Torque, Angular Momentum & Rotational Dynamics Explained | Chapter 10 of University Physics
Torque, Angular Momentum & Rotational Dynamics Explained | Chapter 10 of University Physics
Chapter 10 of University Physics develops the rotational analogs of Newton’s laws by introducing torque, rotational dynamics, and angular momentum. We explore Στ=Iα, combined translational and rotational motion, work and power in rotation, conservation of angular momentum, and gyroscopic precession.

Torque: The Rotational Force
Torque (τ) measures a force’s ability to cause rotation about an axis. Defined as τ = r × F = r F sin(φ), torque uses the lever arm (perpendicular distance) and the right-hand rule to determine its direction. The SI unit is the newton-meter (N·m).
Rotational Form of Newton’s Second Law
For a rigid body about a fixed axis, the net torque equals rotational inertia times angular acceleration:
Στ = I α
This equation parallels F = m a in linear dynamics. Solving problems involves drawing free-body diagrams, choosing rotation axes, writing ΣF = m a and Στ = I α, and solving component equations.
Combined Translation & Rotation
The total kinetic energy of a rigid body combines translation of its center of mass and rotation about that point:
Ktotal = ½ M vcm² + ½ Icm ω²
In rolling without slipping, the no-slip condition vcm = R ω links linear and angular velocities.
Work & Power in Rotational Motion
Analogous to linear work, torque does work through angular displacement:
- W = τ Δθ
- P = τ ω
The rotational work-energy theorem states that the work done by torque equals the change in rotational kinetic energy: W = Δ(½ I ω²).
Angular Momentum & Its Conservation
Angular momentum (L) for a rigid body is L = I ω; for a particle, L = r × p. When net external torque is zero, angular momentum is conserved (dL/dt = 0), making it invaluable for analyzing isolated systems and collisions in rotational contexts.
Gyroscopes & Precession
Gyroscopic precession occurs when an applied torque changes the direction of L without altering its magnitude. The precession rate is given by:
Ω = τ / L = (m g r) / (I ω)
This phenomenon underpins applications in navigation and stabilization.
Conclusion
By mastering torque, Στ=Iα, and angular momentum conservation, you gain powerful methods to analyze rotating systems — from spinning wheels to gyroscopes. Energy and work in rotation complement these tools for comprehensive problem solving.
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