EMU Notes in Mineralogy, Vol. 4 (2002), Chapter 10, 271–309 Diffusion kinetics in minerals: Principles and applications to tectono-metamorphic processes JIBAMITRA GANGULY Bayerisches Geoinstitut, University of Bayreuth D-95440, Bayreuth, Germany; Permanent address: Department of Geosciences, University of Arizona Tucson, AZ 85721, USA; e-mail: ganguly@geo.arizona.edu Introduction Diffusion is the process by which atoms or ions or ionic species migrate within a medium in the absence of a bulk flow. Diffusion in solids has been a subject of interest in the fields of solid state science (physics, chemistry and metallurgy) for nearly a century, starting with the work of Einstein on the relationship between random atomic movement and diffusion process. The phenomenological study of diffusion began even 50 years earlier, with the empirical formulation of Fick on the relationship between the diffusion flux of a component and its concentration gradient. The subject of diffusion in the solids may be subdivided into volume, grain boundary and surface diffusion. The last topic has, however, received very little attention in the study of geological processes. The study of grain boundary diffusion is important to the understanding of many metamorphic processes including the problems of mass transport, fluid/rock interactions, thermal history and crystal growth. The interested reader is referred to Joestein (1991) for an excellent review of the subject of grain boundary diffusion and its applications to geological problems. Diffusion controlled processes within a mineral preserve important records of the thermal and physico-chemical history of the host rocks. Volume diffusion, that is diffusion through the crystal lattices, affects development of compositional zoning in minerals, ordering of atoms in nonequivalent crystallographic sites of a mineral, formation and coarsening of exsolution lamellae, and retention of isotopic characteristics in minerals that can serve as quantitative chronometers in their thermal and growth history. In this chapter, I present a brief overview of the fundamental principles of volume diffusion kinetics, primarily at a phenomenological level, and discuss the various factors that affect diffusion kinetics in minerals. Finally, I discuss some applications of the diffusion kinetic studies in minerals to the understanding of tectonometamorphic processes in major continent–continent collisional environments. It should, however, be emphasized that the scope of applications of volume diffusion 272 J. Ganguly kinetics to geological and planetary problems is much wider than what I have attempted to cover in this chapter. Some incidental references to additional applications have been made in the appropriate places. List of symbols D*i , Di+ and Di Tracer, self- and chemical diffusion coefficients, respectively, of the component i D(i–j) Chemical interdiffusion coefficient of the components i and j Di(EB) Effective binary diffusion coefficient of the component i in a multicomponent system D Matrix of diffusion coefficients Dij An element of the D matrix τ Diagonal matrix of the eigenvalues of a D matrix τi An eigenvalue of the D matrix B A matrix composed of the eigenvectors of D matrix L Matrix of kinetic coefficients (Onsager matrix) G A thermodynamic matrix that relates D and L matrices f Isotopic correlation factor Q and ∆V + Activation energy and activation volume of diffusion, respectively Ji Flux of a component i J A column vector of the fluxes of n–1 independent components in an ncomponent system Ci Concentration of the component i, expressed in atomic units per unit volume C A column vector of the concentrations of n–1 independent components in an n-component system Xi, ai and γi Atomic fraction, activity and activity coefficient, respectively, of the component i µi Chemical potential of the component i W Non-ideal interaction parameter kB Boltzmann constant η A cooling time constant (K–1t–1) t′ Γ ∫ D(t )dt 0 Phenomenological theory of diffusion Fick’s laws Let us consider a planar section that has a fixed position in an isotropic medium with respect to a coordinate system measured normal to the section. According to Fick’s law, which was formulated by analogy with Fourier’s law of heat conduction, the flux (i.e. 273 Diffusion kinetics in minerals: Principles and applications the rate of transfer per unit area) of a component, Ji, through this planar section is proportional to its local concentration gradient. Thus, J i = − Di ∂Ci , ∂x (1) where Ci is the concentration of i, in atomic units per unit volume, which decreases in the direction of increasing x, and Di is the diffusion coefficient of i (with dimension of L2/t). (The negative sign in the above expression is introduced to make the flux positive in the direction of decreasing Ci.) Implicit in the above statement is the assumption that there is no external force (such as electrical and gravitational forces) acting on the diffusing species. The modifications for the expression of flux to incorporate the effects of an external force and the movement of the planar section, with respect to a fixed coordinate system, are discussed below. From the continuity relation that stems simply from the principle of conservation of matter, it follows (e.g. Crank, 1983, p. 2–4) that if diffusion is one-dimensional (i.e. there is a concentration gradient only along the x axis), then ∂Ci ∂ = − ( J i ), ∂t ∂x (2) so that, if the flux is given by Equation 1, then ∂Ci ∂ D ∂C = i i . ∂t ∂x ∂x (3a) If the diffusion coefficient is independent of position, then ∂C i ∂ 2 Ci . = Di ∂t ∂x 2 (3b) The dependence of D on x arises from its compositional dependence and the variation of composition as a function of position. For three dimensional diffusion in an isotropic medium, the equations corresponding to Equations 3a and 3b are written by simply replacing ∂ by the gradient operator (i.e. i(δ/δx) + j(δ/δy) + k(δ/δz)) and ∂2 by the Laplacian operator ∇2 (i.e. δ 2/δx2 + δ 2/δy2 + δ 2/δz2) in the right-hand side of the equations. The equation expressing the time dependence of concentration, that is Equation 3b or its three-dimensional form, is known as the diffusion equation in Cartesian coordinates. Other forms of the diffusion equation in different coordinate systems follow simply from the appropriate transformation of coordinates. The solutions of the diffusion equation, either analytical or numerical, for the appropriate initial and boundary conditions, permit us to model diffusion controlled properties to retrieve quantitative information about geological, planetary and other processes. 274 J. Ganguly Irreversible thermodynamic formulation While Fick’s law is an empirical law, the flux equation can be formulated rigorously from the principles of irreversible thermodynamics. It follows from the latter that, in the absence of interference from diffusion of other species, the appropriate driving force of diffusion of a species i in an isotropic medium is –∂(µi/T)/∂x, where µi is the chemical potential of the component i. Thus, the flux of a component is given by ∂µ / T J i = − Li i ∂x L ∂µ L =− i i =− i T ∂x T ∂µ i ∂C i ∂Ci ∂x , (4) where Li is a phenomenological coefficient. This relation, however, assumes that the higher order terms of the driving force has negligible effect on the flux (i.e. Eqn. 4 holds within the domain of validity of linear irreversible thermodynamics). Since at a constant p–T condition ∂µi = RT∂lnai = RT∂ln(Ciγi), where ai and γi are the activity and activity coefficient of the component i, respectively, it is easy to see that Ji = − RLi Ci ∂ ln γ i 1 + ∂ ln C i ∂Ci ∂x . (5) Comparing Equations 1 and 5, we have ∂ ln γ i Di = Di+ 1 + ∂ ln Ci where Di+ = , RLi . Ci (6a) (6b) The quantity within the parentheses of Equation 6a is usually referred to as the thermodynamic factor. We will henceforth refer to it as D(thermo). From definition Ci = ni /NV = Xi /V, where Xi is the mole fraction of the component i, V is the molar volume and N is the total number of moles in the system. Thus, if the molar volume of the substance remains constant, then dlnCi = dlnXi. Diffusion coefficients: Terminology and definitions Before proceeding further, it is important to discuss certain properties of diffusion coefficient and the related terminology. In the literature, one encounters terms like tracer, self-, inter-, and chemical diffusion coefficient, the meaning of which is not usually clear to the reader. In addition, there is a lack of uniformity in the usage of these terms, which is a source of confusion in the literature on diffusion kinetics. It is, thus, important to define these terms clearly in the sense these are used in any work. Diffusion kinetics in minerals: Principles and applications 275 Tracer, self-, and chemical diffusion coefficients In this paper, the diffusion coefficient of an isotope of an element that describes its flux solely in response to the isotopic concentration gradient in a chemically homogeneous medium will be called the tracer diffusion coefficient of the element i, and be denoted by the symbol D*i(I) or simply D*i, where (I) stands for the specific isotope. By chemically homogeneous we mean homogeneity with respect to the concentration of chemical elements. The term self-diffusion coefficient will be used to define the diffusion coefficient that describes the flux of an element solely in response to its own concentration gradient, and under the condition that its thermodynamic interaction with the solvent matrix is independent of its concentration so that the “thermodynamic factor” (Eqn. 6a) is unity. Thus, the self-diffusion coefficient of an element is the quantity defined by D+i in Equation 6b. The diffusion coefficient Di, which is a product of the selfdiffusion coefficient and the thermodynamic factor (Equation 6a), will be referred to as the chemical diffusion coefficient of the component i. The self- and tracer diffusion coefficients are equivalent when all isotopes of the element have the same diffusivities. Although this is strictly not the case, the terms self- and tracer diffusion coefficients have been used interchangeably. (In the literature, the term self-diffusion coefficient of an element has also been applied to the limiting case of tracer diffusion, in the sense defined above, when the diffusing tracer isotope and the non-tracer solvent belong to the same element, e.g. diffusion of 26Mg in Mg2SiO4.) Chemical interdiffusion coefficient in binary metallic and ionic systems When two or more components diffuse simultaneously in a given medium, the flux of the components becomes coupled. We first consider the case of diffusion of two neutral species (A and B) across a welded plane (Fig. 1), as in a binary metallic alloy. If the component A diffuses faster than B, then the right-hand side of the couple will swell while the left-hand part will shrink. If, however, the specimen is held at a fixed position, then the interface will move leftwards. This phenomenon was first noticed by Smigelskas & Kirkendall (1947) for the interdiffusion of Cu and Zn by placing fine molybdenum markers at the interface, and is usually referred to as Kirkendall effect (instead of Smigelskas effect or Smigelskas–Kirkendall effect!). In