Physical Interpretations

Chapter 5: Integral Theorems of Vector Calculus

Learning objectives

  • Read divergence as net source density and curl as local angular velocity
  • Derive Maxwell's integral equations from their differential forms via the integral theorems
  • Translate conservation principles in physics into integral-theorem statements
Stokes Flux DemoInteractive figure — enable JavaScript to interact.

The integral theorems are not computational shortcuts; they are statements of conservation written in coordinates. Every continuum physics equation you will encounter — mass, momentum, energy, charge, vorticity — has the same shape: rate of change of a quantity inside a region equals net flux through the boundary plus sources inside. The Divergence Theorem and Stokes' Theorem are how that shape gets cashed out in R3\mathbb{R}^3. Once you can read them as conservation statements, you have learned the dialect of mathematical physics.

Divergence as source density

Imagine F\mathbf{F} as the velocity field of a fluid times its density — the mass-flux density. At a point pp, take a tiny box of volume ΔV\Delta V centred at pp. The net outward flux through the box's surface is approximately

boxFdS    (F)(p)ΔV.\iint_{\partial \text{box}} \mathbf{F}\cdot d\mathbf{S} \;\approx\; (\nabla\cdot\mathbf{F})(p)\cdot \Delta V.

Dividing by ΔV\Delta V and taking the limit: F\nabla\cdot\mathbf{F} at pp is the net outflow per unit volume. If the flow models matter, this is the rate at which matter is created per unit volume at pp. Positive: source. Negative: sink. Zero: no creation or destruction. Integrating gives the Divergence Theorem.

Curl as local rotation

Drop an infinitesimal paddle wheel at a point in the flow F\mathbf{F}. Its angular velocity vector ω\boldsymbol{\omega} satisfies ω=12×F\boldsymbol{\omega} = \tfrac{1}{2}\nabla\times\mathbf{F}. The curl's direction is the rotation axis (by the right-hand rule); its magnitude is twice the angular speed. A rigid rotation F=Ω×r\mathbf{F} = \boldsymbol{\Omega}\times\mathbf{r} at angular velocity Ω\boldsymbol{\Omega} has ×F=2Ω\nabla\times\mathbf{F} = 2\boldsymbol{\Omega} everywhere — consistent.

Maxwell's equations in integral form

Maxwell's differential equations in vacuum are

E=ρ/ε0\nabla\cdot\mathbf{E} = \rho/\varepsilon_0
B=0\nabla\cdot\mathbf{B} = 0
×E=B/t\nabla\times\mathbf{E} = -\partial\mathbf{B}/\partial t
×B=μ0J+μ0ε0E/t\nabla\times\mathbf{B} = \mu_0\mathbf{J} + \mu_0\varepsilon_0\, \partial\mathbf{E}/\partial t

Apply the Divergence Theorem to the first two and Stokes' Theorem to the last two. You get the four integral-form Maxwell equations:

  • Gauss's law: VEdS=Qenc/ε0\iint_{\partial V}\mathbf{E}\cdot d\mathbf{S} = Q_{\text{enc}}/\varepsilon_0.
  • No magnetic monopoles: VBdS=0\iint_{\partial V}\mathbf{B}\cdot d\mathbf{S} = 0.
  • Faraday's law: SEdr=ddtSBdS\oint_{\partial S}\mathbf{E}\cdot d\mathbf{r} = -\dfrac{d}{dt}\iint_S \mathbf{B}\cdot d\mathbf{S}.
  • Ampère's law (with Maxwell's correction): SBdr=μ0Ienc+μ0ε0ddtSEdS\oint_{\partial S}\mathbf{B}\cdot d\mathbf{r} = \mu_0 I_{\text{enc}} + \mu_0\varepsilon_0\dfrac{d}{dt}\iint_S\mathbf{E}\cdot d\mathbf{S}.

The differential and integral forms are equivalent; the integral theorems are the bridge. Both are used in practice — differential for local PDEs, integral for symmetry arguments.

The general pattern

For any conserved quantity with density ρ\rho and flux J\mathbf{J}, conservation is

ρt+J=σ,\dfrac{\partial\rho}{\partial t} + \nabla\cdot\mathbf{J} = \sigma,

where σ\sigma is the source density. Integrating over a fixed region VV and applying the Divergence Theorem:

ddtVρdV+VJdS=VσdV.\dfrac{d}{dt}\iiint_V \rho\,dV + \iint_{\partial V}\mathbf{J}\cdot d\mathbf{S} = \iiint_V \sigma\,dV.

Mass, momentum, energy, charge, and probability (in quantum mechanics) all obey this. Memorise this template and you have the structure of most continuum physics.

(These interpretations are inherently 3D and hard to visualise with our 2D lang-core widgets — the references include excellent 3D vector-field demos.)

Pause and think: The continuity equation ρ/t+J=0\partial\rho/\partial t + \nabla\cdot\mathbf{J} = 0 says no sources or sinks. If you integrate over a region VV, what does the resulting integral statement say about the rate of change of total mass inside VV?

Try it

  • For a uniform fluid velocity F=(c,0,0)\mathbf{F}=(c,0,0) with constant cc, predict F\nabla\cdot\mathbf{F}. Then verify and interpret physically.
  • For a rigid rotation F=(y,x,0)\mathbf{F}=(-y, x, 0) at angular speed 11 about the zz-axis, compute ×F\nabla\times\mathbf{F}. Confirm it gives 2Ω2\boldsymbol{\Omega}.
  • Use Gauss's law to find the electric field of a uniformly charged sphere of radius RR and total charge QQ, at a point outside the sphere. (Hint: choose a Gaussian sphere of radius r>Rr > R.)
  • True or false: "flux through a closed surface is zero" is equivalent to "divergence is zero everywhere inside." Why does the equivalence need a smooth region?

A trap to watch for

Confusing the curl direction with the flow direction. Curl is perpendicular to the plane of rotation, NOT in the direction of motion. For F=(y,x,0)\mathbf{F}=(-y, x, 0) (a flow in the xyxy-plane), the curl is (0,0,2)(0,0,2) in the zz-direction. Beginners sometimes mark the curl as horizontal because the flow is horizontal — this confuses the rotational axis with the rotation.

What you now know

You can interpret divergence and curl physically, derive the integral-form Maxwell equations, and recognise the universal conservation template. Section 5.5 sketches the proofs and connects these classical theorems to the generalised Stokes' Theorem of chapter 6.

References

  • Garrity, T. (2002). All the Mathematics You Missed. Cambridge University Press, ch. 5.
  • Griffiths, D. J. (2017). Introduction to Electrodynamics (4th ed.). Cambridge UP — all of Maxwell's equations.
  • Schey, H. M. (2004). Div, Grad, Curl, and All That (4th ed.). W. W. Norton.
  • Marsden, J. E., Tromba, A. J. (2011). Vector Calculus (6th ed.). W. H. Freeman.
  • Feynman, R. P. (1964). The Feynman Lectures on Physics, Vol. II, ch. 2-3 (vector fields).

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