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Zienkiewicz O.C., Taylor R.L. Vol. 3. The finite - tiera.ru

Zienkiewicz O.C., Taylor R.L. Vol. 3. The finite - tiera.ru

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92 Incompressible laminar ¯ow<br />

Conservation of momentum<br />

@U i<br />

@t<br />

@<br />

ˆÿ …u<br />

@x<br />

jUi†‡ j<br />

@ ij<br />

ÿ<br />

@xj @p<br />

ÿ gi @xi In the above we de®ne the mass ¯ow ¯uxes as<br />

…4:2†<br />

U i ˆ u i …4:3†<br />

Conservation of energy is now uncoupled and can be solved independently:<br />

@… E†<br />

@t<br />

@<br />

ˆÿ …uj E†‡<br />

@xj @<br />

@xi k @T<br />

@x i<br />

ÿ @<br />

…u<br />

@x<br />

jp†‡<br />

j<br />

@<br />

…<br />

@x<br />

ijuj† …4:4†<br />

i<br />

In the above u i are the velocity components; E is the speci®c energy (c vT), p is the<br />

pressure, T is the absolute temperature, g i represents the body force and other<br />

source terms, and ij are the deviatoric stress components given by (Eq. 1.12b).<br />

ij ˆ<br />

@ui ‡<br />

@xj @uj ÿ<br />

@xi 2<br />

3 ij<br />

@uk @xk …4:5†<br />

With the substitution made for density changes we note that the essential variables<br />

in the ®rst two equations become those of pressure and velocity. In exactly the same<br />

way as these, we can specify the variables linking displacements and pressure in the<br />

case of incompressible solids. It is thus possible to solve these equations in one of<br />

many ways described in Chapter 12 of <strong>Vol</strong>ume 1 though, of course, the use of the<br />

CBS algorithm is obvious.<br />

Unless the viscosity and in fact the bulk modulus have a strong dependence on<br />

temperature the problem is very weakly linked with the energy equation which can<br />

be solved independently.<br />

<strong>The</strong> energy equation for incompressible materials is best written in terms of the absolute<br />

temperature T avoiding the speci®c energy. <strong>The</strong> equation now becomes simply<br />

c v<br />

@T<br />

@t ‡ u @T<br />

j<br />

@x j<br />

ˆ @<br />

@x i<br />

k @T<br />

@x i<br />

‡ @<br />

…<br />

@x<br />

ijuj†ÿ i<br />

@<br />

…u<br />

@x<br />

jp† …4:6†<br />

j<br />

and we note that this is now a scalar convection±di€usion equation of the type we<br />

have already encountered in Chapter 2, written in terms of the variable temperature<br />

as the unknown. In the above equation, the last two work dissipation terms are<br />

often neglected for fully incompressible ¯ows. Note that the above equation is<br />

derived assuming the density and c v (speci®c heat at constant volume) to be<br />

constants.<br />

In this chapter we shall in general deal with problems for which the coupling is<br />

weak and the temperature equations do not present any di culties. However in<br />

Chapter 5 we shall deal with buoyancy e€ects causing atmospheric or general circulation<br />

induced by small density changes induced by temperature di€erences.<br />

If viscosity is a function of temperature, it is very often best to proceed simply by<br />

iterating over a cycle in which the velocity and pressure are solved with the assumption<br />

of known viscosity and that is followed by the solution of temperature. Many<br />

practical problems have been so solved very satisfactorily. We shall show some of<br />

these applications in the ®eld of material forming later on in this chapter.

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