Introduction to Mathematical Physics/Energy in continuous media/Introduction

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The first principle of thermodynamics (see section secpremierprinci) allows to bind the internal energy variation to the internal strains power \index{strains}: Template:IMP/eq if the heat flow is assumed to be zero, the internal energy variation is: Template:IMP/eq This relation allows to bind mechanical strains (Pi term) to system's thermodynamical properties (dU term). When modelizing a system some "thermodynamical" variables X are chosen. They can be scalars x, vectors xi, tensors xij, \dots Differential dU can be naturally expressed using those thermodynamical variables X by using a relation that can be symbolically written: Template:IMP/eq where F is the conjugated\footnote{ This is the same duality relation noticed between strains and speeds and their gradients when dealing with powers.}

thermodynamical variable of variable

X. In general it is looked for expressing F as a function of X . Template:IMP/rem Template:IMP/rem Template:IMP/rem The next step is, using physical arguments, to find an {\bf expression of the internal energy U(X)} \index{internal energy} as a function of thermodynamical variables X. Relation F(X) is obtained by differentiating U with respect to X, symbolically: Template:IMP/eq In this chapter several examples of this modelization approach are presented.

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