STEMviz
Physics · Electromagnetism and Electrodynamics

Steady Currents and the Continuity Equation

Charge conservation in local form is the continuity equation ∇⋅J⃗=−∂ρ/∂t\nabla\cdot\vec{J}=-\partial\rho/\partial t, which for steady currents becomes ∇⋅J⃗=0\nabla\cdot\vec{J}=0 (solenoidal current, same II at every section of a wire); Ohm's law J⃗=σE⃗\vec{J}=\sigma\vec{E} is a material relation with Drude value σ=ne2τ/m\sigma=ne^2\tau/m, giving R=ρresL/AR=\rho_{\text{res}}L/A and V=IRV=IR; an EMF source supplies E=∮f⃗s⋅dℓ⃗\mathcal{E}=\oint\vec{f}_s\cdot d\vec{\ell} with terminal voltage E−Ir\mathcal{E}-Ir; power dissipated is ∫J⃗⋅E⃗ dτ=I2R\int\vec{J}\cdot\vec{E}\,d\tau=I^2R; at a conductor interface J⊥J_\perp is continuous and interior charge relaxes as e−t/τre^{-t/\tau_r} with τr=ε/σ\tau_r=\varepsilon/\sigma.

Steady Currents, the Continuity Equation and Ohm's Law

This chapter is the bridge between electrostatics and magnetism. Moving charge is a current, and steady (time-independent) currents are the sources of static magnetic fields, taken up in the next chapter. Before that, we need the language of current: the current density J⃗\vec{J}, the local statement of charge conservation (the continuity equation), the microscopic content of Ohm's law, the idea of electromotive force that keeps a steady current flowing against resistance, and the boundary conditions and power relations that go with them.

The organising principle is charge conservation. Charge is never created or destroyed, only transported; the continuity equation ∇⋅J⃗=−∂ρ/∂t\nabla\cdot\vec{J} = -\partial\rho/\partial t is that fact written locally. For a steady current — the defining case of this chapter and of magnetostatics — nothing depends on time, so ∂ρ/∂t=0\partial\rho/\partial t = 0 and ∇⋅J⃗=0\nabla\cdot\vec{J} = 0: steady current is divergence-free, its field lines form closed loops, and the same current crosses every section of a single wire. Everything else (Ohm's law, EMF, resistor networks) is built on that.

How to read this chapter. The two equations to carry forward are ∇⋅J⃗=−∂ρ/∂t\nabla\cdot\vec{J} = -\partial\rho/\partial t (always true) and, for the steady state, ∇⋅J⃗=0\nabla\cdot\vec{J} = 0. Ohm's law in the form J⃗=σE⃗\vec{J} = \sigma\vec{E} is a material property, not a law of nature — it holds for ordinary conductors in ordinary fields and fails for many materials. Keep "conductivity σ\sigma" (this chapter) distinct from "surface charge σ\sigma" (earlier chapters); context disambiguates, and this chapter uses σ\sigma for conductivity throughout.

1. Current and Current Density

The current II through a surface is the rate at which charge crosses it, I=dQ/dtI = dQ/dt, in amperes (C/s). It is a scalar attached to a surface (with a chosen positive sense). The local quantity is the current density J⃗\vec{J}, a vector field: J⃗\vec{J} points in the direction of positive-charge flow, and its magnitude is the current per unit cross-sectional area perpendicular to the flow. The current through any surface S\mathcal{S} is the flux

I=∫SJ⃗⋅da⃗I = \int_{\mathcal{S}} \vec{J}\cdot d\vec{a}

If a density ρ\rho of mobile charge moves with average (drift) velocity v⃗\vec{v}, then

J⃗=ρ v⃗\vec{J} = \rho\,\vec{v}

For a metal with nn conduction electrons per unit volume, each of charge −e-e drifting at v⃗d\vec{v}_d, this is J⃗=−ne v⃗d\vec{J} = -n e\,\vec{v}_d (and the current flows opposite to the electron motion). Drift speeds are tiny — millimetres per second in a household wire — even though signals propagate near the speed of light, because the field, not the electrons, carries the information.

2. The Continuity Equation

Charge conservation applied to a fixed volume V\mathcal{V}: the rate of decrease of enclosed charge equals the net current out through the boundary,

−ddt∫Vρ dτ=∯∂VJ⃗⋅da⃗-\frac{d}{dt}\int_{\mathcal{V}}\rho\,d\tau = \oiint_{\partial\mathcal{V}}\vec{J}\cdot d\vec{a}

Applying the divergence theorem to the right side and shrinking V\mathcal{V} to a point gives the continuity equation:

  ∇⋅J⃗=−∂ρ∂t  \boxed{\;\nabla\cdot\vec{J} = -\frac{\partial\rho}{\partial t}\;}

This is one of the most fundamental statements in physics — more robust than any particular force law. In electrodynamics it is built into Maxwell's equations (it follows from taking the divergence of the Ampère–Maxwell law), which is why the displacement-current term is not optional.

For a steady current, ∂ρ/∂t=0\partial\rho/\partial t = 0 everywhere, so

∇⋅J⃗=0(steady state)\nabla\cdot\vec{J} = 0 \qquad \text{(steady state)}

J⃗\vec{J} is then solenoidal: field lines of J⃗\vec{J} never begin or end, currents flow in closed loops, and ∮J⃗⋅da⃗=0\oint \vec{J}\cdot d\vec{a} = 0 through any closed surface — the current into any region equals the current out. In a single unbranched wire, II is the same at every cross-section.

3. Ohm's Law: the Microscopic Statement

Experimentally, in a wide class of materials the current density is proportional to the field driving it:

  J⃗=σE⃗  \boxed{\;\vec{J} = \sigma\vec{E}\;}

where σ\sigma is the conductivity (S/m) and its reciprocal ρres=1/σ\rho_{\text{res}} = 1/\sigma is the resistivity (Ω⋅\Omega\cdotm). This is Ohm's law in local form. It is a constitutive relation, valid for "ohmic" materials over a range of fields, not a universal law: semiconductors, plasmas, and metals at high field all deviate.

The Drude model gives it microscopic content. Free electrons are accelerated by E⃗\vec{E} between random collisions that occur, on average, every τ\tau (the mean free time) and which randomise the velocity. Between collisions, mv⃗˙=−eE⃗m\dot{\vec{v}} = -e\vec{E}; averaging, the drift velocity reaches a steady value v⃗d=−eτmE⃗\vec{v}_d = -\dfrac{e\tau}{m}\vec{E}. Then

J⃗=−ne v⃗d=ne2τm E⃗⇒σ=ne2τm\vec{J} = -n e\,\vec{v}_d = \frac{n e^2\tau}{m}\,\vec{E} \quad\Rightarrow\quad \sigma = \frac{n e^2\tau}{m}

Conductivity is high when there are many carriers (nn), they are light (mm), and they travel far between collisions (τ\tau). Rising temperature shortens τ\tau (more lattice vibrations), so metals' resistivity increases with temperature.

4. Resistance and Ohm's Law for a Device

For a uniform conductor of length LL, cross-section AA, carrying current II driven by a potential difference VV across its ends: the field inside is E=V/LE = V/L, the current density is J=I/AJ = I/A, and J⃗=σE⃗\vec{J} = \sigma\vec{E} gives IA=σVL\dfrac{I}{A} = \sigma\dfrac{V}{L}, i.e.

V=IR,R=LσA=ρres LAV = IR, \qquad R = \frac{L}{\sigma A} = \frac{\rho_{\text{res}}\,L}{A}

the familiar "Ohm's law" for a resistor. RR is a geometric-plus-material property, in ohms. Note that inside a current-carrying wire E⃗≠0\vec{E}\ne 0 — unlike the electrostatic conductor of Chapter 1, a resistor sustains an interior field, maintained by a slight surface-charge gradient along the wire.

5. Electromotive Force

A steady current in a resistive circuit dissipates energy, so something must continuously supply it. That "something" is a source of electromotive force (EMF), E\mathcal{E} — a battery, a generator, a solar cell. Inside the source, a non-electrostatic force per unit charge f⃗s\vec{f}_s (chemical, mechanical, photovoltaic) pushes charge from low to high potential. The EMF is the work done per unit charge by that source force around the circuit:

E=∮f⃗s⋅dℓ⃗\mathcal{E} = \oint \vec{f}_s\cdot d\vec{\ell}

For an ideal source the entire loop integral comes from inside the source, and E\mathcal{E} equals the open-circuit terminal voltage. A real source has internal resistance rr: with a current II flowing, the terminal voltage is V=E−IrV = \mathcal{E} - Ir, and the load gets E\mathcal{E} minus the internal drop. Motional EMF — the qv⃗×B⃗q\vec{v}\times\vec{B} force on charges in a conductor moving through a magnetic field — is the same idea and is developed fully in Chapter 7.

6. Power

The rate at which the field does work on the moving charge, per unit volume, is J⃗⋅E⃗\vec{J}\cdot\vec{E}. Integrated over a resistor:

P=∫J⃗⋅E⃗ dτ=VI=I2R=V2RP = \int \vec{J}\cdot\vec{E}\,d\tau = VI = I^2 R = \frac{V^2}{R}

For an ohmic conductor this power goes entirely into heat (Joule heating): the drift energy gained from the field between collisions is handed to the lattice at each collision. In a source delivering current, the source does work at rate EI\mathcal{E}I; of this, I2rI^2 r is lost internally and VI=(E−Ir)IVI = (\mathcal{E} - Ir)I reaches the load.

Worked example — the two current-carrying geometries. (a) A wire of resistivity ρres\rho_{\text{res}}, length LL, radius aa: R=ρresL/πa2R = \rho_{\text{res}}L/\pi a^2. Doubling the radius quarters the resistance. (b) Current flowing radially between two concentric spherical shells (radii a<ba < b) through a medium of conductivity σ\sigma: by the steady condition the same II crosses every sphere, so J(r)=I/4πr2J(r) = I/4\pi r^2 and E=J/σE = J/\sigma; integrating, V=I4πσ(1a−1b)V = \dfrac{I}{4\pi\sigma}\left(\dfrac{1}{a} - \dfrac{1}{b}\right), giving R=14πσ(1a−1b)R = \dfrac{1}{4\pi\sigma}\left(\dfrac{1}{a} - \dfrac{1}{b}\right). The same 1/r21/r^2 that governed the electrostatic field of a point charge governs the current spreading from a small electrode.

7. Boundary Conditions and Charge Relaxation

At an interface between two conducting media in the steady state, ∇⋅J⃗=0\nabla\cdot\vec{J} = 0 forces the normal component of J⃗\vec{J} to be continuous:

J1⊥=J2⊥⟺σ1E1⊥=σ2E2⊥J_{1\perp} = J_{2\perp} \quad\Longleftrightarrow\quad \sigma_1 E_{1\perp} = \sigma_2 E_{2\perp}

Since ε1E1⊥≠ε2E2⊥\varepsilon_1 E_{1\perp} \ne \varepsilon_2 E_{2\perp} in general (different σ\sigma and ε\varepsilon), a free surface charge σf=D1⊥−D2⊥\sigma_f = D_{1\perp} - D_{2\perp} (normal pointing from medium 2 into medium 1) accumulates at the interface — a real, measurable effect wherever two materials with different σ/ε\sigma/\varepsilon ratios carry current across their junction.

Charge relaxation. If a charge density ρ\rho is placed in the interior of an ohmic conductor, combine ∇⋅J⃗=−∂ρ/∂t\nabla\cdot\vec{J} = -\partial\rho/\partial t with J⃗=σE⃗\vec{J} = \sigma\vec{E} and ∇⋅E⃗=ρ/ε\nabla\cdot\vec{E} = \rho/\varepsilon:

∂ρ∂t=−σε ρ⇒ρ(t)=ρ0 e−t/τr,τr=εσ\frac{\partial\rho}{\partial t} = -\frac{\sigma}{\varepsilon}\,\rho \quad\Rightarrow\quad \rho(t) = \rho_0\,e^{-t/\tau_r}, \qquad \tau_r = \frac{\varepsilon}{\sigma}

Interior charge decays exponentially to the surface with time constant τr=ε/σ\tau_r = \varepsilon/\sigma — about 10−1910^{-19} s for copper, but seconds or longer for a poor conductor. This is why the electrostatic assumption "all charge on the surface" is justified for good conductors, and it quantifies how quickly a conductor reaches electrostatic equilibrium.

