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CONTINUUM MECHANICS for ENGINEERS

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where dx i is a differential tangent vector along the streamline. This is the<br />

well-known Bernoulli equation. If the motion is steady, the time function G(t)<br />

resulting from the integration reduces to a constant G, which may vary from<br />

one streamline to another. Furthermore, if the flow is also irrotational, a<br />

unique constant G 0 is valid throughout the flow.<br />

When gravity is the only <strong>for</strong>ce acting on the body, we write Ω = gh where<br />

g = 9.81 m/s 2 is the gravitational constant and h is a measure of the height<br />

above a reference level in the fluid. If h p = P/g is defined as the pressure head<br />

and h v = v 2 /2g as the velocity head, Bernoulli’s equation <strong>for</strong> incompressible<br />

fluids becomes<br />

(7.5-3)<br />

Recall that by Eq 2.8-5 in Chapter Two we introduced Stoke’s theorem,<br />

which relates the line integral around a closed curve to the surface integral<br />

over its cap. By this theorem we define the velocity circulation Γ c around a<br />

closed path in the fluid as<br />

(7.5-4)<br />

where n i is the unit normal to the surface S bounded by C and dx i is the<br />

differential tangent element to the curve C. Note that, when the flow is<br />

irrotational, curl v = 0 and the circulation vanishes. If we take the material<br />

derivative of the circulation by applying Eq 5.2-7 to Eq 7.5-4 we obtain<br />

(7.5-5)<br />

For a barotropic, inviscid fluid with conservative body <strong>for</strong>ces, this integral<br />

may be shown to vanish, leading to what is known as Kelvin’s theorem of<br />

constant circulation.<br />

Problems<br />

p v<br />

h h h h<br />

g g G<br />

2<br />

+ p + v = + + =<br />

ρ 2<br />

= vdx = v ndS ∫ ∫<br />

Γc i i εijk<br />

k,j i<br />

S<br />

∫<br />

( )<br />

˙ = vdx ˙ + vdv<br />

Γ c i i i i<br />

7.1 Introduce the stress deviator S ij and the viscous stress deviator<br />

1<br />

Tij = τij − δ τ<br />

into Eq 7.1-5 to prove that =<br />

.<br />

3 ij kk Sij Tij<br />

0

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