The radial and angular Euler-Lagrange equations areWriting the conserved angular momentum aswe obtainA positive constant radius requires zero radial acceleration. Hence the circular motion hasprovided and . Its angular velocity is . No positive circular radius exists for with .
For later use, the conserved radial energy isThe effective potential has , so its stationary radius is a stable minimum. The tension remains positive in the ideal allowed region: the hanging Newton's second law gives .
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