Electromagnetism

Electric Potential and Voltage

Electric potential energy per unit charge — V = U/q, measured in volts

Electric potential V is the electric potential energy per unit charge at a point in space — V = U/q, measured in volts (1 V = 1 J/C). It equals the work per coulomb needed to bring a positive test charge from a reference point (usually infinity or ground) to that location. For a single point charge, V = kq/r with k = 8.99 × 10⁹ N·m²/C²; the electric field is its negative gradient, E = -∇V; and equipotential surfaces are everywhere perpendicular to the field lines. Only potential differences — voltages — are physically measurable.

  • DefinitionV = U / q
  • SI unitvolt · 1 V = 1 J/C
  • Point chargeV = kq / r
  • Coulomb constant k8.99 × 10⁹ N·m²/C²
  • Field relationE = -∇V (V/m = N/C)
  • Work doneW = qΔV = q(V_B - V_A)

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Definition

Electric potential is defined as electric potential energy per unit charge. If a charge q placed at some point has electric potential energy U there, the electric potential at that point is:

V = U / q

Equivalently, V at a point is the work W an external agent must do, per unit charge, to carry a small positive test charge from a chosen reference point to that point without changing its kinetic energy:

V = W_ref→point / q₀

The SI unit is the volt (V), named after Alessandro Volta. One volt is one joule per coulomb:

1 V = 1 J/C = 1 kg·m²·s⁻³·A⁻¹

Potential is a scalar field — it has a value but no direction — which makes it far easier to work with than the vector electric field. Crucially, potential is a property of the location, set up by surrounding charges; the test charge merely samples it and does not have to be present for V to be defined.

Potential of a point charge

Integrating the Coulomb field of a single point charge q inward from infinity (where we set V = 0) gives the most-used result in the subject:

V(r) = k·q / r        with  k = 1/(4πε₀) ≈ 8.99 × 10⁹ N·m²/C²

Note that potential falls off as 1/r, whereas the field magnitude E = kq/r² falls off as 1/r². The sign of V follows the sign of q: near a positive charge V > 0 (a "hill" for positive charges), near a negative charge V < 0 (a "valley").

Because potential is a scalar, the potential of several charges is a simple algebraic sum — no vector components, no angles:

V = Σᵢ k·qᵢ / rᵢ

This superposition-by-addition is why physicists often compute V first and then extract the field from it.

Field from potential: E = -∇V

The electric field is the negative gradient of the potential:

E = -∇V = -(∂V/∂x, ∂V/∂y, ∂V/∂z)

In one dimension this reduces to E_x = -dV/dx. The minus sign encodes a physical fact: the field points from high to low potential, so a positive charge accelerates "downhill," converting potential energy into kinetic energy. The steeper the potential slope, the stronger the field. Consequently the field's unit, volts per metre (V/m), is identical to newtons per coulomb (N/C).

The inverse relationship recovers potential difference by a line integral of the field:

V_B - V_A = -∫_A^B E · dl

Because the electrostatic field is conservative (∇ × E = 0), this integral is path-independent — the same ΔV results no matter which route you take between A and B. That is exactly the condition that lets us define a single-valued potential at all.

Equipotential surfaces

An equipotential surface is the set of all points at the same potential V. Two properties follow directly:

  • No work along the surface. Moving a charge between two points on the same equipotential costs zero work, since W = qΔV and ΔV = 0.
  • Perpendicular to the field. The field is everywhere normal to equipotentials. If E had any component along the surface, moving along it would change V — contradicting "equal potential." So field lines and equipotentials always cross at 90°.

For a point charge the equipotentials are concentric spheres; near a large flat charged plate they are parallel planes; the surface of any conductor in electrostatic equilibrium is itself an equipotential (which is why the field just outside a conductor is perpendicular to it).

Worked example: work to move a charge

Suppose point A sits at 12 V and point B at 4 V. How much work does the field do on a +2 μC charge carried from A to B?

ΔV = V_B - V_A = 4 V - 12 V = -8 V
W_field = -q·ΔV = -(2 × 10⁻⁶ C)(-8 V) = +1.6 × 10⁻⁵ J

The field does positive work (+16 μJ): a positive charge moving from high to low potential loses potential energy, which appears as kinetic energy. Equivalently, the external agent that instead holds it back does -16 μJ. Had the charge been negative, every sign would flip and the field would do negative work.

