Coulomb's Law & the Electric Field
Forces between point charges and the field that surrounds them
Stick a balloon to the wall after rubbing it on your hair and you have already demonstrated Coulomb's law — an inverse-square force between electric charges that was measured with a torsion balance in 1785 and still underpins every antenna, capacitor, and transistor you will study.
Coulomb's Law
In 1785 Charles-Augustin de Coulomb used a sensitive torsion balance to measure the force between two charged spheres. His finding, now called Coulomb's law, states that the electrostatic force between two point charges is directly proportional to the product of the charge magnitudes and inversely proportional to the square of the distance between them. The force acts along the straight line joining the two charges.
For two point charges Q₁ and Q₂ separated by a distance r, the magnitude of the force is:
Direction and Sign
The constant k is Coulomb's constant, with value k = 8.99×10⁹ N·m²/C². The absolute value in the formula gives the magnitude; the direction is determined by the signs of the charges. When both charges have the same sign, the force is repulsive. When the charges have opposite signs, the force is attractive.
It is worth pausing to appreciate the structure of this law. The 1/r² dependence is the same mathematical form as Newton's law of gravitation, but the electrostatic force is enormously stronger. The gravitational attraction between two protons is roughly 10³⁶ times weaker than their electrostatic repulsion. The reason gravity dominates at cosmic scales is simply that matter is almost perfectly electrically neutral, while mass has no negative counterpart.
The full vector form of Coulomb's law is F12 = k Q₁Q₂/r² r̂12, where r̂12 is the unit vector pointing from Q₁ to Q₂. The sign of Q₁Q₂ handles direction automatically: a positive product gives a force along r̂12 (repulsion), while a negative product reverses it (attraction).
The Superposition Principle
When more than two charges are present, the net force on any one charge is the vector sum of the individual forces exerted by each of the other charges. Superposition is a vector addition — you must resolve each force into components, sum the components separately, and then recombine.
Superposition also tells us that the presence of a third charge does not alter the force that the first charge exerts on the second. Each pair-wise interaction is independent. This linearity is the foundation for the integral approach we will use with continuous charge distributions in the next lesson.
- Identify the given values: Q₁ = +3×10⁻⁶ C, Q₂ = −2×10⁻⁶ C, r = 0.5 m.
- Use Coulomb's law for the magnitude: F = k|Q₁Q₂|/r².
- Compute the product of magnitudes: |Q₁Q₂| = (3×10⁻⁶)(2×10⁻⁶) = 6×10⁻¹² C².
- Multiply by k: k|Q₁Q₂| = (8.99×10⁹)(6×10⁻¹²) = 0.05394 N·m².
- Divide by r²: F = 0.05394 / (0.5)² = 0.05394 / 0.25 = 0.2158 N.
- Since the charges have opposite signs, the force is attractive.
From Force to Field
Coulomb's law tells us the force between two charges, but it is often more useful to describe the influence of a single source charge on its surroundings. To do this, we introduce a small positive test charge q at the point of interest and measure the force F on it. The electric field E is defined as the force per unit charge:
Electric Field of a Point Charge
Substituting Coulomb's law into the field definition gives the electric field of a point charge Q at a distance r:
Interpreting the Field
The field points radially outward from a positive charge and radially inward toward a negative charge. Notice that E depends only on the source charge Q and the distance r — the test charge q has been divided out. The electric field is a property of the source charge and the point in space, not of whatever probe we use to measure it.
This is a conceptual shift worth emphasizing. In the Coulomb picture, charges reach across empty space and grab each other. In the field picture, a charge creates a field in the space around it, and that field exerts a force on any other charge placed in it. The unit of electric field is newtons per coulomb (N/C), equivalent to volts per meter (V/m).
The test charge q must be small enough that its own field does not disturb the source charge distribution whose field we are measuring. In practice, this means taking the limit as q approaches zero: E = lim(q→0) F/q.
- Use the point-charge field formula: E = kQ/r².
- Substitute: E = (8.99×10⁹)(5×10⁻⁶) / (2)².
- Compute the numerator: (8.99×10⁹)(5×10⁻⁶) = 44950.
- Divide by r² = 4: E = 44950 / 4 = 11237.5 N/C, rounded to 11238 N/C.
Check your understanding
- Coulomb's law gives the electrostatic force between two point charges: F = k|Q₁Q₂|/r², where k = 8.99×10⁹ N·m²/C².
- Like charges repel; opposite charges attract. The force always acts along the line joining the two charges.
- The superposition principle states that the net force on a charge is the vector sum of the individual forces from all other charges.
- The electric field E = F/q is the force per unit charge a small positive test charge would feel; for a point charge, E = kQ/r².