Torque and angular momentum

Push on a door far from its hinge and it swings easily; push at the same spot near the hinge and almost nothing happens. The difference is not the force but its turning effect — what physics calls torque. Torque is the rotational twin of force, and it has its own conserved partner: angular momentum, the rotational twin of linear momentum. Together they answer a question ordinary force and momentum cannot: how does a spinning or rotating object's motion change over time, and why does a figure skater spin faster when she pulls her arms in? This article builds torque and angular momentum from the definitions you already know for linear motion — position, force, momentum — using nothing but the vector cross product, then shows that they are linked by an equation with exactly the same shape as Newton's second law.

The core insight

Torque τ⃗=r⃗×F⃗\vec\tau=\vec r\times\vec F is the turning effect of a force, angular momentum L⃗=r⃗×p⃗\vec L=\vec r\times\vec p is the rotational analogue of momentum, and the two are tied together by dL⃗/dt=τ⃗d\vec L/dt=\vec\tau, the rotational twin of dp⃗/dt=F⃗d\vec p/dt=\vec F.

The core idea

Torque is a cross product, not a plain product. If a force F⃗\vec F acts at a point whose position vector relative to a chosen pivot is r⃗\vec r, only the component of F⃗\vec F perpendicular to r⃗\vec r actually twists the object — a push straight along r⃗\vec r (toward or away from the pivot) produces no rotation at all. The cross product automatically keeps only that perpendicular part:

τ⃗=r⃗×F⃗,∣τ⃗∣=rFsin⁡θ\vec\tau = \vec r \times \vec F, \qquad |\vec\tau| = rF\sin\theta

where: rr is the distance from the pivot to the point of application, FF is the magnitude of the force, and θ\theta is the angle between r⃗\vec r and F⃗\vec F. The SI unit is N m\text{N m} — numerically identical to the joule, but torque is never quoted in joules because it is a vector describing a turning effect, not a scalar energy.

Angular momentum is the rotational twin of momentum. For a particle of mass mm moving with velocity v⃗\vec v (so momentum p⃗=mv⃗\vec p = m\vec v) at position r⃗\vec r from a chosen origin, its angular momentum about that origin is

L⃗=r⃗×p⃗\vec L = \vec r \times \vec p

where: r⃗\vec r locates the particle, p⃗\vec p is its linear momentum, and L⃗\vec L points along the axis about which the particle appears to circulate, given by the right-hand rule. Like torque, L⃗\vec L depends on where the origin is chosen — the same particle has different angular momentum about different points.

For a rigid body spinning about a fixed axis, every particle's individual L⃗\vec L adds up into two clean scalar relations that mirror F=maF=ma and p=mvp=mv exactly, with mass mm replaced by moment of inertia II:

τ=IαandL=Iω\tau = I\alpha \qquad\text{and}\qquad L = I\omega

where: II is the moment of inertia about the axis, α\alpha is angular acceleration, and ω\omega is angular velocity. The pattern is worth memorising as a translation table: every time you see mm in a linear equation, write II instead, and swap s→θs\to\theta, v→ωv\to\omega, a→αa\to\alpha, F→τF\to\tau, p→Lp\to L.

Figure
A wrench turning a bolt with the force arrow perpendicular to the wrench and the torque vector pointing along the bolt axis by the right hand rule
Torque = r × F, direction by the right-hand rule pivot (bolt) wrench, length r force F, perpendicular to wrench rotation sense torque vector τ, along bolt axis

Torque produces changing angular momentum

The goal of this derivation is to show, using only the product rule for differentiation, that the net external torque on a particle equals the rate at which its angular momentum changes — a genuine derivation, not a stated analogy, and the single equation from which τ=Iα\tau=I\alpha and every conservation-of-angular-momentum result later in the syllabus ultimately follows.

Step 1. Start from the definition L⃗=r⃗×p⃗\vec L=\vec r\times\vec p and differentiate both sides with respect to time, treating the cross product like an ordinary product so the product rule applies to each factor in turn:

dL⃗dt=dr⃗dt×p⃗+r⃗×dp⃗dt\frac{d\vec L}{dt} = \frac{d\vec r}{dt}\times\vec p + \vec r\times\frac{d\vec p}{dt}

Step 2. Evaluate the first term. Since dr⃗dt=v⃗\dfrac{d\vec r}{dt}=\vec v and p⃗=mv⃗\vec p=m\vec v, the first term is v⃗×mv⃗=m(v⃗×v⃗)\vec v\times m\vec v = m(\vec v\times\vec v). The cross product of any vector with itself is zero, because sin⁡θ=sin⁡0∘=0\sin\theta=\sin 0^\circ=0 for parallel vectors, so this whole term vanishes.

Step 3. Evaluate the second term using Newton's second law, dp⃗dt=F⃗\dfrac{d\vec p}{dt}=\vec F. The second term becomes r⃗×F⃗\vec r\times\vec F, which is exactly the definition of torque about the same origin.

Step 4. Combine the two results. The first term is zero and the second term is τ⃗\vec\tau, so

dL⃗dt=τ⃗\frac{d\vec L}{dt} = \vec\tau

Net torque about a point equals the rate of change of angular momentum about that same point — the exact rotational mirror of F⃗=dp⃗/dt\vec F=d\vec p/dt, obtained here by direct differentiation rather than by analogy alone.

