Electric current


The electric current is the rate of change of electric charge in a given point. In other words, it's how much charge is passing through a location. It is defined as the time derivative of electric charge

I(t)=Q(t)dtI(t)=\frac{Q(t)}{dt}

The SI unit of current is the Ampere A\text{A}, which are Coulombs per second.

Current can be seen as both a Scalar and vector quantity. The vector interpretation is more complete as current requires motion of charges, which is described by velocity, a vector quantity. However, the scalar form is often sufficient when motion is constrained to a specific path, such as in electric wiring. In the scalar case, care should be taken to get the sign right.

By convention, negative charges moving in one direction count the same as positive charges moving in the opposite direction. This is to reflect the physical fact that almost all laws regarding charge movement depend on the product of charge and velocity, so if you reverse the signs of both, the phenomenon doesn't change. For an example, see the Lorentz force. In practice, it's usually electrons that move and they do so in the opposite direction of the current.

A current is said to be steady or stationary if it does not vary with time:

Jt=0\frac{\partial \mathbf{J}}{\partial t}=0

This are of major important as they constitute the basis of the entirety of magnetostatics. In fact, a temporally constant current produces only constant magnetic fields and is the magnetic equivalent of a stationary charge for electrostatics. They are also good approximations of household currents.

Linear current

The most common case of current is one going through a wire. In this case, we can represent the charge as a line density:

I=λvI=\lambda v

because a segment of length vΔtv\Delta t carrying charge λvΔt\lambda v\Delta t goes through a point PP in a time interval Δt\Delta t. This derivation shows that current is actually a vector

I=λv\mathbf{I}=\lambda \mathbf{v}

though since current is usually constrained to a very specific path (like the aforementioned wire), it's common practice to just use the scalar form and give the direction for granted. When it comes to surface and volume currents however, the distinction must be clear.

The magnetic force on a current carrying wire subject to a magnetic field B\mathbf{B} is

Fmag=(v×B) dq=(v×B)λ dl=(I×B) dl\mathbf{F}_\text{mag}=\int(\mathbf{v}\times \mathbf{B})\ dq=\int(\mathbf{v}\times \mathbf{B})\lambda\ dl=\int(\mathbf{I}\times \mathbf{B})\ dl

Since I\mathbf{I} and dId\mathbf{I} point in the same direction, we can rewrite the result as

Fmag=I(dI×B)\mathbf{F}_\text{mag}=\int I(d\mathbf{I}\times \mathbf{B})

Since the current is often constant, the force usually is

Fmag=I(dI×B)\mathbf{F}_\text{mag}=I\int(d\mathbf{I}\times \mathbf{B})

Surface current

A current may also move over a surface instead of a line. In this case, we can defined the surface current density K\mathbf{K}. Consider a "ribbon" of infinitesimal width dldl_{\perp}, running parallel to the flow like a surfer on a wave. If the (linear) current (density) in the ribbon is dId\mathbf{I}, then the surface current density is

KdIdl\mathbf{K}\equiv \frac{d\mathbf{I}}{dl_{\perp}}

In other words, it's the current per unit width of the surface. If we have a surface charge density σ\sigma moving at a velocity v\mathbf{v}, then the current density is

K=σv\mathbf{K}=\sigma \mathbf{v}

The magnetic force on the surface current is

Fmag=(v×B)σ da=(K×B) da\mathbf{F}_\text{mag}=\int(\mathbf{v}\times \mathbf{B})\sigma\ da=\int(\mathbf{K}\times \mathbf{B})\ da

As with the electric force on a conductor, the magnetic field suffers a discontinuity across the surface and we instead use the average of the fields above and below.

Volume current

A current may also move in space. Here we define the volume current density J\mathbf{J}. Consider a "tube" of infinitesimal cross section dada_{\perp} running parallel to the flow like an airplane in a wind current. If the current in the tube is I\mathbf{I}, then the volume current density is

JdIda\mathbf{J}\equiv \frac{d\mathbf{I}}{da_{\perp}}

Like the surface density, it's the current per unit area of the volume. If the volume charge ρ\rho is moving at a velocity v\mathbf{v}, then the current density is

J=ρv\mathbf{J}=\rho \mathbf{v}

and the magnetic force on the volume current is

Fmag=(v×B)ρ dτ=(J×B) dτ\mathbf{F}_\text{mag}=\int(\mathbf{v}\times \mathbf{B})\rho\ d\tau=\int(\mathbf{J}\times \mathbf{B})\ d\tau

Continuity equation

The volume current density allows us to reach a fundamental result for currents. Rewrite the linear current in terms of the volume density

I=SJda=SJdaI=\int_{S}Jda_{\perp}=\int_{S}\mathbf{J}\cdot d\mathbf{a}

We can then apply the divergence theorem to get

SJda=VJ dτ\oint_{S}\mathbf{J}\cdot d\mathbf{a}=\int_{V}\nabla\cdot\mathbf{J}\ d\tau

which is the the charge per unit time leaving the surface SS. But charge is always conserved, so the charge the exits must leave a deficit of charge behind:

VJ dτ=ddtVρ dτ=Vρt dτ\int_{V}\nabla\cdot\mathbf{J}\ d\tau=- \frac{d}{dt}\int_{V}\rho\ d\tau=-\int_{V}\frac{ \partial \rho }{ \partial t }\ d\tau

Since there is no requirement on the volume chosen, we can extract the integrands to get the continuity equation:

J=ρt\boxed{\nabla\cdot\mathbf{J}=- \frac{ \partial \rho }{ \partial t } }

This is the mathematical statement that encapsulates local charge conservation. In the magnetostatic case, it becomes

J=0\nabla\cdot\mathbf{J}=0

which states that the current must be solenoidal (divergenceless).

Relativity

The continuity equation takes on a very simple form when using the four-current

Jμ=ρ0ημ=(cρ,Jx,Jy,Jz)J^{\mu}=\rho_{0}\eta^{\mu}=(c\rho,J_{x},J_{y},J_{z})

With the definition of Divergence the old three-current says:

J=i=13Jixi\nabla\cdot \mathbf{J}=\sum_{i=1}^{3} \frac{ \partial J^{i} }{ \partial x^{i} }

By looking at the definition of four-current we can see

ρt=1cJ0t=J0x0\frac{ \partial \rho }{ \partial t } =\frac{1}{c}\frac{ \partial J^{0} }{ \partial t } =\frac{ \partial J^{0} }{ \partial x^{0} }

As it happens, the continuity equation is just the sum of all the partial derivatives of JμJ^{\mu} set to zero:

Jμxμ=0\boxed{\frac{ \partial J^{\mu} }{ \partial x^{\mu} } =0}

This is the relativistic continuity equation for electric charge (in Einstein notation). It states that the four-current is always solenoidal (divergenceless), as opposed to the three-current, which solenoidal only in magnetostatics.