Chapter 5 ยท Introduction

Chapter 5 โ€” Work, Energy and Power

Work, kinetic and potential energy, power and collisions โ€” a way of solving mechanics problems by bookkeeping instead of by tracking forces moment by moment.

A child at the top of a water slide, a cricket ball leaving the bowler's hand, a lift climbing twenty floors, two railway wagons clanging together in a shunting yard. Newton's laws (Chapter 4) can describe every one of them โ€” but only if you know every force at every instant, and the forces in a slide that twists, a bat that flexes or a coupling buffer that crushes are anything but simple. Is there a way to predict the outcome without following the motion step by step?

There is, and it is one of the most powerful ideas in all of science. When a force pushes a body through a distance it does work, and that work changes the body's kinetic energy. Some forces โ€” gravity, springs โ€” store the work done against them as potential energy and give it back later; while only they act, the total mechanical energy never changes. That single bookkeeping rule gives the speed of the child at the bottom of any frictionless slide, whatever its shape. Add the rate at which work is done โ€” power โ€” and the conservation of momentum from Chapter 4, and you can rate motors and engines and predict what happens when bodies collide, from snooker balls to neutrons in a reactor.

Scalar productโ†’Work $W=\mathbf{F}\cdot\mathbf{d}$โ†’Kinetic energyโ†’Workโ€“energy theoremโ†’Potential energyโ†’Conservation of energyโ†’Powerโ†’Collisions
๐ŸŽฏ By the end of this chapter you canโ€ฆ
  • compute and use the scalar product $\mathbf{A}\cdot\mathbf{B}=AB\cos\theta=A_xB_x+A_yB_y+A_zB_z$, including the angle between two vectors;
  • find the work done by a constant force, and by a variable force as the area under an $F$โ€“$x$ graph, with the correct sign;
  • state, prove and apply the workโ€“energy theorem $W_\text{net}=\Delta K$;
  • distinguish conservative and non-conservative forces, use $U=mgh$, $U=\tfrac12kx^2$ and $F=-\dfrac{dU}{dx}$, and solve problems with conservation of mechanical energy (including the vertical circle and energy lost to friction);
  • calculate average and instantaneous power, $P=\mathbf{F}\cdot\mathbf{v}$, efficiency and energy in kWh;
  • solve elastic and perfectly inelastic collisions in one dimension and simple two-dimensional collisions;
  • tackle Board, JEE Main, JEE Advanced and NEET-style problems on work, energy, power and collisions (with potential-energy curves and the coefficient of restitution as exam extensions).
Teaser โ€” The Three-Track Race

Three beads are released together from the same height $H$ and slide without friction to the same finishing point: one down a straight ramp, one down a curve that starts steeply, one along a track that dips below the finish and climbs back up. Before you press Play, predict: which bead arrives first, and which arrives fastest? Then change $H$ and see what stays the same.

5.0 m
straight: time, final speedโ€”
steep curveโ€”
dipping trackโ€”

Sections in this chapter

โœ… Before you start
From Chapter 4 (Laws of Motion) you need Newton's second law, free-body diagrams, friction and the conservation of momentum โ€” this chapter uses them constantly. From Chapter 3 you need vectors and their components (Section 3.1, Section 3.2) and centripetal acceleration (Section 3.4). From Chapter 2, the kinematic equations, especially $v^2=u^2+2as$ (Section 2.3), and the idea of area under a graph (Section 2.2). Units, dimensions and significant figures come from Chapter 1 (Section 1.2, Section 1.3).