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CIE 9702 Physics · A Level · Topic 18

Electric fields

Clear, syllabus-mapped CIE 9702 Physics revision notes on electric fields: explanations, worked examples and exam technique, then a free targeted practice drill.

CIE 9702 PhysicsA LevelFree revision notes
Contents: 9 sections

All five subtopics here are printed under "A Level subject content" in the 9702 syllabus, and every objective carries the tier "A Level". None of it is AS. It is examined on Paper 4. Paper 1 is the AS multiple-choice paper, and the whole 9702 bank on this site comes from Paper 1, so no practice is tagged to this topic.

Syllabus points

18.1 Electric fields and field lines

18.2 Uniform electric fields

18.3 Electric force between point charges

18.4 Electric field of a point charge

18.5 Electric potential

The parallel with gravitation, and where it breaks

Almost every equation here has a twin in topic 13. Learning them as pairs is far more efficient than learning them twice.

GravitationalElectric
Source of the fieldMass MCharge Q
Field strengthg = GM/r²E = Q/(4πε₀r²)
Force between twoF = Gm₁m₂/r²F = Q₁Q₂/(4πε₀r²)
Potentialφ = -GM/rV = Q/(4πε₀r)
Potential energyE_P = -GMm/rE_P = Qq/(4πε₀r)
Force on a test objectF = mgF = qE

Two differences, and both matter:

The constant 1/(4πε₀) is 8.99 × 10⁹ N m² C⁻², where ε₀, the permittivity of free space, is 8.85 × 10⁻¹² F m⁻¹.

Electric field strength

Electric field strength at a point is the force per unit positive charge acting on a small stationary test charge placed at that point:

E = F / q

with unit N C⁻¹, or equivalently V m⁻¹. It is a vector, and its direction is the direction of the force on a positive charge.

Rearranged, the force on a charge in a field is

F = qE

and note that a negative charge experiences a force in the opposite direction to the field.

The words positive and small are both examined. Positive, because the direction of the field is defined by convention using a positive test charge. Small, because a large test charge would disturb the very field being measured.

Field lines

Field lines show the direction of the force on a positive charge, and their spacing shows the strength.

Field lines never cross, because the field at a point has one direction.

Uniform fields between parallel plates

For two parallel plates separated by a distance d with a potential difference V between them, the field between them is uniform and

E = ΔV / Δd

Worked example. Two plates 4.0 mm apart have a potential difference of 250 V.

E = 250 / 0.0040 = 62500

so E is 6.3 × 10⁴ V m⁻¹, and it points from the positive plate towards the negative.

The force on an electron in that field:

F = 1.60 × 10⁻¹⁹ × 62500 = 1.0 × 10⁻¹⁴

so about 1.0 × 10⁻¹⁴ N, directed towards the positive plate, since the electron is negative.

Notice that the field is the same everywhere between the plates, so the force on the charge does not change as it moves across, which is the property that makes the next section work.

Charged particles moving in a uniform field

A charged particle entering a uniform field at right angles to it behaves exactly like a projectile in a gravitational field, and for the same reason: a constant force at right angles to the initial velocity.

Worked example. An electron enters midway between the plates above, travelling parallel to them at 2.0 × 10⁷ m s⁻¹. The plates are 60 mm long. How far is it deflected?

Time between the plates:

t = 0.060 / (2.0 × 10⁷) = 3.0 × 10⁻⁹

Acceleration:

a = 1.0 × 10⁻¹⁴ / (9.11 × 10⁻³¹) = 1.098 × 10¹⁶

Deflection, from s = ½at² with no initial velocity across the gap:

s = 0.5 × 1.098 × 10¹⁶ × (3.0 × 10⁻⁹)² = 0.0494

so about 4.9 cm, which is far more than the 2 mm of clearance available, so this electron in fact hits the plate. Checking an answer against the geometry like that is worth doing, because a deflection larger than the gap tells you the particle never gets through.