Worked example

A force of 15 N15\ \text{N} is applied perpendicular to a wrench of length 0.3 m0.3\ \text{m} to tighten a bolt whose fitting has moment of inertia 0.05 kg m20.05\ \text{kg m}^2 about the bolt's axis and is otherwise free to rotate. Find (a) the torque, (b) the angular acceleration produced, and (c) the angular momentum gained after it has turned for 0.2 s0.2\ \text{s} starting from rest.

Step 1. Torque. The force is perpendicular to the wrench, so θ=90°\theta=90° and sin⁡θ=1\sin\theta=1:

τ=rFsin⁡θ=(0.3)(15)(1)=4.5 N m\tau = rF\sin\theta = (0.3)(15)(1) = 4.5\ \text{N m}

Step 2. Angular acceleration, from τ=Iα\tau=I\alpha:

α=τI=4.50.05=90 rad/s2\alpha = \frac{\tau}{I} = \frac{4.5}{0.05} = 90\ \text{rad/s}^2

Step 3. Angular velocity after 0.2 s0.2\ \text{s} from rest, using the rotational analogue of v=u+atv=u+at:

ω=ω0+αt=0+(90)(0.2)=18 rad/s\omega = \omega_0 + \alpha t = 0 + (90)(0.2) = 18\ \text{rad/s}

Step 4. Angular momentum gained, from L=IωL=I\omega:

L=Iω=(0.05)(18)=0.9 kg m2/sL = I\omega = (0.05)(18) = 0.9\ \text{kg m}^2/\text{s}

This matches L=τt=4.5×0.2=0.9 kg m2/sL=\tau t = 4.5\times0.2=0.9\ \text{kg m}^2/\text{s}, since dL⃗/dt=τ⃗d\vec L/dt=\vec\tau means a constant torque produces angular momentum at a steady rate. The torque is 4.5 N m4.5\ \text{N m}, the angular acceleration is 90 rad/s290\ \text{rad/s}^2, and after 0.2 s0.2\ \text{s} the fitting has gained 0.9 kg m2/s0.9\ \text{kg m}^2/\text{s} of angular momentum.

Common traps

  • Writing τ=rF\tau=rF without the sin⁡θ\sin\theta factor when the force is not perpendicular to r⃗\vec r — only the component of force perpendicular to the position vector (or equivalently the perpendicular "moment arm" distance) produces torque.
  • Forgetting that both torque and angular momentum are defined relative to a chosen origin or pivot — the same force or the same moving particle gives different values of τ⃗\vec\tau or L⃗\vec L about different points, so the origin must always be stated.
  • Confusing the torque unit N m\text{N m} with the energy unit J\text{J} just because they are numerically the same — torque is a vector turning effect, never added to or substituted for work or energy.
  • Applying L=IωL=I\omega to a particle that is not in rigid-body rotation or simple circular motion about the axis — for general motion, angular momentum must be computed from the vector definition L⃗=r⃗×p⃗\vec L=\vec r\times\vec p directly.

Ask the tutor: want to see how dL⃗/dt=τ⃗=0d\vec L/dt=\vec\tau=0 leads straight into the conservation of angular momentum you meet in the next topic, or work through the right-hand-rule direction of torque with a few more examples?

Why does torque use a cross product instead of just multiplying force and distance?

Because only the part of the force perpendicular to the position vector actually turns the object — a force pointing straight along the arm toward or away from the pivot cannot start or change rotation, no matter how large it is. The cross product r⃗×F⃗\vec r\times\vec F automatically extracts exactly that perpendicular contribution through the sin⁡θ\sin\theta factor, and it also encodes the direction of the torque (the axis about which the twist acts) via the right-hand rule, which a plain scalar product rFrF could never do.

How is dL/dt = τ actually a proof, when Pass 1 only stated it as an analogy?

Differentiating L⃗=r⃗×p⃗\vec L=\vec r\times\vec p with the product rule gives two terms: v⃗×p⃗\vec v\times\vec p and r⃗×dp⃗/dt\vec r\times d\vec p/dt. The first term is always zero because v⃗\vec v and p⃗=mv⃗\vec p=m\vec v point the same way, and any vector crossed with itself (or a parallel vector) is zero. The second term is r⃗×F⃗\vec r\times\vec F by Newton's second law, which is exactly the torque. So dL⃗/dt=τ⃗d\vec L/dt=\vec\tau follows directly from the definitions of L⃗\vec L and F⃗\vec F — it is not merely an analogy borrowed from linear motion, it is a genuine consequence of it.

Is L = Iω always true for a rotating body, or only sometimes?

It holds for a rigid body rotating about a fixed axis, or for a single particle moving in a circle about the axis (where I=mr2I=mr^2), because in both cases every bit of mass moves perpendicular to its own position vector, so the cross product reduces cleanly to the scalar form. For a particle moving in some other path, or a body rotating about a changing axis, you cannot assume L=IωL=I\omega — go back to the vector definition L⃗=r⃗×p⃗\vec L=\vec r\times\vec p and compute it directly.

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Where this leads