Discover how exponential screening alters classical orbits, breaking symmetry to drive precessing rosettes and unstable potential cliff collapse.
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Discover how exponential screening in attractive Yukawa fields breaks elliptical symmetry, driving non-closing precessing rosette orbits and rapid dissipative spiral capture into central targets.

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Precession and Orbital Collapse in Screened Potentials
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}}%%
graph LR
subgraph Current_Exploration["Current Exploration (R21: Non-Inverse-Square Dynamics)"]
A(Bound Rosette Orbits):::current
B(Unstable Potential Cliff):::current
C(Dissipative Spiral Capture):::current
D(Repulsive Short-Range Scattering):::current
end
subgraph Potential_Orientation["Potential Orientation (Extensions & Formalisms)"]
E(Analytic Perturbation Theory: Δϕ):::potential
F(Analytical Critical Momentum: Lc):::potential
G(Quantum Wave-Packet Tunneling):::potential
H(Core-Repulsive Generalized Potentials):::potential
end
%% Theoretical Mappings
A -- "Derive closed-form formula for periastron shift" --> E
B -- "Solve dVeff/dr=0 for bifurcation boundary" --> F
C -- "Transition from dissipation to quantum TDSE" --> G
D -- "Extend to models with r⁻¹² repulsive cores" --> H
%% Styling Definitions
classDef current fill:#0277bd,stroke:#01579b,color:#ffffff,stroke-width:2px;
classDef potential fill:#2e7d32,stroke:#1b5e20,color:#ffffff,stroke-width:2px;
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style Potential_Orientation fill:#e8f5e9,stroke:#a5d6a7,stroke-width:2px,color:#1b5e20;
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