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Conservation of Momentum in Electrodynamics 📂Electrodynamics

Conservation of Momentum in Electrodynamics

Overview1

In electrodynamics, the law of conservation of momentum is as follows.

dpdt=ϵ0μ0ddtVSdτ+STda \dfrac{d \mathbf{p}}{dt} =-\epsilon_{0}\mu_{0}\dfrac{d}{dt}\int_{\mathcal{V}} \mathbf{S} d\tau + \oint_{\mathcal{S}} \mathbf{T} \cdot d\mathbf{a}

Explanation

According to Newton’s second law, the force acting on an object and the change in the object’s momentum are equal.

F=dpdt \mathbf{F} = \dfrac{d \mathbf{p}}{dt}

p\mathbf{p} is the total mechanical momentum of particles within volume V\mathcal{V}. To distinguish it from the momentum stored in the electromagnetic field, we’ll refer to p\mathbf{p} as ‘mechanical’ momentum. The electromagnetic force acting on the charge within the volume is as follows.

F=STdaϵ0μ0ddtVSdτ \mathbf{F} =\oint_{\mathcal{S}} \mathbf{T} \cdot d\mathbf{a} -\epsilon_{0}\mu_{0}\dfrac{d}{dt}\int_{\mathcal{V}} \mathbf{S} d\tau

Therefore,

dpdt=ϵ0μ0ddtVSdτ+STda \dfrac{d \mathbf{p}}{dt} =-\epsilon_{0}\mu_{0}\dfrac{d}{dt}\int_{\mathcal{V}} \mathbf{S} d\tau + \oint_{\mathcal{S}} \mathbf{T} \cdot d\mathbf{a}

This equation is the law of conservation of momentum in electrodynamics. Since its form is similar to the Poynting’s theorem, it can be understood in a similar way.

The first integral on the right-hand side represents the momentum stored in the electromagnetic field within volume V\mathcal{V}. In other words, ϵ0μ0S\epsilon_{0} \mu_{0} \mathbf{S} represents the momentum density of the electromagnetic field in unit volume space; simply put, it’s the momentum density of the field. This is expressed as follows.

g=ϵ0μ0S=ϵ0E×B \mathbf{g} =\epsilon_{0} \mu_{0} \mathbf{S} = \epsilon_{0} \mathbf{E}\times\mathbf{B}

The second integral on the right-hand side represents the momentum flowing into the surface (boundary) S\mathcal{S} enveloping volume V\mathcal{V} per unit time. Therefore, if the mechanical momentum p\mathbf{p} increases, it means either the momentum stored in the field is decreasing, or momentum is being carried into the field through the boundary surface. When mechanical momentum within volume V\mathcal{V} does not change over time, as in a vacuum,

0=Vgtdτ+STda    Vgtdτ=STda=VTdτ \begin{align*} && 0 &= - \int_{\mathcal{V}} \dfrac{\partial \mathbf{g}}{\partial t} d\tau + \oint_{\mathcal{S}} \mathbf{T}\cdot d\mathbf{a} \\ \implies && \quad \int_{\mathcal{V}} \dfrac{\partial \mathbf{g}}{\partial t} d\tau &= \oint_{\mathcal{S}} \mathbf{T}\cdot d\mathbf{a}=\int_{\mathcal{V}} \nabla \cdot \mathbf{T} d\tau \end{align*}

The second bracket in the second line is valid due to the divergence theorem. From the above result, the following equation is valid.

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

The above equation is the continuity equation for electromagnetic momentum. g\mathbf{g} and ρ\rho serve similar roles, as do T-\mathbf{T} and J\mathbf{J}. This implies that electromagnetic momentum is locally conserved, but not generally. Since charges and the electromagnetic field exchange momentum, the total momentum of both is conserved; in other words, the combined momentum of matter and the electromagnetic field is preserved.


  1. David J. Griffiths, 기초전자기학(Introduction to Electrodynamics, 김진승 역) (4th Edition1 2014), p393-394 ↩︎