A particle entering along the field is simply accelerated or decelerated in a straight line, and the energy method is quicker there: the work done is qV, so

½mv² = qV

Coulomb's law

The force between two point charges in free space:

F = Q₁Q₂ / (4πε₀r²)

This is an inverse square law, exactly like Newton's law of gravitation. Doubling the separation quarters the force.

Two points about applying it:

Worked example. Two small spheres carry charges of +3.0 nC and -5.0 nC, with centres 20 mm apart.

F = 8.99 × 10⁹ × 3.0 × 10⁻⁹ × 5.0 × 10⁻⁹ / (0.020)² = 3.371 × 10⁻⁴

so the force is 3.4 × 10⁻⁴ N, and it is attractive because the charges are unlike.

Field of a point charge

Dividing Coulomb's law by the test charge gives the field strength due to a point charge Q:

E = Q / (4πε₀r²)

Worked example. Find the field strength 50 mm from a point charge of +8.0 nC.

E = 8.99 × 10⁹ × 8.0 × 10⁻⁹ / (0.050)² = 28768

so E is 2.9 × 10⁴ V m⁻¹, directed away from the charge.

Where two charges both contribute, the resultant field is the vector sum of the individual fields, so the directions must be considered and not just the magnitudes. This is the main difference from the potential calculations below.

Electric potential

Electric potential at a point is the work done per unit positive charge in bringing a small test charge from infinity to that point. It is a scalar, measured in volts, where 1 V is 1 J C⁻¹.

For the field of a point charge:

V = Q / (4πε₀r)

Because V is a scalar, potentials due to several charges are added as ordinary numbers with their signs, which is much easier than adding fields. A point midway between equal positive and negative charges has zero potential but a large field, and a point midway between two equal positive charges has zero field but a large potential. Those two situations are a favourite question precisely because they force you to keep the scalar and vector natures apart.

Worked example. Find the potential 50 mm from the +8.0 nC charge above.

V = 8.99 × 10⁹ × 8.0 × 10⁻⁹ / 0.050 = 1438.4

so V is about 1.4 × 10³ V.

Note the relationship between that answer and the field strength found earlier: 1438.4 / 0.050 = 28768, which is E. That is no coincidence, and it is the next objective.

Field as the potential gradient

The electric field at a point is the negative of the potential gradient at that point:

E = -ΔV / Δr

The minus sign says the field points from high potential to low potential, which is the direction a positive charge would be pushed, and it is the reason the uniform-field equation E = ΔV/Δd works with the magnitudes alone once the direction is known.

Practically, this means that on a graph of V against r, the gradient at a point gives -E, and on a graph of E against r, the area under the curve between two radii gives the change in potential. Both readings are examined.

Since V goes as 1/r and E as 1/r², their graphs have different shapes: the potential curve falls away more gently. Sketching one and assuming the other is the same shape is a common error.

Electric potential energy

The potential energy of a charge q at a point where the potential is V is

E_P = qV

so for two point charges:

E_P = Qq / (4πε₀r)

The sign carries meaning:

Worked example. How much work is needed to bring an alpha particle, charge +2e, from a long distance away to within 2.0 × 10⁻¹⁴ m of a gold nucleus, charge +79e? Take e as 1.60 × 10⁻¹⁹ C.

Charge on the alpha particle:

2 × 1.60 × 10⁻¹⁹ = 3.20 × 10⁻¹⁹

Charge on the nucleus:

79 × 1.60 × 10⁻¹⁹ = 1.264 × 10⁻¹⁷

E_P = 8.99 × 10⁹ × 3.20 × 10⁻¹⁹ × 1.264 × 10⁻¹⁷ / (2.0 × 10⁻¹⁴) = 1.818 × 10⁻¹²

so about 1.8 × 10⁻¹² J, which is roughly 11 MeV. Because energy is conserved, that is also the kinetic energy an alpha particle must have to reach that distance, which is how the closest approach in the Rutherford scattering experiment is calculated, and how the size of a nucleus was first estimated.

Common mistakes

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