analysing this result of Smigelskas and Kirkendall, Darken (1948) raised the important question “what is diffusion?” and introduced the concept of frame of reference in diffusion studies. In the above example, one can describe the diffusion process with reference to two alternative coordinate systems, x and x′, as follows. In the first system, x′ = 0 is fixed to the interface (which may be located by some inert markers, as in the experiment of Smigelskas & Kirkendall, 1947), and increases to the right. In the second system, x = 0 is located at one end of the diffusion couple, say the left end (this frame of reference is usually called the “laboratory frame of reference”). In the x′ coordinate system, the flux of the component A across a plane located at a fixed distance, say x′ = 0, is simply given by Equation 1. However, in the x coordinate system, the flux of A across a plane at x = k (which we may take as the same plane as at x′ = 0) must involve an additional term, vCA(x = k), in order to account for the effect of movement of the plane, where v is the velocity of the plane. Thus, in the x coordinate system, 276 J. Ganguly Fig. 1. Schematic illustration of the Kirkendall effect for the inter-diffusion of two neutral species, A and B, with DA+ > D+B. The interface, which is shown by a dashed line, moves to the left if the specimen is held at a fixed position. (a) is the initial configuration of the diffusion couple, and (c) is the configuration after an elapsed time. In the x′ coordinate system, the moving interface is located at x′ = 0, whereas in the x coordinate system, the interface is located at x = k (modified from Haasen, 1978). ∂CB + (vCB ) x = k . ∂x So that, assuming D to be independent of x J B = − DB (7a) ∂ 2CB ∂C ∂ ∂CB (7b) –+ v B . =– − ( J B ) = DB 2 ∂x ∂t ∂x ∂x In the above example, the velocity v is obviously a consequence of the difference between the individual diffusivities of the two components A and B. Thus, assuming that the volume of the system has remained constant (and also ignoring any effect due to vacancy flow and interactions of the atoms with the vacancies), solution for v in terms of these individual chemical diffusivities, DA and DB, in the x coordinate system, and rearrangement of terms yields (Darken, 1948) J B = − D( A–B ) ∂CB , ∂x (8a) where D(A–B) is given by D(A–B) = [XADB + XBDA], (8b) and is called a chemical interdiffusion coefficient (in the above example, for a metallic system). The flux of the component A in the x coordinate system is also given by 277 Diffusion kinetics in minerals: Principles and applications Equation 8a upon simply replacing CB by CA. Note that both fluxes are described by the same diffusion coefficient, D(A–B). It may be noted incidentally that Equation 7 is a general equation that describes diffusion under the influence of a “driving force”. The latter is defined to be a force, such as those arising from an electrical field or non-ideal mixing property, which causes an atomic jump in one direction across a potential energy barrier to be more probable than that in the reverse direction across the same barrier (Manning, 1968). Equation 7 is also applied to the solution of diffusion-reaction problem where the interface between two crystals moves, with respect to a stationary coordinate system, due to reaction along with diffusion (see later for an application). Instead of neutral atoms, let us now consider the problem of diffusion of ions of the same charge, z. In this case, if A diffuses faster than B, then there would be an accumulation of excess positive charges on the right hand side of the couple, and a corresponding accumulation of positive charge vacancies on the left. This would create an electrical field Ed (which implies a driving force zEd, where z is the charge of the diffusing ion) that would affect the diffusion of ions so that local electrical neutrality of the sample is preserved. The latter requirement implies that, in the absence of any other mechanism of charge compensation, the net flux of ions at the interface must be zero (i.e. there must be equal number of A and B crossing the interface per unit area per unit time). As a result, the interface must remain fixed with respect to a stationary coordinate system if the molar volume remains constant. Expressing the mean drift velocity of the ionic species in terms of Ed (i.e. v = (Di)zEd/kBT) in Equation 7, and also in the analogous expression for JA, and solving Ed in terms of DA and DB under the constraint that JA + JB = 0, yields (e.g. Manning, 1968) J B = −J A = − We now write D(Az – Bz) = = DA DB ∂C B . X A DA + X B DB ∂X (9) DA DB . X A DA + X B DB (10) Equation 10 defines the chemical interdiffusion coefficient in a binary system of equally charged species. By the requirement of mass balance, ∂CB/∂x = –∂CA/∂x. As emphasised by Lasaga (1979), the chemical interdiffusion coefficient in an ionic system will, in general, be overestimated, especially around X = 0.5, if one uses the Darken relation, i.e. Equation 8b instead of Equation 10. The Darken relation has been applied to mineralogical systems, but from a theoretical point of view, it is not applicable to such systems since the diffusing species are ions instead of neutral atoms. For the interdiffusion of unequally charged species, the chemical interdiffusion coefficient in a volume fixed reference frame is given by (Barrer et al., 1963; Brady, 1975) D (AZA – BZB) = DA DB (Z A X A + Z B X B )2 Z A2 X A DA + Z B2 X B DB , (11) where ZA and ZB represent the charges on the specified ionic species. Equation 11 reduces to Equation 10 when ZA = ZB. 278 J. Ganguly Thermodynamic effect on interdiffusion coefficient Substitution of Equation 6a in the expressions of interdiffusion coefficient in either a binary metallic system (Eqn. 8b) or a binary ionic system (Eqns. 10 and 11), and application of the Gibbs–Duhem relation (i.e. n1dµ1 + n2dµ2 = 0 at constant p–T condition) yield, for a system with constant molar volume, ∂ ln ai D (i − j ) = D + (i − j ) ∂ ln Ci ∂ ln γ i = D + (i − j )1 + ∂ ln X i , (12) where D+(i–j) is an appropriate (metallic or ionic) interdiffusion coefficient had the two components mixed ideally. It is expressed according to the forms of Equations 8b, 10 and 11, as appropriate, by substituting the self-diffusion coefficient, D+i , for Di. Thus, for example, if the interdiffusion is between two equally charged ions, then ∂ ln γ i D ( A − B ) = D + ( A − B )1 + ∂ ln X i + DA++D DBA+ = + + X A DA + X B DB ∂ ln γ i 1 + ∂ ln X i . (13) Note that in Equations 12 and 13, component i can be either A or B, since, according to the Gibbs–Duhem relation and stoichiometric constraint for a binary solution (i.e. dXA = –dXB) with a constant molar volume, d ln aA/d ln CA = d ln aB/d ln CB. Also recall that if the molar volume of the material is constant, then d ln Ci = d ln Xi. It should be noted that, in general, the self-diffusion coefficients are also functions of composition. Thus, D+i values should be for the same composition for which one wishes to compute D(A–B). However, usually we do not have enough data for geologically important systems to treat self-diffusion coefficients as function of composition. If the binary solution has a sub-regular thermodynamic mixing property, i.e. the excess Gibbs energy of mixing can be expressed according to ∆Gxs = X1X2(W12X2 + W21X1), where Wij represents the Margules parameters (see, for example, Ganguly & Saxena, 1987), then ∂ ln γ1i X X = 1 2 [W12 (2 X 1 − 4 X 2 )+ W21 (2 X 2 − 4 X 1 )]. ∂ ln X 1 RT (14) For the special case of “Simple Mixture” or “Regular Solution”, W12 = W21 = W, so that ∂ ln γ1i 2WX 1 X 2 . =− ∂ ln X 1 RT (15) As an illustration of thermodynamic effect, we show in Figure 2 the thermodynamic factor calculated by Brady & McCallister (1983) at 1150 °C for the quasi-binary Ca–Mg(+Fe) interdiffusion between pigeonite lamellae and sub-calcic diopside host. The sample is a diopside megacryst (Fe/(Fe + Mg) = 0.14) from Mabuki kimberlite, Tanzania. The experimentally determined critical mixing temperature (Tc) between the Ca and Mg (+ Fe) components is 1132 °C, and the critical mixing composition is ~ 20 mol% diopside. Also shown in the figure is the thermodynamic factor (dashed curve) calculated from the mixing energy data of Lindsley et al. (1981) in Diffusion kinetics in minerals: Principles and applications 279 the diopside–enstatite join at temperatures that have the same relative position with respect to Tc (1500 °C) in this join as the inferred temperature of the natural sample has with respect to its own Tc. It is evident from Figure 2 that the thermodynamic effect on the diffusion coefficient is very pronounced near the critical mixing temperature (also see Christoffersen et al., 1983). It should be noted from Equation 13, and the equivalent expression for the metallic system that follows from Equation 8b, that as XA → 0, D(thermo) = 1 (since γi = constant). Consequently, lim X i →0 D (i − j ) = Di+ . Thus, we arrive at the rather counter-intuitive conclusion that the interdiffusion coefficient in a binary system approaches the self-diffusion coefficient of the dilute component (instead of the major component). This conclusion can be shown to be valid also for multi-component solutions by examining the limiting behaviour of the extension of Equation 13 for the ternary solution (see below, Eqn. 24). Diffusion, atomic motions and correlation effect Diffusion takes place via atomic jumps. The correlation effect arises from the nonrandomness of the atomic jumps. To illustrate this point, let us consider the common case of a vacancy mediated diffusion. In this case, an atom moves by interchanging position with a vacancy after it arrives (or diffuses) into one of the neighbouring lattice sites. But Fig. 2. Thermodynamic factor (TF) for the inter-diffusion of Ca–Mg(+Fe) as a function of diopside content of clinopyroxene, as calculated by Brady & McCallister (1983). The dashed line is for the quasi-binary system Ca–Mg(+Fe), with Fe/(Fe + Mg) = 0.14, corresponding to the composition of a natural diopside megacryst from Mabuki kimberlite, Tanzania, at 1150 °C. The critical mixing temperature in this join is 1132 °C. The solid line is for Fe-free system at a temperature that has the same ratio with the Tc in this join, which is 1500 °C, as the chosen temperature of the Fe-bearing sample has with its own Tc. 280 J. Ganguly after making the first jump, there is a greater probability for the atom to return to its original position (because it now finds a vacancy in that position) when it executes the next jump, than moving into any of the other neighbouring lattice sites that are occupied by atoms. Thus, a certain fraction of the atomic jumps are “wasted”. The correlation factor, f, accounts for this problem by expressing Di as a product of fi and Di(random). The latter is the value of D that should be obtained under conditions of completely random atomic jumps. By definition, fi ≤ 1. It can be shown that for one dimensional diffusion, D(random) = 〈X2〉/2t, where 〈X2〉 is the mean square displacement of the atoms after time t (for random atomic jumps of equal length, we obviously have 〈X〉 = 0, but 〈X2〉 ≠ 0). This relation between the mean square displacement and diffusion coefficient for random atomic motion is often referred to as the Einstein relation, and provides the basis for the determination of D by molecular dynamics simulation. In this approach, 〈X2〉 is determined at several different time steps, and the slope of the linear relation between 〈X2〉 vs. t yields the diffusion coefficient (e.g. Tirone, 2002). Hermeling & Schmalzried (1984) determined the correlation factors for the diffusion of Fe2+ and Mg in olivine. So far these constitute the only measurements of fi for diffusion in rock forming minerals. Their results are illustrated in Figure 3. Diffusivities of the different isotopes of an element would differ from each other because of the differences in their masses, which affect their jump frequencies, and the correlation coefficient. If Di(*α) and Di(*β) are the tracer diffusion coefficients of two Fig. 3. Correlation factors of Fe2+ and Mg as a function of XMg in binary Fe–Mg olivine at 1 bar, 1130 °C, and log fO2 = –10.67 (modified from Hermeling & Schmalzried, 1984). 