A convenient energy unit follows from W = qΔV: accelerate one electron (q = 1.602 × 10⁻¹⁹ C) through 1 volt and it gains one electron-volt, 1 eV = 1.602 × 10⁻¹⁹ J — the working currency of atomic and particle physics.

Reference points and why voltage is a difference

Only differences in potential produce measurable work, force, or field. The zero of potential is therefore an arbitrary choice, like sea level for altitude:

  • Electrostatics. Set V = 0 at infinity — this makes V = kq/r come out cleanly.
  • Circuits. Set V = 0 at the earth (ground) or the battery's negative terminal, and measure everything relative to it.

Shifting the reference adds the same constant to V everywhere, which never changes E = -∇V or any voltage you can measure with a meter. A "9-volt battery" does not put its terminals at 9 V absolutely; it maintains a 9 V difference between them. This is why "voltage" in engineering almost always means potential difference ΔV, and why a voltmeter always has two probes.

Representative potentials and voltages

SituationPotential difference / potential
Neuron resting membrane potential≈ -70 mV
Single AA / alkaline cell1.5 V
Car battery12 V
Household mains (RMS, US / EU)120 V / 230 V
Van de Graaff generator domeup to ~10⁶ V
High-voltage transmission line≈ 10⁵–10⁶ V
Lightning leader-to-ground≈ 10⁸–10⁹ V
Potential 1 cm from a +1 nC chargeV = kq/r ≈ 900 V

Key relations at a glance

QuantityRelationNotes / units
Potential (definition)V = U / qvolts; U in J, q in C
Point chargeV = kq / rV = 0 at r → ∞; scalar sum for many charges
Potential energy of a chargeU = qVjoules; depends on the charge placed
Work by the fieldW = -qΔVpositive charge falls from high to low V
Field from potentialE = -∇VV/m = N/C
Potential from fieldV_B - V_A = -∫ E·dlpath-independent (conservative field)
Pair of point chargesU = kq₁q₂ / rinteraction energy, joules
Energy unit1 eV = 1.602 × 10⁻¹⁹ Jone electron through 1 V

JavaScript — potential calculations

const k = 8.9875517923e9;   // Coulomb constant, N·m²/C²
const e = 1.602176634e-19;  // elementary charge, C

// Potential of a single point charge at distance r (V=0 at infinity)
function pointPotential(q, r) { return k * q / r; }

console.log(`+1 nC at 1 cm: ${pointPotential(1e-9, 0.01).toFixed(0)} V`); // ~899 V

// Potential from many charges — SCALAR sum (no vectors!)
function totalPotential(charges, x, y) {
  return charges.reduce((V, c) => {
    const r = Math.hypot(x - c.x, y - c.y);
    return V + k * c.q / r;
  }, 0);
}

// A dipole: +1 nC and -1 nC, 2 cm apart, evaluated at the midpoint-off-axis
const dipole = [{ q: 1e-9, x: -0.01, y: 0 }, { q: -1e-9, x: 0.01, y: 0 }];
console.log(`Dipole V at (0, 0.02): ${totalPotential(dipole, 0, 0.02).toFixed(3)} V`); // ~0 by symmetry

// Work done BY the field moving charge q from A to B
function workByField(q, V_A, V_B) { return -q * (V_B - V_A); }

console.log(`+2 µC from 12 V to 4 V: ${(workByField(2e-6, 12, 4) * 1e6).toFixed(1)} µJ`); // +16.0 µJ

// Convert a kinetic energy in joules to electron-volts
function toEV(joules) { return joules / e; }

// Electron accelerated through 100 V gains 100 eV
console.log(`Electron through 100 V: ${toEV(e * 100).toFixed(0)} eV`); // 100 eV

// Interaction potential energy of two point charges
function pairEnergy(q1, q2, r) { return k * q1 * q2 / r; }

console.log(`Two protons 1 fm apart: ${pairEnergy(e, e, 1e-15).toExponential(2)} J`); // ~2.3e-13 J

Where electric potential shows up

  • Circuits. Voltage drives current: Ohm's law V = IR, power P = IV, and Kirchhoff's voltage law (Σ ΔV = 0 around a loop) are all statements about potential.
  • Capacitors. Stored charge Q = CV and energy U = ½CV² depend directly on the potential difference across the plates.
  • Particle accelerators. Charged particles gain kinetic energy qΔV; the electron-volt is the natural unit — the LHC runs to 6.8 TeV per beam.
  • Electrochemistry. Cell EMF and electrode potentials (measured in volts) determine which redox reactions run spontaneously.
  • Neuroscience. Membrane potentials (~-70 mV rest, spiking to +40 mV) encode and transmit every nerve signal.
  • Electronics design. "Ground," logic-level thresholds, and signal levels are all defined relative to a chosen reference potential.
  • Field mapping. Equipotential/field-line plots make electrostatic geometry (conductors, shielding, corona) intuitive.

