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The Timpson Lyceum · University Physics I (2025)

Dynamics of Rotational Motion: Torque and Angular Momentum – Lecture 10 (University Physics I)

Overview

This lecture builds the dynamics of rotation by carrying every linear idea over to its rotational analogue. Force becomes torque, mass becomes moment of inertia, and Newton's second law F=maF = ma becomes τ=Iα\tau = I\alpha. From there we build the kinetic energy of a body that both moves and spins, prove a rotational work–energy theorem, and introduce angular momentum L⃗=r⃗×p⃗\vec L = \vec r \times \vec p along with its conservation. These tools explain everyday phenomena — why a door knob sits far from the hinge, why a solid sphere wins a race down a ramp, and why a skater spins faster when pulling their arms in. Mastering the linear-to-rotational dictionary is the key to the whole chapter, so you carry intuition instead of memorizing a pile of new formulas.

Key Concepts

The linear → rotational dictionary

Torque — the rotational cause of angular acceleration.

Rotational form of Newton's second law

Kinetic energy of a rigid body (translation + rotation)

Rolling without slipping

Rotational work, power, and the work–energy theorem

Angular momentum

Conservation of angular momentum

Worked Example

A solid sphere rolling down a ramp. A solid sphere (I=25MR2I = \tfrac25 MR^2) is released on an incline of angle β\beta and rolls without slipping. Find the acceleration of its center of mass.

Forces along the incline (down-slope positive), with fsf_s the static friction: Macm=Mgsin⁡β−fsMa_{\text{cm}} = Mg\sin\beta - f_s

Torque about the center (only friction provides it), using τ=Iα\tau = I\alpha and the rolling condition α=acm/R\alpha = a_{\text{cm}}/R: fsR=Iα=25MR2⋅acmR  ⇒  fs=25Macmf_s R = I\alpha = \tfrac25 MR^2\cdot\frac{a_{\text{cm}}}{R} \;\Rightarrow\; f_s = \tfrac25 M a_{\text{cm}}

Substitute fsf_s into the force equation and solve:

Macm=Mgsin⁡β−25Macm75Macm=Mgsin⁡βacm=57 gsin⁡β\begin{aligned} Ma_{\text{cm}} &= Mg\sin\beta - \tfrac25 M a_{\text{cm}} \\ \tfrac{7}{5} M a_{\text{cm}} &= Mg\sin\beta \\ a_{\text{cm}} &= \tfrac{5}{7}\,g\sin\beta \end{aligned}

The friction needed to sustain rolling then follows:

fs=25Macm=25M(57gsin⁡β)fs=27 Mgsin⁡β\begin{aligned} f_s &= \tfrac25 M a_{\text{cm}} = \tfrac25 M\left(\tfrac57 g\sin\beta\right) \\ f_s &= \tfrac27\,Mg\sin\beta \end{aligned}

Notice the acceleration is only 57\tfrac57 of the frictionless sliding value gsin⁡βg\sin\beta, and it depends on neither MM nor RR — only on the geometry through the 25\tfrac25 coefficient.

Short companion — conservation of angular momentum. A spinning person holds two 5 kg5\ \text{kg} dumbbells. With arms out (I1=13 kg⋅m2I_1 = 13\ \text{kg}\cdot\text{m}^2) the spin rate is ω1=π rad/s\omega_1 = \pi\ \text{rad/s} (one turn per 2 s2\ \text{s}). Arms pulled in give I2=2.6 kg⋅m2I_2 = 2.6\ \text{kg}\cdot\text{m}^2:

ω2=I1I2 ω1ω2=132.6 π=5π rad/s\begin{aligned} \omega_2 &= \frac{I_1}{I_2}\,\omega_1 \\ \omega_2 &= \frac{13}{2.6}\,\pi = 5\pi\ \text{rad/s} \end{aligned}

The spin rate quintuples — and the rotational KE rises fivefold, supplied by the work done pulling the masses inward.

Summary