281 Diffusion kinetics in minerals: Principles and applications isotopes α and β of an element i, then with certain simplifying assumptions (see Bokshtein et al., 1985 for further details), it can be shown that Mβ ∆D ≈ fα * M Di ( β ) α 1 2 − 1 , (16) where ∆D = Di(*α) – Di(*β) and M stands for the masses of the specified isotopes. There is only one correlation factor in the above equation since the correlation factors of two isotopes of an element are interrelated (e.g. Bokshtein et al., 1985; Borg & Dienes, 1988). In the treatment of multi-component diffusion, it is usually assumed that the self-diffusion coefficient of an element is the same as the diffusion coefficient of a tracer isotope of the element. While this is not strictly correct, the error introduced by this assumption is usually small compared to other sources of error, especially in complex geological problems. Multi-component diffusion Extension of Fick’s laws During geological processes, diffusion in many minerals, e.g. garnet, is often multicomponent in nature in that it involves simultaneous flow of more than two components. Understanding of multi-component diffusion processes is, therefore, important to the interpretation of diffusion induced compositional modifications of minerals during geological processes. In this section, I would try to provide a brief overview of some of the important phenomenological concepts of multi-component diffusion. In a multi-component system, the diffusion flux of any component does not depend only on its own concentration or chemical potential gradient, but also on those of all other diffusing components. Assuming that only the first spatial derivatives of concentrations are important for the flux of any component, Fick’s law can be extended to a system of n components in a volume fixed reference frame as follows (Onsager, 1945): ∂C ∂C ∂C J 1 = − D11 1 − D12 2 ........................... − D1( n−1) n−1 ∂ ∂ x x ∂x ∂C ∂C ∂C J 2 = − D21 1 − D22 2 ......................... − D2( n−1) n−1 ∂x ∂x ∂x . ............................................................................................. (17) ∂C ∂C ∂C J n−1 = − D( n−1)1 1 − D( n−1) 2 2 ........... − D( n−1)( n−1) n−1 ∂x ∂x ∂x In the above system, there are n – 1 flux equations since in an n-component system of fixed mass and volume, the concentration of one component is fixed by those of others at any given point. An on-diagonal term in Equation 17 shows the extent by which the flux of a component is affected by its own concentration gradient, whereas the off-diagonal terms 282 J. Ganguly indicate the extent of hydrodynamic coupling in the diffusion process, i.e. the extent to which the flux of a given component is influenced by the concentration gradients of the other independent components. If these off-diagonal terms are significant, then one could get a positive flux of a component in the direction of increasing concentration, leading to what is known as uphill diffusion. Indeed, because of the effect of cross terms, a component could diffuse even in the direction of its increasing chemical potential. Uphill diffusion has not been documented in any mineralogically important system, but has been found in several silicate melts (e.g. Chakraborty et al., 1995a, 1995b) that are of interest in the understanding of magmatic processes. D matrix Using the principle of matrix multiplication, we can re-write Equation 17 as D11 D12 ..........D1( n −1) ∂C1 / ∂x J1 D D ..........D2( n −1) ∂C2 / ∂x J 2 = − 21 22 ............................... ⋅ ............. , .... D( n −1)1 ....... D( n −1)( n −1) ∂Cn −1 / ∂x J n −1 (18a) or, in matrix notation ∂C ∂x (18b) ∂C ∂ ∂C = D , ∂t ∂x ∂x (18c) J = −D so that where J and C are (n – 1) column vectors and D is an (n – 1)×(n – 1) matrix of diffusion coefficients, which is usually referred to as the D matrix. For n = 2, Equation 17 reduces to the expression of flux in binary diffusion, in which case D11 is a binary interdiffusion coefficient. In general, the D matrix is not symmetrical. However, from the principles of irreversible thermodynamics, it can be related to two symmetric (n – 1) × (n – 1) matrices, L and G, as D = LG. (19) The matrix L is the Onsager matrix or the matrix of kinetic, or phenomenological, coefficients, and G is the thermodynamic matrix. (Recall from Eqn. 6 that the chemical diffusion coefficient of a species consists of a product of an L coefficient and a thermodynamic factor.) The L and G matrices are also positive definite, that is, they have real and positive eigenvalues. Consequently, the D matrix must also have real and positive eigenvalues. This requirement provides important constraints on the values of the elements of the D matrix (see Lasaga, 1998, for further discussion). Furthermore, Equation 19 permits one to test the mutual compatibility of the data on the diffusion kinetic and thermodynamic mixing properties of species 283 Diffusion kinetics in minerals: Principles and applications in a solution. One can also extract the unknown value of a diffusion kinetic or thermodynamic mixing property, if other values are well constrained, by inserting guessed values of these parameters into the L and G matrices until the product of D and G–1 yields a symmetric and positive definite matrix (Chakraborty & Ganguly, 1994; Chakraborty, 1994). In terms of the L matrix, we can write an expression for flux analogous to Equation 18b as ((∂µ/T) ∂ ì/ T) J = −L . (20) ∂x The symmetry of the L matrix is a consequence of Onsager reciprocity principle (Onsager, 1931a, 1931b). In a system of constant molar volume, which is a good approximation for most diffusion process in minerals, the elements of G matrix can be calculated as follows (e.g. Loomis, 1978). Gij = ∂(µi − µ n ) , ∂X i (21) where the nth component has been chosen to be the dependent component. The diffusion matrix, as defined above, has the property that it can always be diagonalised (Toor, 1964; Cullinan, 1965). This enables reduction of multicomponent diffusion to the mathematical forms of binary diffusion (Toor, 1964; Cullinan, 1965), as follows. If τ is a diagonal matrix of the eigenvalues of the D matrix, and B is a matrix for which the columns are composed of the corresponding eigenvectors, then B–1DB = τ (or B–1D = τ B–1). Therefore, on pre-multiplying both sides of Equation 18c by B–1, the multi-component diffusion equation can be expressed in the following form ∂ C′ ∂ ∂ C′ = τ , ∂x ∂x ∂t (22) where C′ = B–1C. Thus, instead of the coupled diffusion equations of the original components, we obtain uncoupled or independent diffusion equations of the transformed components, Ci′, as ∂Ci′ ∂ ∂Ci′ = τ i ∂t ∂x ∂x , (23) where the eigenvalue τi is the diffusion coefficient of the transformed component Ci′. These equations can be solved for Ci′(x, t) using solutions of diffusion equations characterised by a single concentration gradient (e.g. Crank, 1983). The solution for C′(x, t) can then be converted to that of the real component C(x, t) using the relationship between the two variables. The elements of the D matrix can be calculated from the self-diffusion and thermodynamic mixing property data of the species from the extensions of Equations 8b and 11 to multi-component systems. These extensions are due to Hartley & Crank (1949) for the metallic system and Lasaga (1979) for the ionic systems. The equation derived 284 J. Ganguly by Lasaga (1979), which is appropriate for the mineralogical problems, is as follows if the activity coefficients of the diffusing components (γi) are constant within the domain of compositional variation D*Z Z X ij i j i (D Di*i* –− D Dij = Di*δ ij − k = n Dn*n*) , 2 * ∑ Z k X k Dk k =1 ( ) (24) where δij is the Kronecker delta (δij = 1 when i = j, and δij = 0, when i ≠ j). Full treatment to incorporate the effects of variation of γi can be found in Lasaga (1979). Because of the paucity of experimental data on diffusion in multicomponent mineralogical systems, the off-diagonal terms of the D matrix are usually neglected. Such approximations, however, are not always justified. Chakraborty & Ganguly (1991, 1992) have discussed examples of D matrix in garnets that show significant off-diagonal terms. An example from their study is given below, where the matrix elements are in units of cm2/s, and Ca was treated as the dependent component. Mn Mg Fe Mn 8.38(10–20) –2.78(10–21) –7.16(10–20) Mg –9.91(10–23) 7.26(10–21) –4.81(10–23) Fe –4.68(10–21) –8.81(10–23) 1.19(10–20) This D matrix was calculated for a fixed garnet composition (Alm0.79Prp0.06Sps0.10Grs0.05) in the Barrovian zone rocks (Dempster, 1985) at the inferred peak metamorphic condition of 600 °C, 5 kbar, fO2 = graphite–O2 equilibrium (see below for discussion about the dependence of D on fO2). It is evident that the magnitude of some of the offdiagonal terms are comparable to the on-diagonal ones (compare DFeFe with DFeMn and DMgMg with DMgMn) so that neglect of these cross effects on diffusion could lead to significant errors in the modelling of diffusion modification of compositional zoning in multi-component garnets. To illustrate the importance of accounting for the multi-component interactions, I show in Figure 4 the diffusion profiles for Fe, Mg, Mn and Ca that would be generated in a semi-infinite garnet/garnet diffusion couple according to the D matrix given above. Although the D matrix is a function of composition, and hence of position, a constant D matrix has been assumed for the sake of simplicity. The profiles were calculated using the program PROFILER, which is discussed in detail in Glicksman (2000). The initial composition of Mn on the two sides of the couple were chosen to be the same, and Ca was treated as the dependent component. The simulation is for 40 Myr, and each division on the distance axis of the main figure equals 1 µm. It is interesting to note that Mn shows uphill diffusion and develops a wavy pattern near the interface of the couple due to the influence of the other diffusing species. It should be noted that uphill diffusion of a component in a semi-infinite diffusion couple not only depends on the magnitude of the off-diagonal terms of the D matrix, but also on the nature of the compositional difference of the components on two sides of the 285 Diffusion kinetics in minerals: Principles and applications 70 Concentrations (at%) 60 50 40 Mg 30 Fe 20 Mn 10 0 –3 (a) Ca –2 0 –1 1 2 3 Distance Fig. 4. (a) Calculated diffusion profiles of Fe, Mg, Mn and Ca in a semi-infinite garnet/garnet diffusion couple using the D matrix given in the text. The initial concentration of all components was homogeneous in each garnet crystal, and that of Mn was the same on both sides of the couple. Multi-component interaction produces the uphill diffusion and wavy pattern of Mn profile near the interface, which is magnified in (b). The simulation is for 40 Myr. Each division on the distance axis in (a) equals 1 µm. couple (see, for example, Chakraborty et al., 1995a; Glicksman, 2000). Because of the multi-component interaction, one or more components in a multi-component diffusion can have either stationary or moving zero flux planes (ZFP). A ZFP defines a plane where the flux of a component vanishes. In other words, the component with a ZFP diffuses on both sides of the plane, but not across the plane. The dynamics of ZFP have recently been explored in detail by Glicksman & Lupulescu (in press). This property has interesting industrial and potential geological applications. Diffusion in anisotropic crystals: Diffusion tensor In anisotropic crystals, diffusion properties are, in principle, different along different directions. In such medium, Equation 1 holds only for the special case that there is concentration gradient only along the x direction. If there are concentration gradients along the other directions that are orthogonal to x, then the flux along any direction is linearly related (within the domain of validity of linear irreversible thermodynamics) to the concentration gradients along all three orthogonal directions. Thus, in the absence of a driving force, the flux of a component along the x direction is given by J x = − Dxx ∂C ∂C ∂C . − Dxy − Dxz ∂x ∂y ∂z (25) Similar relation holds for the flux of the component along the other directions. Thus, using the principle of matrix multiplication, as in Equations 17 and 18, we have J = – D∇C (26) where J and ∇C are column vectors of the directional fluxes and concentration gradients, respectively, and D is a symmetric matrix of the diffusion coefficients, which is known 286 J. Ganguly as the diffusion tensor. It is, however, always possible to find three orthogonal directions ξ1, ξ2, ξ3 in an anisotropic medium such that the flux along any of these directions depends only on the concentration gradient along the specific direction, i.e. Jξi = – Dξi(∂C/∂ξi). These directions and the corresponding diffusion coefficients are known as the principal diffusion axes and principal diffusion coefficients, respectively. Diffusion along any arbitrary direction κ, which makes angles θ1, θ2, θ3 with the principal diffusion axes (1, 2 and 3), is given by J κ = − Dκ ∂C ∂κ , (27) where Dκ = Dξ1 cos2θξ1 + Dξ2 cos2θξ2 + Dξ3 cos2θξ3, and ∂C/∂κ is the concentration gradient along the direction κ. The direction of a crystallographic symmetry axis coincides with that of a principal diffusion axis. Thus, the a, b and c crystallographic directions in cubic, tetragonal, orthorhombic and hexagonal systems constitute the directions of principal diffusion axes. For monoclinic system, the b axial direction constitutes the direction of one of the principal diffusion axes. The other two, which must lie in the a–c plane, can be determined by three measurements of diffusion coefficients in that plane. For triclinic system, one needs measurements of diffusion coefficients in six different directions to determine the directions of the three principal diffusion axes (see Nye, 1957 for further discussions). Anisotropic diffusion was measured in several non-cubic minerals such as olivine (orthorhombic: Buening & Buseck, 1973; Misener, 1974; Jurewicz & Watson, 1988; Chakraborty et al., 1994), orthopyroxene (orthorhombic: Schwandt et al., 1988), clinopyroxene (Sneeringer et al., 1984; Tirone, 2002) and feldspar (triclinic: e.g. Christoffersen et al., 1983). Because of the relaxation of structure with increasing temperature, diffusion anisotropy should be expected to decrease with increasing temperature. The anisotropic diffusion data for olivine were summarised and discussed by Morioka & Nagasawa (1991). The tracer diffusion coefficients of Ni, Co, Ca, as well as Fe–Mg interdiffusion coefficient, were found to be fastest parallel to the c axis, and slowest parallel to the b axis in olivine. The observed anisotropy is consistent with the arrangement of divalent cation sites and the energetics of defect formation in the olivine structure in that the M1 sites form a closely spaced chain parallel to the c axis, and the energy of formation of cation vacancies in the M1 site is significantly less than that in the M2 site (e.g. Ottonello, 1997). Niemeier et al. (1996) observed by high temperature Mössbauer spectroscopy that cation diffusion in olivine takes place predominantly via M1–M1 jumps along the c direction. In contrast to the above results, Jurewicz & Watson (1988) found that at fO2 < 10–8 bar, Mn and Fe show highest diffusion rates parallel to the a axis. These authors tried to explain the unexpected anisotropic behaviour in terms of different diffusion mechanisms along a and b/c crystallographic axes. For alkali feldspars, Na and K self-diffusion and Na–K interdiffusion were found to be faster within (010) plane than normal to it. As discussed by Christoffersen et al. (1983), the observed diffusion anisotropy is consistent with the feldspar structure in that the alkali sites are much closer to each other within the (010) plane than normal to it. The above 287 Diffusion kinetics in minerals: Principles and applications examples suggest that consideration of the packing density of the host structural sites could provide useful, although not unfailing, guidelines about the expected diffusion anisotropy in minerals. Factors affecting diffusion coefficient Diffusion can take place through a number of different mechanisms such as through exchange of position between atoms and lattice vacancies (vacancy mechanism), migration of atoms through interstitial sites (interstitial mechanism) etc. These have been discussed in detail in many standard books on diffusion in solids (e.g. Shewmon, 1963; Bokshtein et al., 1985; Borg & Dienes, 1988). Vacancy mechanism is by far the most important of all diffusion mechanisms. All cases of substitutional diffusion seem to operate through a vacancy mechanism (Borg & Dienes, 1988). Thus, any physicochemical factor that affects the vacancy concentrations in a crystal significantly also has a significant effect on its diffusion properties. Since diffusion involves climbing an energy barrier by atoms between two stable states, temperature has the strongest effect on diffusion coefficient as it provides the energy (kBT) to elevate the atoms over the energy barrier. The other factors affecting the volume diffusion coefficient of a species are pressure, volatile species (fO2 and the fugacities of the “water” related species), dislocations, bulk composition of the phase, and radioactive damage. The last topic is not of any interest in the context of the present chapter, and, thus, will not be discussed any further. The interested readers are referred to Borg & Dienes (1988) for a general discussion about the theory, and to Cherniak (1993) for discussions in the context of geological systems. Effect of temperature and pressure The temperature and pressure dependencies of a diffusion coefficient are given by ∂ ln D Q( p) =− ∂ (1 / T ) R (28) ∂ ln D ∆V + (T ) , =− ∂p RT (29) where Q(p) and ∆V +(T) are known as the activation energy (at pressure p) and activation volume (at temperature T) of diffusion, respectively. Note that the above equations are formally similar to those governing the temperature and pressure dependencies of the equilibrium constant, K. In general, any kinetic constant or coefficient has the same formal dependencies on temperature and pressure. Assuming that Q(p) is independent of temperature, integration of Equation 28 yields D = D0 e − Q( p) RT , (30) where D0 is D(T = ∞). Assuming that ∆V + is independent of pressure, we have Q(p) = Q(p′) + ∆V +(p – p′). The activated state is an energetically higher transient state that a system passes 288 J. Ganguly through in any kinetic process. For diffusion in solids, the activation energy is the sum of the potential energy (or enthalpy) barrier, ∆H+m, that an atom must climb over in order to move from one lattice position to the next (i.e. enthalpy barrier to migration), and the enthalpy of formation of vacancies, ∆H+v, if the diffusion process is controlled by intrinsic vacancies. The activation volume has analogous definition, i.e. ∆V + = ∆V +m + ∆V+v, where ∆V m+ is the transient volume change of the crystal during the process of atomic migration and ∆V v+ is the volume change associated with the formation of intrinsic vacancies when the diffusion process is in an intrinsic domain. The pre-exponential factor, D0, is + proportional to e∆S /R, where ∆S+ is the activation entropy of diffusion, and has components associated with both migration and vacancy formation, as in the other activation terms. Available experimental data on diffusion in minerals show that at pressures up to several tens of kilobars, ∆V + > 0, so that increasing pressure within this range will reduce the diffusion coefficient. Review of the experimental data on divalent cation diffusion in olivine, garnet and spinel (Chakraborty & Ganguly, 1992; Chakraborty et al., 1994; Chakraborty & Rubie, 1996; Misener, 1974; Liermann & Ganguly, 2002) show ∆V + to be less than 10 cm3/mol, and probably around half as much. Thus, on the basis of the available experimental data, one would expect a relatively small pressure effect on D for divalent cation diffusion in minerals. For example, at 1000 K, the expected effect of a change of 5 kbar pressure would be to reduce logD by no more than 0.26, and probably by half as much. In principle, ∆V + is a function of pressure. However, within experimental error, no pressure dependence of ∆V + could be detected in garnet up to ~ 85 kbar (Chakraborty & Rubie, 1996). On the other hand, diffusion kinetics of a substance at a given temperature seems to bear a relation with the degree of proximity of the temperature to the melting temperature, Tm (e.g. Borg & Dienes, 1988). Melting temperature maximum has been found in olivine, and probably all minerals have the same property. Thus, after the pressure exceeds that of Tm(max), increasing pressure at a fixed temperature may enhance the diffusion kinetics in a mineral since it would bring the mineral progressively closer to Tm. Effect of fO2 In solids containing elements that can have variable oxidation states, such as iron, fO2 is expected to influence the diffusion property by changing the vacancy concentration through the change of the oxidation state of the element. For example, if the homogeneous redox equilibrium of iron in a solid is governed by the reaction 3Fe2+(l) + ½ O2(g) ↔ 2Fe3+(l) + FeO(surface) + VFe , (a) where l, g and VFe stand for lattice site, gas and vacancy in Fe lattice site, respectively, then it is easy to show that VFe, and hence the diffusion coefficient, would vary approximately as (fO2)1/6. This relation follows by combining the expression of equilibrium constant of the above reaction with the relation 2(Fe3+) = VFe (which follows from the requirement of charge conservation if the vacancies are neutral), and assuming that XFe is not significantly altered by the oxidation. It is further assumed, although rarely 2+ Diffusion kinetics in minerals: Principles and applications 289 stated explicitly, that the activities of both Fe2+ and Fe3+ are proportional to their mole fractions (in the spirit of the laws of dilute solutions). Experimental data on the diffusion coefficients in ferromagnesium olivine (Buening & Buseck, 1973; Nakamura & Schmalzried, 1983) show that D varies approximately as (fO2)1/6. It should be noted that fO2 affects the diffusion coefficient not just of Fe, but also that of other cations (i.e. Fe does not have any exclusive right to utilise the vacancies created by its oxidation). The dominant diffusion mechanism could change as a function of Fe concentration and fO2. For example, the experimental data of Chakraborty et al. (1994) suggest that the above defect forming reaction is of primary importance in the diffusion behaviour of olivine only when the Fe content exceeds a threshold value of ~ 150 ppm. Dieckmann & Schmalzried (1975, 1977) showed that at a fixed temperature, logD*Fe in Fe3O4 vs. log fO2 has a minimum, which shifts to higher fO2 with increasing temperature. The experimental data can be matched very well by a theoretical relation between D*Fe and fO2 that they derived by invoking that Fe diffuses through both vacancy and interstitial mechanisms. The vacancy diffusion plays the dominant role at fO2 above the minimum whereas the interstitial diffusion plays the dominant role at lower fO2. Effect of hydrous condition Diffusion in the presence of water has been investigated by a number of workers. The species affecting diffusion may be H+, (OH)– or H2O. We will simply refer to these as “water”. A summary of the available experimental data on the effect of “water” on diffusion in mineralogically important systems may be found in Cherniak (1993). On reviewing these data, she concluded that “water” may not play a significant role in the interdiffusion process that involves only a simple exchange between cations of the same charge. On the other hand, “water” (the actual species could be proton) has been shown to have a significant enhancement effect on the interdiffusion or ordering process in feldspars that involves Al–Si exchange (e.g. Yund & Snow, 1989; Goldsmith, 1991; Graham & Elphick, 1991). Also, experimental study on the effect of “water” at 300 bars and fO2 defined by the Ni–NiO buffer on the Fe2+–Mg interdiffusion in olivine also shows an increase of D(Fe2+–Mg) by a factor of ~ 10 relative to the dry diffusion data of Chakraborty (1997) (Kohlstedt, pers. commun.). The experimental data for olivine seem contrary to the conclusion of Cherniak (1993). The effect of “water” on diffusion kinetics needs to be carefully investigated so the experimental data can be applied to natural systems in a meaningful way. Our understanding of the problem at the present stage is sketchy at best. Effect of dislocations Diffusion along dislocations, commonly referred to as pipe diffusion, is much faster than diffusion through crystal lattice. In the presence of distributed dislocations, the apparent volumetric diffusion would reflect a combination of the diffusion through normal crystal lattice and that through the dislocations. Yund et al. (1989) investigated the effect of dislocations on the apparent volumetric diffusion in albite–adularia diffusion couples. Comparing the result of experiments at hydrostatic condition with that in which the 290 J. Ganguly diffusion couple was strained at a rate of 10–6 s–1 during the process of diffusion at the same p–T condition (1.5 kbar, 1000 °C), they concluded that distributed dislocations are unlikely to have any significant effect on the bulk volumetric diffusion in alkali feldspars at all metamorphic conditions. The above result, however, does not guarantee that dislocations have, in general, negligible effect on the bulk volumetric diffusion in minerals during metamorphism, especially when these are in motion. Nonetheless, the effect of distributed dislocations on the bulk diffusion process in minerals at the strain rate of metamorphic rocks may not be a matter of major concern. The effect of localised dislocations should be apparent in the extended nature of the diffusion profile in a mineral as compared to those in other parts of the same mineral in a rock. These anomalous profiles should obviously be avoided in modelling compositional profiles that are aimed at retrieving time scales of metamorphic processes (see below). Change of diffusion mechanism: Applicability of laboratory data to geological problems A point of critical importance in the application of laboratory experimental data to natural systems is the possible change of diffusion mechanism in moving from the laboratory to the natural conditions. There are two important issues in this respect, namely, (a) the change of mechanism as a function of temperature and other physical variables such as fO2 and pressure, and (b) change of mechanism due to the “purity” of mineral composition that are sometimes used in the laboratory experiments. These problems are discussed below. The lattice vacancies originate for two different reasons. First, there are always an equilibrium number of lattice vacancies in a crystal, which varies as a function of temperature. These are known as intrinsic lattice vacancies, and result from the effect of entropy of mixing between the vacancies and ions in lowering the Gibbs energy (G) of the system. The Gibbs energy of a solution must decrease in the terminal compositional segments of any solution (for a proof of this statement, see, for example, Ganguly & Saxena, 1987, p. 37). Inasmuch as the vacancy can also be treated as a component in the solid solution, G of a crystal must also decrease as function of Xv (atomic fraction of vacancies) in the terminal region of Xv = 0. Second, vacancies are created by the replacement of an ion in a lattice site by an ion of different charge (e.g. replacement of Na+ by Cd2+), or by the oxidation of an ion in a lattice site (e.g. oxidation of Fe2+ to Fe3+). These are known as extrinsic vacancies since their formation results from interaction with an external source. As discussed by Chakraborty (1997), one should distinguish between the extrinsic vacancies created by an impurity substitution, in which case there is no defect formation energy, and those created by the redox reaction of a transition metal element. In the latter case, there is a defect formation energy, which equals the enthalpy change of the redox reaction, and the defect concentration changes as a function of temperature. Chakraborty (1997) called the first case as pure extrinsic diffusion (PED) and the second case as transition metal extrinsic diffusion (TaMED). Diffusion kinetics in minerals: Principles and applications 291 Fig. 5. Change of self-diffusion mechanism of Na+ in Cd2+ doped NaCl as a function of temperature. At high temperature, the diffusion is controlled dominantly by the equilibrium or intrinsic point defects whereas at low temperature, it is controlled by the extrinsic point defects created by the substitution of Cd2+ for Na+ according to 2 Na+ → Cd2+ + V(Na+) , where V(Na+) stands for a vacancy in the sodium site (modified from Mapother et al., 1950). The atomic fraction of the intrinsic lattice vacancies have an exponential dependence on temperature according to Xv ∝ exp(–∆H0v/RT), where ∆H0v is the enthalpy of formation per mole of the particular type of vacancy†. Consequently, at high temperature, Xv(intrinsic) >> Xv(pure extrinsic), so that diffusion takes place essentially through the intrinsic vacancies. On the other hand, at low temperature, Xv(intrinsic) << Xv(pure extrinsic) so that diffusion takes place dominantly through the extrinsic defects created by heterovalent substitution. The temperature for transition from a dominantly intrinsic to a dominantly extrinsic mechanism depends on the system. An example of this transition for the self-diffusion of Na+ in Cd2+ doped NaCl is shown in Figure 5. As discussed above, the activation energy in the intrinsic domain is the sum of the energies of defect formation and atomic migration, whereas † Note that if the vacancies are of Schottky type, that is created in pairs of cation (c) and anion (a) vacancies, and H0v is the enthalpy of formation of the Schottky pair, then from the expression of equilibrium constant of the vacancy forming reaction, we have Xv(c)Xv(a) ∝ exp (–∆H0v /RT), or Xv(c) ∝ exp (–∆H0v /2RT). 292 J. Ganguly that in the pure extrinsic domain is only due to atomic migration. Thus, the difference between these two activation energies yields the energy of (intrinsic) defect formation. Similar to the case of intrinsic diffusion, the defect concentration for TaMED diffusion also vary as a function of temperature as exp(–∆Hr0/RT), where –∆Hr0 is the enthalpy change of the appropriate redox reaction. The latter is, however, much less than the enthalpy of formation of intrinsic defects. Thus, the log D vs. 1/T slope in the TaMED domain is less than that in the intrinsic domain. A qualitatively similar behaviour to the extrinsic–intrinsic transition for volume diffusion is also shown by the transition from grain boundary to volume diffusion in polycrystalline aggregates. At low temperature, the pathways offered by the grain boundaries dominate those due to intrinsic defects, but the situation reverses at high temperature. In mineralogical systems, extrinsic–intrinsic transition was first suggested for cation diffusion in olivine at ~ 1100 °C by Buening & Buseck (1973). These data served as an illustration of the change of volume diffusion mechanism in many mineralogical publications. Also, these diffusion data have been used extensively to model thermal histories of terrestrial and planetary samples. However, Buening & Buseck (1973) used a diffusion couple consisting of Mg-rich olivine single crystal and powdered synthetic fayalite. They noted that the observed change of mechanism could have also been due to a change of grain boundary to volume diffusion – a point that seems to have been ignored in favour of an interpretation of extrinsic–intrinsic transition. Recently Chakraborty et al. (1994), Meissner et al. (1998) and Chakraborty (1997) determined both tracer diffusion of Mg (D*Mg) and interdiffusion of Fe–Mg (D(Fe–Mg)) in olivine single crystals over the temperature range of 980–1300 °C. Their data (Fig. 6) show no change of volume diffusion mechanism in olivine within this temperature range. Chakraborty & Ganguly (1991) and Ganguly et al. (1998) also showed that there is no change of self- or tracer diffusion mechanism of Mg in garnet within the temperature range of ~ 750–1475 °C (Fig. 6). On the basis of the evidence presented above, it seems reasonable to conclude that volume diffusion in olivine and garnet does not show any change of mechanism within the temperature range of geological interest. From comparison of the intrinsic defect formation energy (~ 800 kJ/mol) and the experimental activation energy of diffusion in olivine (~ 275 kJ/mol), Chakraborty et al. (1994) pointed out that the latter cannot represent a combination of defect formation and migration energies. Thus, the observed diffusion in olivine is in the extrinsic domain. Chakraborty et al. (1994) argued, from consideration of the intrinsic vacancy content that follows from conservative estimate of defect formation energy, that intrinsic diffusion is unlikely to be observed in silicates at temperatures below 1300 °C. Wuensch (1982) came to similar conclusion for refractory oxides. The above conclusion about the extrinsic nature of diffusion in silicates and refractory oxides at the laboratory conditions is very important from the point of view of extrapolation of the experimental data to temperatures of geological processes of interest since the experimental data are usually collected at temperatures that are higher than those at which these processes take place in nature. The Arrhenian relation could be extrapolated linearly to lower temperatures with, of course, due consideration for the statistical uncertainties associated with the regression of the experimental data. On the other hand, once the diffusion is in the extrinsic domain, it becomes vulnerable to Diffusion kinetics in minerals: Principles and applications 293 Fig. 6. Summary of Fe–Mg diffusion data in (a) garnet (open symbols: Ganguly et al., 1998; filled circles: Chakraborty & Rubie, 1996; circles with inscribed crosses: Cygan & Lasaga, 1985) and (b) olivine of composition Fo86 (Chakraborty et al., 1994; Meissner et al., 1998) as function of temperature. For garnet (a), all data have been normalised by Ganguly et al. (1998) to p = 10 kbar, and f O2 corresponding to those defined by graphite in the system C–O. For olivine (b) the filled symbols represent D(Fe–Mg) data derived from composition profile determined by analytical transmission electron microscope, whereas the open symbols represent those derived from compositional profiles determined by an electron microprobe. 294 J. Ganguly substitutions of ions that have different charge than the host species. Experimental studies on iron-bearing garnets, however, did not show any significant dependence of the diffusion coefficient on garnets from different sources (Chakraborty & Ganguly, 1992; Ganguly et al., 1998). This is fortunate, and is probably due to the fact, as discussed by Chakraborty et al. (1994), that the equilibrium vacancies controlled by the ferrous–ferric equilibrium in an iron-bearing mineral greatly dominates its vacancy content. Chakraborty et al. (1994) found that the activation energy for Mg self-diffusion in nominally pure synthetic forsterite (Fo100) at 1000–1300 °C is 400 (±60) kJ/mol, which is in contrast to that of 275 (±25) kJ/mol in San Carlos olivine (Fo92) within the same temperature range. Both sets of experiments were carried out by them following the same experimental technique. Also the D(Mg) in the San Carlos olivine had a much stronger fO2 dependence than that in Fo100 (the latter was essentially independent of fO2). Chakraborty et al. (1994), thus suggested that the diffusion mechanism in the nominally pure forsterite is different from that in olivine, which contains significant amount of Fe2+. When the FeO content falls below a critical value, the vacancies created by the Fe2+–Fe3+ equilibria have relatively minor role in the diffusion process. Liermann & Ganguly (2002) determined the Fe and Mg self-diffusion coefficients in spinel, (Fe2+,Mg)Al2O4, from modelling the Fe–Mg interdiffusion data obtained from diffusion-couple experiments at 20 kbar, 950–1325 °C. The retrieved activation energy is much lower than that determined by Sheng et al. (1992) for Mg tracer diffusion in spinel at 1 bar, 1261–1553 °C (202±8 kJ/mol vs. 343±8 kJ/mol). The latter workers used a tracer isotope of Mg on an essentially pure end member natural MgAl2O4 spinel (they did not report any FeO in their microprobe analysis of the sample, for which the wt% MgO, Al2O3, SiO2 and CaO add up to 100.88). Thus, it seems very likely, as discussed by Liermann & Ganguly (2002), that the high activation energy of Mg self-diffusion in the studies of Sheng et al. (1992) relative to that in their work is due to the extremely small, probably below the detection limit in microprobe analysis, amount of FeO content in the sample used by Sheng et al. (1992). It seems highly unlikely that the change of extrinsic–intrinsic transition of diffusion mechanism is responsible for the observed difference in the activation energies in the two sets of experiments. In summary, one must exercise great caution in the application of diffusion data obtained from pure crystals to natural samples that contain iron since there could be major difference between the defect formation energies in the two types of materials. Some modelling simplifications for geological problems Complex diffusion processes in geological and planetary systems are not often amenable to analytical treatment. These problems have to be dealt with numerically, and considerable progress has indeed been made along these directions over the past decade (e.g. Florence & Spear, 1993; Okudaira, 1996; Carlson, 2002; Tirone, 2002). However, some simplifications may be made to the problems of diffusion in natural processes, which in many cases make it possible to treat the problems analytically to gain useful insights about the behaviour of the system without requiring extensive computations. Some of these simplifications are discussed below. 295 Diffusion kinetics in minerals: Principles and applications Time dependence of diffusion coefficient Diffusion during geological and planetary processes usually takes place over a range of temperature, which changes as a function of time, t. Thus, the diffusion coefficient becomes a function of time. Problem with the time dependent diffusion coefficient can be handled in a simple way as follows. Let us define a new variable Γ as dΓ = D(t) dt so that the diffusion equation (Equation 3b) transforms to ∂C ∂ 2C = . ∂Γ ∂x 2 . (31) This equation may be viewed as a diffusion equation in which C is a function of a new variable Γ, and D = 1 (note, however, that Γ does not have the dimension of time). Solutions of the diffusion equation under isothermal condition can often be expressed in the form C(x, t) = f[x/(Dt)½]. One such solution is given in a later section (Eqn. 41). Solution for Equation 31 is the same as that for the standard diffusion Equation 3b, with Dt replaced by Γ. Now from the definition of Γ, we also have the relation t′ Γ = ∫ D(t )dt . (32) 0 This relation provides an important constraint on the thermal history of the sample in that the integral of D(t) dt over the postulated T–t path must equal the value of Γ derived from modelling the compositional zoning. Examples of the application of this concept to geological problems are discussed in the section on tectono-metamorphic processes. Let us consider a case in which the observed compositional zoning had developed during cooling, and suppose that the system had cooled according to an “asymptotic” relation 1 1 (33) = + ηt , T T0 where T0 is the initial temperature at the onset of cooling, and η is a cooling time constant with the dimension of K–1t–1. The Arrhenian relation of diffusion coefficient (Eqn. 30) then transforms to (34) Q 1 D = D0 e or − Q RT = D0 e − + ηt R T0 , D(t ) = D(T0 )e −η′t , where η′ = Qη/R, and D(T0) is the diffusion coefficient at T0. In general, the time dependence of D can be expressed as D(t) = D(T0)f(t). Substituting Equation 34 in 32, we obtain (Ganguly et al., 1994) t′ Γ ≡ ∫ D(t )dt = − o [ ] D (T0 ) −η′t′ [e − 1].. η′ (35) 296 J. Ganguly Since the time scale of geological processes is very large (at least for those for which cooling rates are of any interest), the above equation simplifies to t′ Γ ≡ ∫ D(t )dt = 0 D(T0 ) D (T0 ) R . = η′ Qη (36) Using an exponential cooling model, i.e. T = T0e–αt, Kaiser & Wasserburg (1983) obtained the following expression for the integral quantity: t′ Γ ≡ ∫ D (t )dt = 0 D (T0 ) RT0 αQ (37) Equations 36 and 37 were used to retrieve the cooling rates of meteorites from the values of Γ obtained from modelling the observed compositional zoning in minerals according to the appropriate solutions of the diffusion equation (Kaiser & Wasserburg, 1983; Ganguly et al., 1994). Characteristic diffusion coefficient Another useful simplifying concept in the treatment of natural processes in which D changes as a function of time due to the change of temperature is that of “characteristic temperature”, Tch, and the related diffusion coefficient D(Tch). In a non-isothermal process, it is always possible to find a temperature, Tch, such that t′ D(Tch )∆t = ∫ D(t )dt ≡ Γ . (38) 0 Chakraborty & Ganguly (1992) explored the characteristic temperature that satisfies the above relation in T–t cycles of metamorphic rocks, which are characterised by a single thermal peak. They found that Tch ≈ 0.97Tpeak, where Tpeak is the peak metamorphic temperature in K. Concept of effective binary diffusion in multi-component systems Although the phenomenological theory and mathematical treatment of multi-component diffusion is well developed in the linear domain, one can simplify the mathematical analysis of multi-component diffusion in some cases by using the concept of effective binary diffusion coefficient (EBDC), as if there are only two components, the diffusing solute and a solvent matrix. By applying chain rule to the expression of flux in a multicomponent system in the linear domain (Eqn. 17), we obtain ∂C ∂C ∂C ∂C J1 = − D11 + D12 2 + D13 3 + ... + D1( n −1) n−1 1 ∂C1 ∂C1 ∂C1 ∂x or J1 = − D1 (EB) ∂C1 , ∂x (39) (40) Diffusion kinetics in minerals: Principles and applications 297 where D1(EB) is the effective binary diffusion coefficient (EBDC) of component 1, and equals the quantity within the square brackets in Equation 39. It is important to note that, unlike true binary diffusion, Di(EB) for each component is different. Cooper (1968) showed that Di(EB) must be a single valued function of composition, and hence independent of the spatial concentration gradient, in order that Equation 40 has the property of Fickian diffusion, that is, flux ∝ force. Specifically, the concept of effective binary diffusion holds for diffusion in a semi-infinite diffusion couple in a multi-component system that does not show any inflection of the diffusion profile. Chakraborty & Ganguly (1992) discussed applications of this approach in modelling diffusion profiles in multi-component diffusion couple experiments. An example of application to a natural diffusion couple is discussed below. Time scales of tectono-metamorphic processes in collisional environments: Records in garnet zoning Garnet is the single most important mineral in the study of p–T–t history of metamorphic rocks. It participates in a large number of cation exchange and discontinuous reactions that are used to calculate the p–T conditions of rocks from the compositions of the coexisting mineral phases. It is amenable to geochronological studies using a number of decay systems, and often shows compositional zoning that preserve records of its tectono-metamorphic and exhumation history. In addition, since garnet is isotropic, diffusion in garnet has no directional dependence – a property that offers a practical advantage in the modelling of garnet compositional zoning. I will discuss here several types of compositional zoning in garnet in metamorphic rocks from collisional environments, and retrieval of the time scales of the attendant metamorphic and exhumation processes from modelling of the observed compositional profiles. Compositional zoning in a natural garnet–garnet diffusion couple Overgrowth of a mineral on itself is a well-documented petrographic feature in many terrestrial and planetary samples. When the overgrowth and core segment have significantly different compositions, as in polymetamorphic rocks, the composite sample forms a natural diffusion couple with continuous concentration profiles of components across the interface as a result of diffusion driven by the initial compositional contrasts between the core and overgrowth. The extent of these diffusion profiles depends on temperature and the time scale over which diffusion was effective. As an illustration of the retrieval of the time scale of a geological process from modelling compositional zoning of this type, I summarise below the analysis of a natural garnet–garnet diffusion couple by Ganguly et al. (1996a). Figure 7a shows a backscattered electron image of a composite garnet collected from the biotite grade rock from eastern Vermont. The couple consists of a grossular–spessartine garnet that had formed during regional metamorphism on an almandine core, which had crystallised during an earlier period of contact metamorphism at 411±5 Ma. The regional metamorphism took place during the Acadian 298 J. Ganguly Fig. 7. (a) Backscattered electron (BSE) image of the overgrowth of spessartine–grossular garnet on an almandine core during the Acadian orogeny, eastern Vermont, USA; (b) compositional profiles of the divalent cations across the core–overgrowth interface, as determined in an analytical transmission electron microscope (ATEM); (c) fits to the measured ATEM profiles in (b) according to the solution of Equation 41. The fits yield a value of ∫D(t)dt = 7.5 × 10–12 cm2 (modified from Ganguly et al., 1994). orogeny, which is believed to be a short-lived tectonic event that involved the collision between two plates and the closing of an ocean basin (Naylor, 1971). The diffusion induced compositional zoning between the two segments was too narrow to be clearly resolved by electron microprobe analyses because of convolution or spatial averaging effect (Ganguly et al., 1988). The compositional zoning was, thus, determined by an analytical transmission electron microscope (ATEM), which had negligible convolution effect because of the very small size of the excited analytical volume resulting from the small beam size and thinness of the sample to electron transparency. The results are shown in Figure 7b. Mg profile is not shown since the XMg is between 0.001 (overgrowth) and 0.06 (core). Since in this problem we are dealing with a semi-infinite diffusion couple, and there is no inflection in the diffusion profile, the diffusion problem may be treated in terms of an effective binary diffusion coefficient, as discussed above. Assuming that the 299 Diffusion kinetics in minerals: Principles and applications EBDC of a component is independent of distance within the diffusion zone, we seek solution of the diffusion equation (Eqn. 3b) for the conditions that the diffusion couple is semi-infinite so that the initial concentrations are preserved at sufficiently large distances from the interface, which is located at x = 0, and that there is no initial concentration gradient on either side of the interface. For an isothermal diffusion process, the solution is (Crank, 1983; Equation 2.14) Ci (t , x) = Ci (0) + ∆C 0 x 1 − erf 2 2 Di ( EB)t (41) where ∆C0 represents the initial difference between the concentrations of the components on the two sides of the couple, and Ci(0) is the lower of the two initial values of Ci. If diffusion had taken place under condition of variable temperature, then, as discussed above, Dt in the above equation is to be replaced by Γ (Eqn. 32). Using Equation 41, a single value of Γ = 7.5×10–12 cm2 was found to match well both Fe and Ca diffusion profiles (Fig. 7c). No attempt was made to fit the Mn profile because of the irregularity in the measured data points. On the basis of the Fe–Mn fractionation data between the overgrowth garnet and ilmenites, which are present as inclusions within this garnet, the peak metamorphic temperature for the biotite grade regional metamorphism was estimated to be 353±15 °C (the thermometric formulation is due to Pownceby et al., 1991, as corrected in Ganguly et al., 1996a). Using now the concept of characteristic temperature (Eqn. 38) and the above value of Γ, Ganguly et al. (1996a) obtained the following relation for the time scale of the metamorphic process: ∆t = 7.5 ×10 −12 cm 2 , Di ( EB) (Tch ) (42) where the term in the denominator represents the effective binary diffusion coefficient of either Ca or Fe at the characteristic temperature, which is ~ 0.97 × Tpeak. The calculation of EBDC of Ca and Mn requires data for the self-diffusion of Fe, Mg, Mn and Ca. Chakraborty & Ganguly (1992) determined the self-diffusion of the first three elements using diffusion couple made from natural almandine and spessartine crystals, but well constrained data for the diffusion of Ca was not available. However, one can simultaneously solve for both ∆t and DCa by calculating EBDCs of both Ca and Fe for guessed values of DCa according to Equation 24, and satisfying the condition that ∆t calculated from the DCa(EB) and DFe(EB) according to Equation 42 must be the same. This procedure yields ∆t = 47 Myr and DCa = 9.7 × 10–27 cm2/s at the inferred Tch = 343 °C. Ganguly et al. (1996a) discussed the potential uncertainties in the above calculation of time scale, and suggested ∆t ≈ 40–50 Ma as the probable time scale of biotite grade regional metamorphism reflected by the diffusion zoning across the core–overgrowth interface of garnet. 300 J. Ganguly Reaction-diffusion zoning in garnet: Pan-African tectono-metamorphic event Ganguly et al. (2001) have carried out modelling of compositional zoning in a garnet from granulite facies rocks in Søstrene Island, which is located in Prydz Bay, Antarctica. The garnet (Fig. 8) shows reaction textures corresponding to two metamorphic episodes, M1 and M2. The outer reaction texture formed during M1 by the breakdown of garnet according to Grt + Qtz → Opx + Plag at ~ 1000 Ma, while the fracture cleavage within the garnet and the included fine-grained symplectites, which formed by the reaction Grt → Opx + Plag + Spl, developed during M2 at ~ 500 Ma. The latter is believed to be associated with a regional Pan-African tectono-metamorphic event that has been interpreted to represent a continent–continent collision, followed by extensional collapse (Fitzsimons, 1996, 2000). The garnet shows Fe–Mg zoning parallel and normal to the fracture cleavage. The latter developed during M2 by a combined process of reaction and diffusion. The zoning parallel to fracture cleavage developed during both M1 and M2. The zoning normal to the fracture cleavage (Fig. 9) is a consequence of the fact that the composition of garnet in equilibrium with the symplectitic orthopyroxenes at the p–T condition of M2 is different from its initial composition, which is preserved in the core, and that the duration of M2 was too short to homogenise the garnet by volume diffusion. Using the Fe–Mg distribution coefficient between the garnet rim and adjacent orthopyroxenes and the thermometric formulation of Ganguly et al. (1996b) for Fe–Mg exchange between garnet and orthopyroxene yield T ≈ 730±20 °C at p = 6 kbar. This temperature estimate is in good agreement with that inferred by Thost et al. (1991) and Hensen et al. (1995) as the peak temperature of M2 at the same pressure. This agreement suggests that the compositional zoning in garnet developed and froze before the rock experienced sufficient cooling following peak M2, so that the reaction diffusion process may be approximated by an isothermal process. With the above framework, and assuming that the D(Fe–Mg) is not significantly affected by compositional change within the diffusion zone, the appropriate diffusion equation to be solved is Equation 7b, where v is the velocity of the garnet–matrix interface, which is set at x = 0, towards a fixed marker point at x > 0. The initial and boundary conditions are C = C0 at x > 0, t = 0 and C = Cr at x = 0, t > 0. The solution of the diffusion equation can then be easily obtained as a special case of that derived by Carslaw & Jaeger (1959, p. 388, Equation 7) for heat conduction in a moving body. The solution is C ( x, t ) = C0 + x + vt 1 (Cr − C0 ) erfc 2 2 Dt x − vt − vx + exp erfc D 2 Dt . (43) Ganguly et al. (2001) assumed that the breakdown of garnet within the fracture cleavage proceeded symmetrically in both directions so that v = RZ/t, where RZ is the observed half-width of the reaction zone. Substitution of this relation in Equation 43 eliminates one variable. C(x, t) can then be solved in terms of time (t) if the value of D(Fe–Mg) is known. The latter was calculated from the self-diffusion data of Fe and Mg in garnet (Ganguly et al., 1998) at the median composition of the diffusion zone according to Equation 10. Fig. 8. Photomicrograph showing reaction texture and fracture cleavage of a large garnet grain in a granulite sample from the Søstrene Island, Antarctica. The coarse outer grain symplectite consists primarily of ortho-pyroxene (Opx), and plagioclase (Plag), which were interpreted to have formed by the breakdown of garnet during decompression following an earlier metamorphism (M1) at ca. 1000 Ma. The finer grained symplectite mantling the garnet and within the fracture zones were interpreted to have formed by the breakdown of garnet according to Grt → Opx + Plag + Spl during a subsequent metamorphism (M2) accompanying Pan-African collision event at ca. 500 Ma. Scale is 1.7 mm. Cpx: clinopyroxene, Hbl: hornblende, Ilm: ilmenite, Mag: magnetite Diffusion kinetics in minerals: Principles and applications 301 302 J. Ganguly Fig. 9. Mg/(Mg + Fe) profile in garnet from Søstrene Island, Antarctica, normal to a fracture cleavage (see Fig. 8), and model fit to the data according to the solution of Equation 43. Reproduced from Ganguly et al. (2001). Modelling of the measured compositional zoning in garnet was carried out according to Equation 43 by linking it with a non-linear optimisation program (see Ganguly et al., 2001 for details). The initial composition, C0, and time, t, were the floating variables. The optimisation program finds values of the floating variables that lead to the best match between the calculated and the observed zoning data. This procedure yields t ≈ 5–16 Myr for the duration of peak M2 at the inferred temperature of 750–710 °C. The model fit to the measured compositional profile in garnet is illustrated by a solid line in Figure 9. From geochronological constraints in an adjacent area in Prydz Bay, Fitzsimons (pers. commun.) suggested 17±13 Myr for the duration of peak Pan-African metamorphism. Comparing the time scale inferred from modelling the compositional zoning of garnet with the geochronological constraints, Ganguly et al. (2001) suggested that the duration of peak M2 during the Pan-African event was probably not significantly in excess of 16 Myr. Cooling and exhumation of metamorphic rocks Diffusion in garnets becomes sufficiently rapid at the temperature of sillimanite grade to smoothen the compositional gradients that developed during the growth of a few mm size garnets at the lower grade conditions (Chakraborty & Ganguly, 1991). During the exhumation, however, the rim composition of garnet re-equilibrates with the matrix in response to the changing p–T condition, but the interior of the garnet does not come to equilibrium with the matrix because of the slow volume diffusion kinetics. Thus, the garnet crystals develop compositional gradients between the core and rim segments during the exhumation process, the extent of which depends on the cooling rate defined by the exhumation velocity, peak temperature and grain size. Typically, the rim Diffusion kinetics in minerals: Principles and applications 303 composition “freezes” at ~ 500–550 °C for cooling rates experienced during the exhumation of regionally metamorphosed rocks. Lasaga (1983) developed the theoretical groundwork for the retrieval of cooling rate from the forward modelling of retrograde compositional zoning. Several workers (Lindstrom et al., 1991; Chakraborty & Ganguly, 1992; Spear & Parrish, 1996; Weyer et al., 1999; Ganguly et al., 2000; Liermann & Ganguly, 2001; Ganguly et al., 2001) have since followed this basic idea to retrieve cooling rates of metamorphic rocks and planetary samples from the retrograde compositional zoning of minerals, especially garnet. Spear & Parrish (1996) and Weyer et al. (1999) compared the cooling rates obtained from modelling the retrograde compositional zoning of garnet in metamorphic rocks with those constrained by the closure age and closure temperatures (TC) of multiple geochronological systems. They found that the cation diffusion data in garnet by Chakraborty & Ganguly (1992) yield cooling rates that are in good agreement with those obtained from the geochronological data. I discuss below an example on the retrieval of cooling and exhumation rates from modelling the retrograde compositional zoning in garnets with homogeneous core composition. The sample is from northern Sikkim in the eastern Himalayas, where the metamophic isograds are disposed in an arcuate regional fold pattern. The thermal evolution and exhumation of the Himalayan metamorphic rocks have been subjects of extraordinary interest among earth scientists as these record the thermo-tectonic evolution of rocks in a major collisional and continental subduction environment, and also because of the presence of an inverted (Barrovian) metamorphic sequence almost along the entire length of the mountain belt. Ganguly et al. (2000) calculated the cooling and exhumation rates of rocks from the upper part of the High Himalayan Crystalline Complex (HHC) in the Sikkim–Darjeeling section on the basis of the retrograde compositional zoning of garnet crystals along with phase equilibrium constraints. The HHC is bounded on the south and north by the Main Central Thrust (MCT) zone and the South Tibetan Detachment System (STDS), respectively. The MCT is a southerly directed thrust (20–23 Ma) whereas the STDS is a northerly directed system of normal faults (16–23 Ma). Ganguly et al. (2000) determined the compositions of a number of garnet crystals along traverses that are normal to the traces of the interface between garnet and biotite. The zoning profiles for Mg along two traverses in one of the samples are illustrated in Figure 10. The compositions of biotite grains in contact with garnet were homogeneous and were essentially the same as those of other biotite grains within the same thin section. Because of its compositional homogeneity and large mass compared to that of thin garnet rims affected by cation exchange, it was assumed that the biotite behaved essentially as a homogeneous infinite reservoir of the exchanging components, Fe2+ and Mg. Ideally, the compositional zoning in a crystal used for retrieving cooling rate should be measured along a direction that is normal to the interface; otherwise, the length of the measured concentration profile would be longer (and consequently the retrieved cooling rate smaller) than that due to diffusion normal to the plane. The most definitive way to ensure normalcy of the traverse with respect to the interfacial plane is to obtain three- 304 J. Ganguly 0.30 (a) 0.26 X(Mg) (b) X(m) = X(t)/cosQ 0.22 Q Interface for (a) 46 Interface for (b) relative to (a) 0.18 0 40 80 120 Distance (µm) Fig. 10. Mg zoning in garnet in contact with a large mass of biotite in a granulite sample from the Sikkim–Darjeeling section of the eastern Himalayas, ~ 10 km south of the South Tibetan Detachment System. X(Mg) = Mg/(Mg + Fe). Line (a) is a fit to the filled squares according to the numerical solution of the diffusion equation, as discussed in the text. Line (b) is derived from (a) by 46° counterclockwise rotation of the garnet–biotite interface (see inset). X(m) in the inset stands for the measured length of the profile when the orientation of the interface deviates from the vertical by an angle Q, whereas X(t) is the length of the diffusion profile normal to the interface. Line (b) fits the data (circles) along another traverse in a garnet in the same thin section. The garnet–biotite interface for (b) is, thus, interpreted to have been rotated 46° counterclockwise with respect to that for (a). If it is assumed that the interface for (b) is not rotated from the vertical by more than 75°, then Q < 30°, which has insignificant effect on the retrieved value of cooling rate (CR) from the profile in (a). (Modified from Ganguly et al., 2000.) dimensional image of the rock by computer aided X-ray tomography, and cut the thin section normal to the interfacial plane (Carlson & Denison, 1992). As a practical substitute of this laborious procedure, which is rarely used, Ganguly et al. (2000) analysed the effect of geometric distortion of the zoning profile on the retrieved cooling rate, and chose a profile that did not seem to have been affected significantly by the rotation of the interface from the vertical (see Ganguly et al., 2000, for further details about this procedure). Multiplying both sides of Equation 31 by a2, we obtain dC d 2C , = dΓr dx r2 (44) Diffusion kinetics in minerals: Principles and applications 305 where Γr and xr are Γ x and xr = . 2 a a Both Γr and xr are dimensionless quantities. The following assumptions were made to model the retrograde compositional zoning in garnet in the Himalayas: (a) the cooling rate followed the ‘asymptotic’ relation given by Equation 33, (b) the interface composition of garnet was governed by exchange equilibrium between garnet and biotite, (c) biotite behaved as a homogeneous infinite reservoir of the exchanging components, as justified above, and (d) the garnet composition was homogeneous at the peak metamorphic condition (T0). Equation 44 was solved numerically subject to the boundary condition that dC/dx = 0 at x = a. The normalising distance a may be any distance from the interface where dC/dx = 0 (i.e. it need not be the distance to the core of the crystal). As above, the numerical program was linked to an optimisation program that was allowed to choose the best value of X(T0), but it returned the observed core composition of garnet as the best choice implying that it was not affected by diffusion. The same conclusion was arrived at from other observations. Figure 10 shows the model fit to the measured compositional data of garnet, which enables one to retrieve the quantity Γ, that is the integral of D(t)dt from the peak metamorphic condition to the “freezing” of the compositional profile in garnet. The retrieved value is 8.18×10–5 cm2. As a next step, Ganguly et al. (2000) calculated the exhumation velocity (Vz) of the rock by calculating the T–t path for a given Vz, integrating D(t)dt over this path, and repeating the process until the above value of ∫D(t)dt was obtained. This procedure yields Vz = 2 mm/year. However, the phase equilibrium constraints that are imposed by the retrograde reaction relations in the rock, which could be deduced from petrographic observations, require a nearly isothermal exhumation, corresponding to Vz ≈ 15 mm/year from a depth of ~ 34 km to ~ 15 km. The potential geodynamic implications of this change of exhumation velocity have been discussed by Ganguly et al. (2000, 2001). Γr = Diffusion modification of growth zoning in garnet A mineral develops compositional zoning during the growth process if it fractionates components with the matrix, and the diffusion within both the matrix and the mineral is slow compared to the growth velocity of the crystal. This may be understood by considering crystal growth in incremental steps. Owing to the fractionation of components with the crystal, the matrix in the immediate vicinity of the crystal (or “adjacent” matrix) would become depleted in the components that partition preferentially into the crystal, and enriched in those that have the reverse behaviour. Consequently, during the next growth step, the adjacent matrix would have a bulk composition that is effectively different from that in the previous step. Thus, the segment of the crystal that had grown in the second step would have a different composition than that in the previous step (because it had partitioned components with two different matrix compositions in the two steps). Continuation of the process would lead to the development of a zoned crystal. Such growth zoning is very common in the garnet zone rocks of regionally metamorphosed 306 J. Ganguly Barrovian sequence, in which the garnets typically show a bell shaped Mn profile and bowl shaped Fe, Mg and Ca profiles, with the extrema near the centre of the crystals. The retrograde compositional adjustment of the rim leads to two types of zoning profiles in garnet. If the crystal had homogenised earlier, then it would have a flat core and zoned rim, as in the Himalayan garnet sample discussed above. On the other hand, if the initial growth zoning were partly or completely preserved, then the crystal would have complicated zoning profiles in which some of the components could show extrema in their profiles from the centre to the rim of a grain. Modelling of these partially modified growth zoning profiles hold great promise in the retrieval of the full thermal history of the rock. Discussion of this modelling procedure is, however, beyond the scope of this review, as it requires consideration of crystal growth and resorption processes simultaneously with volume and intergranular diffusion kinetics. The interested readers are referred to Florence & Spear (1993), Okudaira (1996) and Carlson (2002) for an appreciation of the topic and interesting examples of applications to metamorphic processes. 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