Work and the Work-Energy Theorem
~6 min read · Tier toggle changes depth (T1 plain · T2 standard · T3 rigour)
You should be comfortable with vector dot products, basic integration, and Newton's Second Law. Familiarity with free-body diagrams from the previous lecture is essential for identifying net forces.
Why this matters
The work-energy theorem provides a scalar shortcut to solve dynamics problems without tracking time-dependent acceleration.
In many mechanical systems, determining the final speed of an object is more relevant than knowing its exact position at every intermediate time. While Newton's Second Law requires solving differential equations involving vectors and time, the work-energy theorem relates the cumulative effect of forces directly to the change in speed. This scalar relationship is particularly powerful when forces vary with position, as it allows us to bypass the complexity of time-dependent motion analysis entirely.
The Core Idea
Imagine pushing a heavy box across a rough floor. You apply a force over a certain distance. The "effort" you expend depends not just on how hard you push, but also on how far the box moves in the direction of your push. If you push sideways while the box moves forward, you do no work on its forward motion. Work is the measure of energy transferred to an object by a force acting through a displacement. It is not a new kind of energy, but rather the mechanism by which energy is changed. If the net force on an object does positive work, the object speeds up; if it does negative work, the object slows down. This theorem connects the cause (force acting over distance) to the effect (change in kinetic energy) in a single, elegant equation.
Defining Work
Work is defined as the dot product of the force vector and the displacement vector. For a constant force \(\vec{F}\) acting over a straight-line displacement \(\Delta \vec{r}\), the work \(W\) is given by:
where \(\theta\) is the angle between the force and the displacement. The unit of work is the joule (\(\mathrm{J}\)), equivalent to one newton-metre (\(\mathrm{N \cdot m}\)). Note that work is a scalar quantity; it has magnitude but no direction. If the force is perpendicular to the motion (\(\theta = 90^\circ\)), the work done is zero. This explains why the normal force from a horizontal table does no work on a sliding block, as the force is vertical while the displacement is horizontal.
For a variable force \(\vec{F}(\vec{r})\) acting along a curved path from point \(A\) to point \(B\), we must sum the infinitesimal work done along each small segment \(d\vec{r}\). This leads to the line integral definition:
This integral depends on the path taken if the force is non-conservative, such as friction. For the net force acting along the path the particle actually follows, however, the result is always the change in kinetic energy, as the theorem below shows.
The Work-Energy Theorem
The Work-Energy Theorem states that the net work done on a particle by all forces acting on it equals the change in its kinetic energy. This result is derived directly from Newton's Second Law and the definition of kinetic energy. The theorem is valid for any net force, whether constant or variable, and for any trajectory.
Here, \(K = \frac{1}{2}mv^2\) is the kinetic energy. The theorem implies that if the net work is zero, the speed of the object remains constant, even if its direction changes (as in uniform circular motion, where the centripetal force does no work). Conversely, if the net work is positive, the kinetic energy increases; if negative, it decreases. This scalar equation is often easier to solve than the vector equations of motion, especially when time is not a variable of interest.
Applying the Theorem
To apply the work-energy theorem, follow these steps: First, identify the initial and final states of the system. Second, draw a free-body diagram to identify all forces acting on the object. Third, determine the work done by each force. Forces that are perpendicular to the displacement do zero work. Fourth, sum the work done by all forces to find the net work. Finally, equate the net work to the change in kinetic energy and solve for the unknown quantity, usually the final speed.
Consider a block sliding down a frictionless incline. The forces are gravity and the normal force. The normal force is perpendicular to the displacement, so it does no work. Gravity does positive work. The net work is equal to the work done by gravity. By equating this to the change in kinetic energy, we can find the speed at the bottom of the incline without needing to know the time taken or the acceleration directly. This method is robust and avoids the complexities of vector decomposition in non-Cartesian coordinates.
The derivation
The Work-Energy Theorem
For a particle of constant mass \(m\) moving under a net force \(\vec{F}\), the work done by that net force as the particle travels from point \(A\) to point \(B\) along its actual trajectory equals the change in its kinetic energy: \(\displaystyle \int_{A}^{B}\vec{F}\cdot d\vec{r} = \tfrac{1}{2}mv_B^{2}-\tfrac{1}{2}mv_A^{2}\), where \(K=\tfrac12 mv^2\) and \(v=|\vec v|\) is the speed.
A common misconception is that work is a property of the object itself. In reality, work is a process quantity associated with the interaction between a force and a displacement. An object can have kinetic energy, but it does not "have" work. Work is the transfer of energy. Furthermore, the work done by a force depends on the reference frame. For example, in a moving train, a passenger pushing a box does work relative to the train, but the work done by the same force relative to the ground may be different because the displacement is different. Always specify the reference frame when calculating work. C
Worked example
Problem. A \(10\ \mathrm{kg}\) block is pushed from rest across a horizontal surface by a constant horizontal force of \(50\ \mathrm{N}\). The coefficient of kinetic friction between the block and the surface is \(0.2\). Calculate the speed of the block after it has moved \(4\ \mathrm{m}\). Take \(g = 9.8\ \mathrm{m/s^2}\).
- Identify the forces: Applied force \(F_{\text{app}} = 50\ \mathrm{N}\), Friction \(f_k = \mu_k N\), Normal force \(N\), Gravity \(mg\).
- Calculate the normal force: Since the surface is horizontal and there is no vertical acceleration, \(N = mg = 10 \times 9.8 = 98\ \mathrm{N}\).
- Calculate the friction force: \(f_k = 0.2 \times 98 = 19.6\ \mathrm{N}\).
- Determine the net force: \(F_{\text{net}} = F_{\text{app}} - f_k = 50 - 19.6 = 30.4\ \mathrm{N}\).
- Calculate the net work: \(W_{\text{net}} = F_{\text{net}} \times d = 30.4 \times 4 = 121.6\ \mathrm{J}\).
- Apply the work-energy theorem: \(W_{\text{net}} = \Delta K = \frac{1}{2}mv_f^2 - \frac{1}{2}mv_i^2\). Since \(v_i = 0\), \(121.6 = \frac{1}{2} \times 10 \times v_f^2\).
- Solve for \(v_f\): \(v_f^2 = \frac{2 \times 121.6}{10} = 24.32\), so \(v_f = \sqrt{24.32} \approx 4.93\ \mathrm{m/s}\).
Units check. Work is in joules (\(\mathrm{kg \cdot m^2/s^2}\)). Kinetic energy is \(\frac{1}{2}mv^2\), which is \(\mathrm{kg \cdot (m/s)^2} = \mathrm{kg \cdot m^2/s^2}\). The units are consistent.
Three quick tests
- Does the normal force do work on an object sliding down a frictionless incline?
Answer
No, because the normal force is perpendicular to the displacement, so \(\cos(90^\circ) = 0\). - If the net work done on an object is zero, what can you say about its speed?
Answer
The speed remains constant, although the direction of velocity may change. - How does the work-energy theorem simplify the analysis of motion compared to Newton's Second Law?
Answer
It converts a vector differential equation problem into a scalar algebraic equation, eliminating the need to solve for time-dependent acceleration.
Problem set for PU-101 →
Each derivation in this unit ends with five graded problems with full solutions.
Lecture notes drafted with a local model and checked line by line by the editor; every number in the worked example was recomputed.