Introduction
The concept of a discrete body sets aside the notion of a continuum to establish the conservation laws of Mechanics. All of the theorems and mathematical properties are applied directly to objects of finite dimensions. Discrete Mechanics essentially takes elementary results from differential geometry to establish the laws of conservation along an edge. The Fundamental Law of Dynamics is the starting point for establishing the conservation of momentum equation.
A certain number of the concepts used in Continuum Mechanics will be abandoned; thus, the very notion of a continuum is not necessary in order to obtain discrete equations. Similarly, the hypothesis of Local Thermodynamic Equilibrium is set aside, because within the elementary volume, it is not necessary for a state equation to be satisfied. The concept of a tensor is replaced by the concepts of differential geometry and elementary operators, gradient, rotational and divergence, using which we are able to establish the link between single-point values, oriented vectors, oriented surfaces and volumes, and vice versa. Similarly, the projection onto an orthonormal axis system is not necessary to establish the conservation equations.
Although this formalism gives us a momentum balance equation which is different to the Navier–Stokes equation, their application to simple flows yields identical results. The Hodge–Helmholtz decomposition will play an essential role in showing how the momentum balance equation can be employed to separate any of the terms in this equation into a solenoidal part and an irrotational part.
In Fluid Mechanics, the pressure in the momentum balance equation cannot be reduced to the role of mechanical pressure. This equation represents an instantaneous equilibrium and the thermodynamic pressure, which plays the role of a stress accumulator, depends not only on properties such as the temperature or density, but also on the heat flux and the velocity. If we limit our discussion to mechanical and thermal effects, the role of the divergences of the flux and velocity in reading the thermodynamic pressure will become apparent.
The elements deriving from differential geometry, differential algebra, exterior calculus, and so on, will be omitted in the interests of a presentation which is as simple as possible, using the classic theorems such as those of Ostrogradski and Stokes, etc., and the properties of the standard differential operators.
The laws of conservation in mechanics were established over two centuries ago, and have evolved very little since. The important contributions made by C. Truesdell and W. Noll [TRU 74, TRU 92] to integrate the laws of thermodynamics and the constitutive laws into the conservation of momentum- and energy laws, however, led to the establishment of the Navier–Stokes equations, which offer a very accurate representation of the physical reality of the phenomena being observed. Many more important contributions have helped construct the corpus of equations in Continuum Mechanics as it is taught today [LAN 59, BAT 67, SAL 02, GER 95, COI 07, GUY 91].
However, there are a certain number of difficulties inherent to the continuum theory which need to be taken into consideration:
The continuum formalism is essentially linked to the relations between stresses and strains (also known as deformations), which are represented by a stress tensor, of varying degrees of complexity. The most complete tensors, such as the Green–Lagrange tensor, enable us to take account of significant deformations, whilst certain tensors found by linearization, such as the Cauchy tensor, are limited to small transformations. The displacement field gradient thus introduces the notion of a tensor which can be decomposed into symmetric and antisymmetric parts. The purpose of this operation is to filter out the rigid translational motion which does not give rise to any force within the material.
The issue that we tackle in the area of Discrete Mechanics is based on the laying aside of the idea of a continuum, where all the scalar and vectorial variables are defined at a single point. In a discrete medium, the scalar values are associated with a point, whereas the vectorial values are defined on an edge which can be as short as it needs to be, provided its direction is preserved. To begin with, we shall work in the context of small displacements, and in order to counter the disadvantages that come with that approach, we shall introduce the principle of accumulation, whereby each equilbrium state is conserved so as to represent the evolution of the physical system.
There are a certain number of principles which seem indispensable in order to model all the mechanical effects:
The theory taking shape in this book is founded upon the fundamental law of dynamics and on some elementary experiments, using these as bases upon which to construct coherent and balanced models of the observed effects – in particular the diffusion of momentum and the propagation of waves. It also draws on certain elements which were established in a previous publication by this author on the subject [CAL 01] to specify and supplement the derivation of the scalar and vectorial conservation equations without using tensors whose order is equal to or higher than two.
Next, we go on to discuss the general properties of these equations. In particular, the differences between the Navier–Stokes equation and the momentum balance equation stemming from this theory will be illustrated; also, the two forms of the dissipation term will be compared.