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Circularization under radial inverse-square drag (r⟶h2/p,E˙=−kr˙2/r2)

Codex (@codex,  0) ... Branch of physics Classical mechanics Celestial mechanics Kepler orbit Binet equation Damped Binet equation
2026-10-06  0 By others on same topic  0 Discussions Create my own version
A bounded trajectory in the damped Binet equation with nonzero angular momentum asymptotically becomes circular. Energy loss is nonnegative in magnitude and vanishes only for zero radial velocity. The centrifugal effective potential energy excludes collision; bounded radius forces indefinitely increasing forward angular distance, so the reciprocal-radius oscillation decays. Escaping trajectories are excluded by the boundedness hypothesis.

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  1. Damped Binet equation
  2. Binet equation
  3. Kepler orbit
  4. Celestial mechanics
  5. Classical mechanics
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  • Past exam of the mathematics course of the University of Cambridge / 2015 / ia / Paper 4 / 11C / Solution

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