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Physics LibreTexts

1.8: Flux

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The product of electric field intensity and area is the flux \Phi_E. Whereas E is an intensive quantity, \Phi_E is an extensive quantity. It dimensions are ML3T-2Q-1 and its SI units are N m2 C-1, although later on, after we have met the unit called the volt, we shall prefer to express \Phi_E in V m.

With increasing degrees of sophistication, flux may be defined mathematically as:

\Phi_E = EA

I.4A.png
\text{FIGURE I.4}: Flow that is perpendicular to the surface.

\Phi_E = EA \cos \theta = \textbf{E} \cdot \textbf{A}
I.5a.png

\text{FIGURE I.5}: Flow that is at an angle to the surface.

Note that \textbf{E} is a vector, but \Phi_E is a scalar.

\Phi_E = \iint \textbf{E} \cdot d\textbf{A}

I.6a.png
\text{FIGURE I.6}

We can also define a D-flux by

\Phi_D=\iint \textbf{D}\cdot d\textbf{A}.

The dimensions of \Phi_D are just Q and the SI units are coulombs (C).

An example is in order:

I.7.png
\text{FIGURE I.7}

Consider a square of side 2a in the xy-plane as shown. Suppose there is a positive charge Q at a height a on the z-axis. Calculate the total D-flux, \Phi_D through the area.

Consider an elemental area dxdy at (x,\, y ,\, 0). Its distance from Q is (a^2+x^2+y^2)^{1/2} so the magnitude of the D-field there is \frac{Q}{4\pi}\cdot \frac{1}{a^2+x^2+y^2}. The scalar product of this with the area is \frac{Q}{4\pi}\cdot \frac{1}{a^2+x^2+y^2}\cdot \cos \theta dxdy,\text{ and }\cos \theta = \frac{a}{(a^2+x^2+y^2)^{1/2}}. The surface integral of \textbf{D} over the whole area is

\label{1.8.1}\iint D\cdot dA=\frac{Qa}{\pi}\int_0^a \int_0^a \frac{dxdy}{(a^2+x^2+y^2)^{3/2}}.

Now all we have to do is the nice and easy integral. Let x=\sqrt{a^2+y^2}\tan ψ and the inner integral \int_0^a \frac{dx}{(a^2+x^2+y^2)^{3/2}} reduces, after some modest algebra, to \frac{a}{(a^2+y^2)\sqrt{2a^2+y^2}}. Thus we now have

\label{1.8.2}\iint D\cdot dA = \frac{Qa^2}{\pi}\int_0^a \frac{dy}{(a^2+y^2)\sqrt{2a^2+y^2}}.

With the further substitution a^2+y^2=a^2 \sec \omega this reduces, after more careful algebra, to

\iint D\cdot dA=\frac{Q}{6}.\label{1.8.3}

Two additional examples of calculating surface integrals may be found in Section 5.6, of the Celestial Mechanics section of these notes. These deal with gravitational fields, but they are essentially the same as the electrostatic case; just substitute Q for m and -1/(4\pi \epsilon) for G.

I urge readers actually to go through the pain and the algebra and the trigonometry of these three examples in order that they may appreciate all the more, in the next section, the power of Gauss’s theorem.


This page titled 1.8: Flux is shared under a CC BY-NC 4.0 license and was authored, remixed, and/or curated by Jeremy Tatum via source content that was edited to the style and standards of the LibreTexts platform.

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