# Introduction to Mathematical Physics/Energy in continuous media/Generalized elasticity

## Introduction[edit]

In this section, the concept of elastic energy is presented. \index{elasticity} The notion of elastic energy allows to deduce easily "strains--deformations" relations.\index{strain--deformation relation} So, in modelization of matter by virtual powers method \index{virtual powers} a power that is a functional of displacement is introduced. Consider in particular case of a mass attached to a spring of constant .*Deformation* of the system is referenced by the elongation of the spring with respect to equilibrium. The *virtual work* \index{virtual work} associated to a displacement is

deltWfdx

Quantity represents the *constraint* , here a force, and is the deformation. If force is conservative, then it is known that the elementary work (provided by the exterior) is the total differential of a potential energy function or *internal energy* :

eqdeltaWdU

In general, force depends on the deformation. Relation is thus a *constraint--deformation relation* .

The most natural way to find the strain-deformation relation is the following. One looks for the expression of as a function of the deformations using the physics of the the problem and symmetries. In the particular case of an oscillator, the internal energy has to depend only on the distance to equilibrium position. If admits an expansion at , in the neighbourhood of the equilibrium position can be approximated by:

As is an equilibrium position, we have at . That implies that is zero. Curve at the neighbourhood of equilibrium has thus a parabolic shape (see figure figparabe

figparabe

As

the strain--deformation relation becomes:

## Oscillators chains[edit]

Consider a unidimensional chain of oscillators coupled by springs of constant . this system is represented at figure figchaineosc. Each oscillator is referenced by its difference position with respect to equilibrium position. A calculation using the Newton's law of motion implies:

figchaineosc

A calculation using virtual powers principle would have consisted in affirming: The total elastic potential energy is in general a function x_i</math> to the equilibrium positions. This differential is total since force is conservative\footnote{ This assumption is the most difficult to prove in the theories on elasticity as it will be shown at next section} . So, at equilibrium: \index{equilibrium} :

If admits a Taylor expansion:

eqdevliUch

In this last equation, repeated index summing convention as been used. Defining the differential of the intern energy as:

one obtains

Using expression of provided by equation eqdevliUch yields to:

But here, as the interaction occurs only between nearest neighbours, variables are not the right thermodynamical variables. let us choose as thermodynamical variables the variables defined by:

Differential of becomes:

Assuming that admits a Taylor expansion around the equilibrium position:

and that at equilibrium, yields to:

As the interaction occurs only between nearest neighbours:

so:

This does correspond to the expression of the force applied to mass :

if one sets .

secmaterelast

## Tridimensional elastic material[edit]

Consider a system in a state which is a deformation from the state . Each particle position is referenced by a vector in the state and by the vector in the state :

Vector represents the deformation.

**Remark:**

Such a model allows to describe for instance fluids and solids.

Consider the case where is always "small". Such an hypothesis is called small perturbations hypothesis (SPH). The intern energy is looked as a function .

**Definition:** The deformation tensor SPH is the symmetric part of the tensor gradient of .

At section secpuisvirtu it has been seen that the power of the admissible intern strains for the problem considered here is:

with

Tensor is called rate of deformation tensor. It is the symmetric part of tensor . It can be shown [ph:fluid:Germain80] that in the frame of SPH hypothesis, the rate of deformation tensor is simply the time derivative of SPH deformation tensor:

Thus:

dukij

Function can thus be considered as a function . More precisely, one looks for that can be written:

where is an internal energy density with\footnote{ Function depends only on .} whose Taylor expansion around the equilibrium position is:

eqrhoel

We have\footnote{

footdensi

Indeed:

and from the properties of the particulaire derivative:

Now,

From the mass conservation law:

}

eqdudt

Thus

Using expression eqrhoel of and assuming that is zero at equilibrium, we have:

thus:

with . Identification with equation dukij, yields to the following strain--deformation relation:

it is a generalized Hooke law\index{Hooke law}. The 's are the elasticity coefficients.

**Remark:** Calculation of the footnote footdensi show that calculations done at previous section secchampdslamat should deal with volumic energy densities.

secenernema

## Nematic material[edit]

A nematic material\index{nematic} is a material [ph:liqcr:DeGennes74] whose state can be defined by vector field\footnote{ State of smectic materials can be defined by a function . } . This field is related to the orientation of the molecules in the material (see figure figchampnema)

figchampnema

Let us look for an internal energy that depends on the gradients of the field:

with

The most general form of for a linear dependence on the derivatives is:

eqsansder

where is a second order tensor depending on . Let us consider how symmetries can simplify this last form.

*Rotation invariance.*Functional should be rotation invariant.

where are orthogonal transformations (rotations). We thus have the condition:

that is, tensor has to be isotrope. It is know that the only second order isotrope tensor in a three dimensional space is , that is the identity. So could always be written like:

*Invariance under the transformation maps to*. The energy of distortion is independent on the sense of , that is . This implies that the constant in the previous equation is zero.

Thus, there is no possible energy that has the form given by equation eqsansder. This yields to consider next possible term . general form for is:

Let us consider how symmetries can simplify this last form.

*Invariance under the transformation maps to*. This invariance condition is well fulfilled by .*Rotation invariance.*The rotation invariance condition implies that:

It is known that there does not exist any third order isotrope tensor in , but there exist a third order isotrope pseudo tensor: the signature pseudo tensor (see appendix secformultens). This yields to the expression:

- {\bf Invariance of the energy with respect to the axis transformation , , .} The energy of nematic crystals has this invariance property\footnote{ Cholesteric crystal doesn't verify this condition.} . Since is a pseudo-tensor it changes its signs for such transformation.

There are thus no term in the expression of the internal energy for a nematic crystal. Using similar argumentation, it can be shown that can always be written:

and :

Limiting the development of the density energy to second order partial derivatives of yields thus to the expression: