Lorentz force


The Lorentz force is the force applied onto an electric charge in the presence of both an electric and magnetic field. It is a more general case of Coulomb's law, to which it goes back to if there is no magnetic field. It is

F=q[E+(v×B)]\mathbf{F}=q[\mathbf{E}+(\mathbf{v}\times \mathbf{B})]

where v\mathbf{v} is the velocity of the test charge qq. These fields refer to external source fields.

As a force density

It is possible to rewrite the Lorentz force as a force density over a volume. To do so, first notice that qv=Isq\mathbf{v}=I\mathbf{s}, where s\mathbf{s} is a length of space in which the electric current II runs. So

F=qE+Is×B\mathbf{F}=q\mathbf{E}+I\mathbf{s}\times \mathbf{B}

If we divide by volume V\mathcal{V} and notice that Is/V=JI\mathbf{s}/\mathcal{V}=\mathbf{J}, being the volume current density, and using q/V=ρq/\mathcal{V}=\rho the volume charge density, we have

f=ρE+J×B\mathbf{f}=\rho \mathbf{E}+\mathbf{J}\times \mathbf{B}

This is the force density. The amount fdτ\mathbf{f}d\tau is the Lorentz force applied to the volume element dτd\tau.

Using the Maxwell stress tensor

The Lorentz force can also be written in an extremely general and manifestly time-dependent form using the Maxwell stress tensor T\mathrm{T} and the Poynting vector S\mathbf{S}. The force is

F=STdaε0μ0ddtVS dτ\mathbf{F}=\oint_{\mathcal{S}}\mathrm{T}\cdot d\mathbf{a}-\varepsilon_{0}\mu_{0}\frac{d}{dt} \int_{\mathcal{V}}\mathbf{S}\ d\tau

which reduces to

F=STda\mathbf{F}=\oint_{\mathcal{S}}\mathrm{T}\cdot d\mathbf{a}

in static, time-independent contexts. Here, V\mathcal{V} is some volume and S\mathcal{S} is the bounding Surface of that volume. The force density instead reads

f=Tε0μ0St\mathbf{f}=\nabla\cdot \mathrm{T}-\varepsilon_{0} \mu_{0} \frac{ \partial \mathbf{S} }{ \partial t }

Work done

The Lorentz force does do work, but only the electric part does. Magnetic forces do no work. In fact, the work per unit distance dsd\mathbf{s} is

dW=Fds=q(E+v×B)ds=qEds+q(v×B)dsdW=\mathbf{F}\cdot d\mathbf{s}=q(\mathbf{E}+\mathbf{v}\times \mathbf{B})\cdot d\mathbf{s}=q\mathbf{E}\cdot d\mathbf{s}+q(\mathbf{v}\times \mathbf{B})\cdot d\mathbf{s}

The electric field can be in any direction, so Eds\mathbf{E}\cdot d\mathbf{s} gives something. Meanwhile, the (instantaneous) velocity has at any moment the same direction as dsd\mathbf{s}, since it's defined as v=ds/dt\mathbf{v}=d\mathbf{s}/dt. But remember that the vector product is always perpendicular to both of its arguments, so v×B\mathbf{v}\times \mathbf{B} has to be perpendicular to ds=vdtd\mathbf{s}=\mathbf{v}dt, which means that the scalar product is always zero: (v×B)ds=0(\mathbf{v}\times \mathbf{B})\cdot d\mathbf{s}=0. So what we're left with is

dW=qEdsdW=q\mathbf{E}\cdot d\mathbf{s}

The total work is then given by integrating this over any path.

The work is always carried out by the electric part of the force due to the charges having to move "counter-current" against the magnetic field. In this sense, a magnetic force just redirects an electric force, but it does no work itself, in the same way a normal force over a sloped surface redirects a force to push an object up against gravity but doesn't do work itself.

Newton's third law

Consider a point charge qq going at speed vv down the xx axis. Its electric and magnetic fields emit radially, as per the Liénard-Wiechert potentials. Say then that another charge qq travels down the yy axis. They would repel each other off the axes of course, but assume they are forced to remain on them through tracks or something of the sort. The electric force between them is clearly repulsive, so let's look at the magnetic one.

80%

The magnetic field of the particle 1 goes into the page (z^-\hat{\mathbf{z}}) at the position of particle 2. The force, by right hand rule, is to the right (x^\hat{\mathbf{x}}). Similarly, the magnetic field of 2 goes out of the page (z^\hat{\mathbf{z}}) at the position of 1, so the force is up (y^\hat{\mathbf{y}}). These are manifestly not opposites, so they do not cancel out. The action, so to say, does not result in an equal and opposite reaction. There's something very wrong with Newton's third law here, because it clearly does not hold in electrodynamics. But that's a problem: the conservation of momentum relies on the third law! So how do we fix it? Well, we fix it by saying that it's not just the particles that carry momentum, but also the fields themselves.

Conservation of linear momentum

According to the general form Newton's second law, the force on an object is the time derivative of its momentum:

F=dpmechdt\mathbf{F}=\frac{d\mathbf{p}_\text{mech}}{dt}

Here we are specifically calling the momentum "mechanical": you'll see why in a moment. Since we know F\mathbf{F}, we can see where this leads. We'll use the stress tensor form:

dpmechdt=ε0μ0ddtVS dτ+STda\frac{d\mathbf{p}_\text{mech}}{dt}=-\varepsilon_{0}\mu_{0}\frac{d}{dt} \int_{\mathcal{V}}\mathbf{S}\ d\tau+\oint_{\mathcal{S}}\mathrm{T}\cdot d\mathbf{a}

This expression is remarkably similar to Poynting's theorem and it is sensible to interpret it in a similar manner. The volume integral must then be the momentum "stored" in the fields

pfield=μ0ε0VSdτ\mathbf{p}_\text{field}=\mu_{0}\varepsilon_{0}\int_{\mathcal{V}}\mathbf{S}d\tau

and the surface integral must be the momentum flowing in through the surface. The mechanical momentum must be the total of these two. This equation expresses conservation of momentum due to electromagnetic forces: if momentum "enters" through the surface, then the total "stored" momentum must increase.

Just like in Poynting's theorem, it is interesting to express the same statement using a density instead, in this case the momentum density g\mathbf{g}. Dividing the field momentum by volume we get

g=ε0μ0S=ε0(E×B)\boxed{\mathbf{g}=\varepsilon_{0}\mu_{0}\mathbf{S}=\varepsilon_{0}(\mathbf{E}\times \mathbf{B})}

Meanwhile, the momentum flux transported by the fields must be T-T.

If we keep the mechanical momentum static, such as when we are in empty space, the time derivative vanishes and we can rearrange the conservation law to read

gt=T\frac{\partial \mathbf{g}}{\partial t}=\nabla\cdot \mathrm{T}

This is the momentum continuity equation for electrodynamics. Just like with energy and electric charge, individual charges and their fields constantly exchange momentum, with the total momentum being conserved.

Conservation of angular momentum

Just like how fields carry angular momentum, they also carry angular momentum. By definition L=r×p\mathbf{L}=\mathbf{r}\times \mathbf{p}, so the angular momentum density \boldsymbol{\ell} must be

=r×g=ε0[r×(E×B)]\boxed{\boldsymbol{\ell}=\mathbf{r}\times \mathbf{g}=\varepsilon_{0}[\mathbf{r}\times(\mathbf{E}\times \mathbf{B})]}

This is interpreted in the same way as above: it's not just charges that induce an angular momentum, fields themselves also carry it and this amount is mandatory for the conservation law to be upheld.

Relativity

The Lorentz force has a relativistic expression as a Minkowski force in spacetime caused by the electromagnetic tensor FμνF^{\mu \nu}. A charge qq moving at proper velocity ημ=(γc,v)\eta^{\mu}=(\gamma c,\mathbf{v}) will be subject to a relativistic Lorentz force

Kμ=qηνFμν\boxed{K^{\mu}=q\eta_{\nu}F^{\mu \nu}} > Thus, with the other two components we get > $$\mathbf{K}=\frac{q}{\sqrt{ 1-v^{2}/c^{2} }}[\mathbf{E}+(\mathbf{v}\times \mathbf{B})]=\gamma q[\mathbf{E}+(\mathbf{v}\times \mathbf{B})]

and since the spatial components of a Minkowski force are related to the ordinary force by K=γF\mathbf{K}=\gamma\mathbf{F} we get