Work & Kinetic Energy
Source lecture(s): SC133 Lec 8
Intuition
Newton's laws track forces instant by instant. Energy methods take a shortcut: instead of following the whole trajectory, compare before and after. Work is the currency — force succeeding at pushing something through a distance — and kinetic energy is the account balance of motion. The exchange rate is exact: net work in, kinetic energy up, joule for joule.
Definitions
Work by a constant force \(\vec F\) over displacement \(\vec d\):
Only the force component along the motion counts (dot product). Perpendicular forces (the normal force on a sliding block, tension in a circular swing) do zero work. For varying forces:
Kinetic energy:
Power — rate of doing work:
The work–energy theorem
Derivation (1-D, from Newton II): \(W = \int F\,dx = \int m\frac{dv}{dt}dx = \int m\frac{dv}{dt}v\,dt = \int mv\,dv = \tfrac12 mv_f^2 - \tfrac12 mv_i^2\). ∎ (Full version on the equation page.)
The theorem is Newton's second law integrated over distance — no new physics, but a scalar equation that skips all the trajectory details.
Worked example: braking distance
A car at speed \(v\) locks its brakes; kinetic friction \(\mu_k mg\) acts over distance \(d\). The theorem: \(-\mu_k mg\,d = 0 - \tfrac12 mv^2\), so
Mass cancels; distance grows with the square of speed. Doubling your speed quadruples the skid — the single most life-relevant equation in this course.
Signs of work
| Situation | Sign of \(W\) | Effect on \(K\) |
|---|---|---|
| Force along motion (engine) | + | speeds up |
| Force against motion (friction, braking) | − | slows down |
| Force ⊥ motion (normal, centripetal) | 0 | speed unchanged (direction may change!) |
The zero-work case explains why magnetic forces never change a particle's speed.
Common mistakes
- "I pushed hard, so I did work." Pushing a wall does zero work — no displacement. Holding a suitcase stationary: zero work (tiring ≠ work).
- Forgetting work is signed. Friction does negative work; the theorem needs the net, signed total.
- Confusing power with energy. A 1000 W kettle running for one hour uses energy \(= P t = 3.6\) MJ; watts measure the rate.
- Using \(W = Fd\) with the total force in circular motion — the centripetal force does no work at all.
Related concepts
- Potential energy — work stored for later
- Conservation of energy — the full budget
- Work–energy theorem (equation page)
- Vectors — the dot product
Knowledge graph position
Prerequisites: Newton's laws, Vectors. Leads to: Potential energy → Conservation of energy.
Quiz
Q1 (computational). A 2 kg block accelerates from 3 m/s to 7 m/s. Net work done?
Answer
\(W = \Delta K = \tfrac12(2)(49 - 9) = 40\,\text{J}\) — regardless of how the force varied along the way.
Q2 (conceptual). A satellite in circular orbit: how much work does gravity do per revolution?
Answer
Zero. Gravity is exactly centripetal (⊥ velocity) at every instant, so \(\vec F\cdot d\vec s = 0\) throughout — consistent with constant orbital speed.
Q3 (computational). What steady power must a 1200 kg car deliver to climb a 5% grade at 20 m/s (ignore drag)?
Answer
Force along slope \(\approx mg\times 0.05 = 588\,\text{N}\); \(P = Fv = 588\times20 \approx 11.8\,\text{kW}\) (≈16 hp) — hills, not flat cruising, are what engines are sized for.
Q4 (multiple choice). Two objects with equal momentum but different masses: which has more kinetic energy? (a) heavier (b) lighter (c) equal
Answer
(b). \(K = p^2/2m\) — at fixed \(p\), smaller mass means larger \(K\). (A bullet beats a truck at equal momentum.)