters photon path length, modulating force. For binary stars, mutual attraction arises from spatial forces, mass concentration, and orbital dynamics.
The Kinetiverse explains the mutual attraction of binary stars through the following mechanisms:
The force maintaining the orbit is modeled as \( F = m a_{\text{effective}} \), where \( a_{\text{effective}} = v^2 / r \) is the centripetal acceleration, driven by the stars’ orbital motion, not gravitational attraction.
Centrifugal force (\( F_{\text{cent}} = m v^2 / r \)) pushes stars outward, balanced by an inward contact force (\( F = m(1/a) \)), where \( a \propto 1/r^2 \) reflects medium resistance. For PSR B1913+16 (\( v \approx 300 \, \text{km/s} \), \( r \approx 10^9 \, \text{m} \)):
Nuclear reactions convert lighter elements to heavier ones (e.g., H to Fe), increasing core density. Heavier elements sink, increasing the moment of inertia and enhancing the inward contact force:
Orbital motion creates a differential acceleration field, stabilizing the orbit, similar to tidal effects in the tsunami model’s \( \sqrt{\frac{c}{c_0}} \) term, where \( c \) is orbital acceleration and \( c_0 = 50 \, \text{m/s}^2 \).
Clock motion alters photon path length, reducing the effective force:
where \( k_{\text{photon}} \approx 10^{-10} \).
Mass concentration reduces the moment of inertia, causing energy loss (\( \Delta E_{\text{rot}} \approx 10^{40} \, \text{J} \)) and orbital decay (~76 µs/year for PSR B1913+16):
The force scales as:
where \( k_{\text{kinetiverse}} \) mimics \( G \approx 6.674 \times 10^{-11} \, \text{m}^3 \text{kg}^{-1} \text{s}^{-2} \).
The model matches PSR B1913+16’s orbital decay (\( \dot{P}_b / P_b \approx -2 \times 10^{-6} \, \text{yr}^{-1} \)), closely aligning with general relativity’s prediction. The Kinetiverse’s success in hurricane (1.2% surge error) and tsunami models (0–3 minutes error) supports its applicability to binary stars.