Common mistakes

  • Confusing potential V with potential energy U. V is energy per charge (volts, a field property); U = qV is energy (joules, tied to a specific charge). Doubling the test charge doubles U but leaves V unchanged.
  • Treating potential as a vector. V is a scalar — you add the numbers. It is the field E = -∇V that has direction. Never resolve potential into components.
  • Forgetting the reference point. A bare statement "V = 20 V" is meaningless without saying relative to what. Only ΔV between two points is measurable.
  • Assuming zero field means zero potential (or vice versa). At the center of a uniformly charged sphere or midway between equal charges, E = 0 but V ≠ 0. Potential can be flat (large V, zero slope) or zero-crossing with strong slope.
  • Dropping the minus sign in E = -∇V. The field points toward decreasing potential; forgetting the sign reverses the force direction.
  • Confusing the 1/r of potential with the 1/r² of the field. V = kq/r but E = kq/r² for a point charge — they scale differently with distance.

Frequently asked questions

What is electric potential in simple terms?

Electric potential V at a point is the electric potential energy a charge would have there, divided by the size of the charge: V = U/q. It tells you how much work per coulomb it takes to bring a positive test charge from a reference point to that location. Its unit is the volt, where 1 volt = 1 joule per coulomb (1 V = 1 J/C). Potential is a property of the point in space set up by other charges — the test charge just samples it.

What is the difference between voltage and electric potential?

"Voltage" almost always means a potential difference — the difference in electric potential between two points, ΔV = V_B - V_A. Electric potential V is defined at a single point relative to a reference where V = 0. A 9-volt battery does not mean either terminal is at 9 V absolutely; it means the two terminals differ by 9 V. Because only differences do measurable work (W = qΔV), the terms are often used interchangeably in circuits.

How do you calculate the potential of a point charge?

For a single point charge q, the potential at distance r (taking V = 0 at infinity) is V = kq/r, where k = 1/(4πε₀) ≈ 8.99 × 10⁹ N·m²/C². Note it falls off as 1/r, not 1/r² like the field. For several charges, potential is a scalar sum: V = Σ kqᵢ/rᵢ — you just add the numbers, no vector components. That scalar nature makes potential far easier to compute than the electric field.

Why is the electric field the negative gradient of potential?

The field is E = -∇V. The gradient ∇V points toward increasing potential, so the field points from high to low potential (the minus sign). Physically, a positive charge accelerates "downhill" in potential, releasing energy. In one dimension, E_x = -dV/dx, so the field magnitude equals the steepness of the potential slope. Volts per metre (V/m) and newtons per coulomb (N/C) are therefore the same unit.

What are equipotential surfaces?

An equipotential surface connects all points at the same potential V. No work is done moving a charge along it, because ΔV = 0. Equipotentials are always perpendicular to the electric field lines: if the field had any component along the surface, that would imply a potential change, contradicting "equal potential." For a point charge the equipotentials are concentric spheres; near a flat charged plate they are parallel planes.

What is the difference between electric potential and potential energy?

Potential energy U is measured in joules and depends on the specific charge: U = qV. Electric potential V is the energy per unit charge, in joules per coulomb (volts), and is a property of the location alone — it exists whether or not a charge is placed there. Double the test charge and its potential energy doubles, but the potential at that point is unchanged. Potential is to potential energy what temperature is to heat: an intensive field, not an amount.

Why is the ground defined as zero volts?

Because only potential differences matter, the zero of potential is a free choice. In circuits we usually call the earth (ground) or the battery's negative terminal 0 V and measure everything relative to it. In electrostatics theory we instead set V = 0 at infinity, which makes V = kq/r come out cleanly. Both conventions are valid; they just shift every potential by the same constant, which never changes any field, force, or measurable voltage.