PART 1
Fundamentals
Chapter 1
Interfaces: the Physics, Chemistry and Mechanics of Heterogeneous Continua
Of what does an interface between two solids consist? What qualifying or quantitative physical or chemical parameters must we specify to define it? What general considerations can we set out about the mechanical behavior of an interface in a heterogeneous solid? These are the basic questions that this chapter proposes to answer as an introduction to the following chapters, focusing on more specific points.
1.1. Definition and terminology
Strictly speaking, an interface can be defined as the two-dimensional border area between two dissimilar materials. These two materials may differ in their physical state (such as in the case of solidâliquid or solidâgas interfaces); their chemical composition (such as an interface between two immiscible liquids in an emulsion); their structure (such as a residual martensite/austenite interface in quenched steel); their relative orientation (such as the twin boundaries or grain boundaries in a polycrystal or the interface between layers in a multilayer composite); or even by their relative translation (such as a stacking fault surface in a crystal). In this book, as the title indicates, we will focus on the case of interfaces between two solid materials.
The geometric aspect of a solidâsolid interface can prove extremely variable, depending on the scale at which it is observed. Abrupt interfaces, in which the physical and chemical characteristics change suddenly as the interface is crossed (see Figure 1.1a), are an ideal and simple case that is rarely encountered in reality. In real cases, the physical or chemical interaction between the two materials disturbs their composition or their structure in a layer of varying thickness near the interface, producing what we call a diffuse interface, with or without a marked discontinuity of properties (see Figures 1.1b and 1.1c).
This heterogeneity may even appear as a complex interpenetration of particles or protrusions of adjacent materials (see Figure 1.1d). Finally, the interface may have one or more intermediate layers, or interphases, composed of material that is different from the join between two bulk materials that have either been inserted voluntarily during the development of a synthesis interface (for example, a layer of adhesive in a glued interface) or are the result of a solid state reaction between the two basic materials (see Figure 1.1e and Chapter 5).
Even without taking a closer look at the crystalline or atomic scale (see Chapter 2), it is clear that a real interface almost always has some âthicknessâ; the ideal notion of an interface reduced to a surface of abrupt separation between two solid media, such as the one in Figure 1.1a, is in reality only a convenient, simplified assumption that is frequently used, keeping in mind that it is only valid on a scale of sufficient width.
1.2. Energy considerations
On the free surface of a solid, or along an internal interface, the interaction stresses acting on an atom or molecule due to its bonds with its neighbors are obviously different from the ones in the bulk of the same solid; since the local atomic environment is neither homogeneous nor isotropic, the result of these interactions is not zero and leads, for example, to atomic reconstructions on the surface or to interatomic distances with equilibrium values that are different from those in the bulk of the material. The same is true for electronic distributions. In the case of the free surface of a homogeneous solid, the result is an increase in internal energy Îłs in the free surface area (in J/mÂČ) in comparison with any surface embedded within the volume of the solid. This surface energy Îł includes an enthalpy contribution due to the local chemical composition, which is different from that within the solid, and an entropy contribution related to the difference in atomic structure between the surface and the volume of the solid. In the case of an interface between two media A and B, for similar reasons each unit of area of the interface represents additional internal energy ÎłI, the value of which can be expressed by the DuprĂ© relation (see Chapter 5):
where ÎłA and ÎłB are the energies of the surfaces of materials A and B when they are free and ÎłAB represents the energy of the interatomic bonds per unit of interface area established between the two materials at the moment when the interface is produced. This energy is usually negative (with the usual conventions of thermodynamics); that is, the side-by-side placement of the two free surfaces leads to a reduction in internal energy, and the interface thus created is more stable than the two separate elements. Its value, on the basis of both theoretical considerations and experimental results, in typically on the order of 1 J/mÂČ.
Returning to the case of the total free area of a solid, where the formulation of a physical demonstration is simpler, two different types of variations can be imagined for its total energy, Ws:
â with the extent of area A of the free surface of interest, at constant interatomic distances (the strain Δ being constant) we have:
which leads to the definition of the surface energy Îłs mentioned above;
â with the extent of area A, but at a constant number of atomic sites, N, for variable strains Δij (i, j = 1, 2) in the plane (x1, x2) of the surface, we have:
which leads to the definition of a second-order, two-dimensional tensor Æij, the elements of which have the dimension of stresses, called surface stresses. Writing the differential of the previous total energy (equation [1.3]) as d(Îł.A) = Îł.dA + A.dÎł and expressing the variation of area A (at a constant number of sites) as dA = A.ÎŽij.Δij (i, j = 1, 2, and ÎŽij being the Kronecker symbol), we get the expression of the surface stresses in relation to the surface energy Îłsand its derivative with regard to the strains of the surface plane:
The variations dΔij of the surface strains are, i...