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Calculus- Early Transcendentals, 2021a

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552 Vector <strong>Calculus</strong><br />

16.5 The Divergence Theorem<br />

The third version of Green’s Theorem (Equation 16.3)wesawwas:<br />

∫<br />

∫∫<br />

f · Nds = ∇ · fdA.<br />

With minor changes this turns into another equation, the Divergence Theorem:<br />

Theorem 16.15: Divergence Theorem<br />

∂D<br />

Under suitable conditions, if E is a region of three dimensional space and D is its boundary surface,<br />

oriented outward, then<br />

∫∫<br />

∫∫∫<br />

f · NdS = ∇ · fdV .<br />

D<br />

D<br />

E<br />

Proof. Again this theorem is too difficult to prove here, but a special case is easier. In the proof of a<br />

special case of Green’s Theorem, we needed to know that we could describe the region of integration in<br />

both possible orders, so that we could set up one double integral using dxdy and another using dydx.<br />

Similarly here, we need to be able to describe the three-dimensional region E in different ways.<br />

We start by rewriting the triple integral:<br />

∫∫∫<br />

E<br />

∫∫∫<br />

∇ · fdV =<br />

E<br />

The double integral may be rewritten:<br />

∫∫<br />

∫∫<br />

∫∫<br />

f · NdS = ( f 1 i + f 2 j + f 3 k) · NdS =<br />

D<br />

D<br />

( ∂ f 1<br />

∂x + ∂ f 2<br />

∂y + ∂ f 3<br />

∂z<br />

∫∫∫E<br />

)dV = ∂ f 1<br />

∂x<br />

∫∫∫E<br />

dV + ∂ f 2<br />

∂y<br />

∫∫∫E<br />

dV + ∂ f 3<br />

∂z dV .<br />

D<br />

∫∫<br />

∫∫<br />

f 1 i · NdS+ f 2 j · NdS+ f 3 k · NdS.<br />

D<br />

D<br />

To prove that these give the same value it is sufficient to prove that<br />

∫∫<br />

∫∫∫<br />

∂ f 1<br />

f 1 i · NdS = dV , (16.4)<br />

D<br />

E ∂x<br />

∫∫<br />

∫∫∫<br />

∂ f 2<br />

f 2 j · NdS = dV , and (16.5)<br />

D<br />

E ∂y<br />

∫∫<br />

∫∫∫<br />

∂ f 3<br />

f 3 k · NdS = dV . (16.6)<br />

D<br />

E ∂z<br />

Not surprisingly, these are all pretty much the same; we’ll do the first one.<br />

We set the triple integral up with dx innermost:<br />

∫∫∫<br />

E<br />

∫<br />

∂ f g2 1<br />

∂x<br />

∫∫B<br />

dV = (y,z) ∂ f 1<br />

g 1 (y,z) ∂x<br />

∫∫B<br />

dxdA = f 1 (g 2 (y,z),y,z) − f 1 (g 1 (y,z),y,z)dA,<br />

where B is the region in the yz-plane over which we integrate. The boundary surface of E consists of a<br />

“top” x = g 2 (y,z), a “bottom” x = g 1 (y,z), and a “wrap-around side” that is vertical to the yz-plane. To

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