6.2.4 - Electric potential, energy and isolated spheres

6.2.4 - Electric potential, energy and isolated spheres

Electric potential lets you talk about energy in an electric field without carrying a particular test charge through every sentence. In this lesson you will define potential relative to infinity, use the point-charge potential equation, derive the capacitance of an isolated conducting sphere, and connect force-distance graphs to work done. The key habit is to choose the right model: radial fields around point or spherical charges are not uniform parallel-plate fields.

Potential from infinity

Electric potential is the electric version of "energy per unit charge". It is useful because the field around a source charge may be complicated, but once you know the potential at a point, the energy of a charge placed there is found by multiplying by that charge.

Electric potential

Electric potential at a point is the work done by an external agent per unit positive charge in bringing a small positive test charge slowly from infinity to that point, with no change in its kinetic energy. Electric potential is zero at infinity.

The unit of electric potential is the volt, V\mathrm{V}. Since it is work done per unit charge,

1 V=1 J C−1.1\ \text{V} = 1\ \text{J C}^{-1}.

The phrase "unit positive charge" matters. Potential is defined using a positive test charge, so a positive source charge gives a positive potential and a negative source charge gives a negative potential. Potential is a scalar: it has a sign, but it is not a vector direction.

Infinity is chosen as the zero because, very far from an isolated point charge or spherical charge, the field becomes negligible and the potential tends to zero. This is like choosing a reference level for gravitational potential energy: the value only makes sense once the zero has been chosen.

Do not confuse electric potential with electric field strength. Electric field strength is force per unit charge and is a vector, measured in N C−1\mathrm{N}\,\mathrm{C}^{-1} or V m−1\mathrm{V}\,\mathrm{m}^{-1}. Electric potential is energy per unit charge and is a scalar, measured in J C−1\mathrm{J}\,\mathrm{C}^{-1} or V\mathrm{V}.

Potential near a point charge

For a point charge, or for a charged sphere when you are outside the sphere, the electric potential depends on distance from the centre of the charge distribution.

Electric potential due to a point charge

V=Q4πε0rV = \frac{Q}{4\pi\varepsilon_0 r}

Here VV is the electric potential at the point in volts, QQ is the source charge in coulombs, rr is the distance from the source charge in metres, and ε0\varepsilon_0 is the permittivity of free space. The factor 1/(4πε0)1/(4\pi\varepsilon_0) is the same constant that appears in Coulomb's law.

There are three important consequences.

First, the sign of VV follows the sign of QQ. A positive source charge gives a positive potential; a negative source charge gives a negative potential.

Second, the magnitude of VV decreases as rr increases. The potential tends towards zero at infinity, so a point close to a positive source charge is at a higher potential than a point further away.

Third, this equation is not the uniform-field equation. The equation E=V/dE = V/d belongs to a uniform field between parallel plates. Around a point charge or isolated sphere, the field is radial and changes with distance, so you must use the point-charge potential equation for VV.

For changes in potential between two distances:

ΔV=VB−VA=Q4πε0(1rB−1rA).\Delta V = V_B - V_A = \frac{Q}{4\pi\varepsilon_0}\left(\frac{1}{r_B}-\frac{1}{r_A}\right).

Worked example: change in potential

A small object has charge Q=+8.0 nCQ = +8.0\,\mathrm{nC}. Point A is 0.20 m0.20\,\mathrm{m} from the object and point B is 0.50 m0.50\,\mathrm{m} from it. Determine the change in electric potential from A to B.

Convert the charge:

8.0 nC=8.0×10−9 C.8.0\ \text{nC} = 8.0 \times 10^{-9}\ \text{C}.

Use 1/(4πε0)=8.99×109 N m2C−21/(4\pi\varepsilon_0) = 8.99 \times 10^9\ \text{N m}^2\text{C}^{-2}.

At A:

VA=(8.99×109)(8.0×10−9)0.20=3.6×102 V.V_A = \frac{(8.99\times10^9)(8.0\times10^{-9})}{0.20} = 3.6\times10^2\ \text{V}.

At B:

VB=(8.99×109)(8.0×10−9)0.50=1.4×102 V.V_B = \frac{(8.99\times10^9)(8.0\times10^{-9})}{0.50} = 1.4\times10^2\ \text{V}.

So

ΔV=VB−VA=144−360=−216 V.\Delta V = V_B - V_A = 144 - 360 = -216\ \text{V}.

The negative sign means the potential has decreased as the point has moved further from the positive charge.

Isolated sphere capacitance

An isolated conducting sphere can store charge. The charge spreads over the outside surface, and outside the sphere the electric field and potential are the same as if all the charge were concentrated at the centre.

The capacitance of any conductor is

C=QV,C = \frac{Q}{V},

where QQ is the charge on the conductor and VV is its potential relative to infinity.

For a conducting sphere of radius RR, the surface is at distance RR from the centre. Use the point-charge potential equation at the surface:

V=Q4πε0R.V = \frac{Q}{4\pi\varepsilon_0 R}.

Now substitute this into C=Q/VC = Q/V:

C=QQ/(4πε0R).C = \frac{Q}{Q/(4\pi\varepsilon_0 R)}.

The charge QQ cancels:

C=4πε0R.C = 4\pi\varepsilon_0 R.

Capacitance of an isolated sphere

C=4πε0RC = 4\pi\varepsilon_0 R

This result has a simple meaning: a larger isolated sphere has a larger capacitance. It can hold more charge for the same potential because the charge is spread over a larger conductor and the surface is further from the centre.

Be careful with the word "isolated". It means the sphere is far from other conductors and charge distributions, so infinity can act as the zero-potential reference. It is not a parallel-plate capacitor, and it does not have a second nearby plate.

Worked example: OCR-style sphere calculation

A metal sphere has radius 1.5 cm1.5\,\mathrm{cm} and is charged to a potential of +5.0 kV+5.0\,\mathrm{kV}. Calculate the charge on the sphere.

Convert the values:

R=1.5 cm=1.5×10−2 mR = 1.5\ \text{cm} = 1.5\times10^{-2}\ \text{m} V=5.0 kV=5.0×103 V.V = 5.0\ \text{kV} = 5.0\times10^3\ \text{V}.

First calculate the capacitance:

C=4π(8.85×10−12)(1.5×10−2)=1.67×10−12 F.C = 4\pi(8.85\times10^{-12})(1.5\times10^{-2}) = 1.67\times10^{-12}\ \text{F}.

Then use Q=CVQ = CV:

Q=(1.67×10−12)(5.0×103)=8.3×10−9 C.Q = (1.67\times10^{-12})(5.0\times10^3) = 8.3\times10^{-9}\ \text{C}.

The answer is small because even a conducting sphere has a very small capacitance unless its radius is very large.

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