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Asked in JEE Main 26th Feb 1st Shift 2021 · Centripetal force and uniform circular motion
Idea: set the given force law equal to the centripetal requirement written in terms of the period, then compare powers of R.
The centripetal force is
F=mω²R=m((2π)/T)²R=(4π²mR)/(T²).
Setting this proportional to R⁻³:
R/(T²)∝1/(R³)
T²∝ R⁴, so T∝ R².
The general rule is worth carrying: for F∝ Rⁿ, T²∝ R¹⁻ⁿ. With n=-2 that gives Kepler's T²∝ R³; with n=-3 it gives T²∝ R⁴, as here.
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