8. Common Pitfalls

  • Assuming E⃗=0\vec{E} = 0 inside a current-carrying conductor. That is the electrostatic result. A resistor with current flowing has E⃗=J⃗/σ≠0\vec{E} = \vec{J}/\sigma \ne 0 inside, sustained by surface charge.
  • Treating ∇⋅J⃗=0\nabla\cdot\vec{J} = 0 as always true. It holds only in the steady state. In general ∇⋅J⃗=−∂ρ/∂t\nabla\cdot\vec{J} = -\partial\rho/\partial t; a charging capacitor plate has ∇⋅J⃗≠0\nabla\cdot\vec{J}\ne 0 at its surface.
  • Confusing conductivity σ\sigma with surface charge σ\sigma. Different quantities sharing a symbol; this chapter's σ\sigma is conductivity. Some texts write ρ\rho for resistivity, which then collides with charge density — watch the context.
  • Thinking EMF is a force. It is work per unit charge (units: volts), an integral of a force per unit charge around the loop.
  • Using V=EV = \mathcal{E} for a battery under load. With current flowing, the terminal voltage is E−Ir\mathcal{E} - Ir; only the open-circuit voltage equals E\mathcal{E}.
  • Forgetting the interface charge in steady currents. Continuity of J⊥J_\perp (not D⊥D_\perp) is the steady-current condition; the mismatch generically deposits free charge at the junction.
  • Expecting instantaneous electrostatic equilibrium. Charge relaxes with τr=ε/σ\tau_r = \varepsilon/\sigma; for good conductors this is fantastically fast, but for insulators it can be macroscopically slow.

Summary

  • Current I=∫J⃗⋅da⃗I = \int\vec{J}\cdot d\vec{a}; current density J⃗=ρv⃗\vec{J} = \rho\vec{v}, or −nev⃗d-ne\vec{v}_d in a metal.
  • Continuity equation: ∇⋅J⃗=−∂ρ/∂t\nabla\cdot\vec{J} = -\partial\rho/\partial t (charge conservation, local form). Steady state: ∇⋅J⃗=0\nabla\cdot\vec{J} = 0, so J⃗\vec{J} is solenoidal and II is the same at every section of a wire.
  • Ohm's law (local): J⃗=σE⃗\vec{J} = \sigma\vec{E}, a material relation. Drude model: σ=ne2τ/m\sigma = ne^2\tau/m; resistivity rises with TT because τ\tau falls.
  • Resistance: V=IRV = IR with R=L/σA=ρresL/AR = L/\sigma A = \rho_{\text{res}}L/A. Inside a current-carrying resistor E⃗≠0\vec{E}\ne 0.
  • EMF: E=∮f⃗s⋅dℓ⃗\mathcal{E} = \oint\vec{f}_s\cdot d\vec{\ell}, work per unit charge by the source. Real source: Vterminal=E−IrV_{\text{terminal}} = \mathcal{E} - Ir.
  • Power: P=∫J⃗⋅E⃗ dτ=VI=I2R=V2/RP = \int\vec{J}\cdot\vec{E}\,d\tau = VI = I^2R = V^2/R; Joule heating in an ohmic conductor.
  • Steady-current boundary condition: J⊥J_\perp continuous (σ1E1⊥=σ2E2⊥\sigma_1 E_{1\perp} = \sigma_2 E_{2\perp}); a free charge builds up at an interface where σ/ε\sigma/\varepsilon differs.
  • Charge relaxation: interior charge decays as e−t/τre^{-t/\tau_r} with τr=ε/σ\tau_r = \varepsilon/\sigma — the timescale for a conductor to reach electrostatic equilibrium.