Point defects. process complicated. Now we shall discuss on defects, which will help to understand the atomic mechanism of diffusion.

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Point defects Diffusion of elements is possible because of the presence of defects. For example, substitutional diffusion occurs because of exchange of an atom with acancies. Further, impurities are present at the interstitial positions, which could diffuse to any neighboring acant interstitial sites. This is called interstitial diffusion. Certain concentration of these impurities are always present in the pure elements in equilibrium condition, which will be discussed here. Further in the intermetallic compounds (ordered phases), antisites defects also could be present along with acancies. Moreoer, different sublattices could hae different concentration of process complicated. defects, which makes the diffusion Now we shall discuss on defects, which will help to understand the atomic mechanism of diffusion.

Equilibrium point defect calculations Let us not get confused with the structural defects present in pure elements. To understand simple atomic mechanism of diffusion at this point, we shall calculate the equilibrium concentration of point defects that is the equilibrium concentration of acancies and interstitial atoms in pure elements Interesting point to be mentioned here that unlike dislocations, grain boundary or interfaces, point defects are equilibrium defects. It means that the system will try to hae certain concentration of defects to decrease the free energy. Let us first calculate the equilibrium concentration of acancies, because of which lattice substitutional diffusion is possible

Equilibrium acancy concentration in a pure element Pure elements A and acancies (V) can be considered as a mixture of two entities and follow the similar treatment as we did to calculate the total free energy after mixing of elements A and B. It can be easily isualized how the moement of atoms can create acancies in the material in few steps. Equilibrium number of acancies is so small that we can neglect the interaction between them. This means that we are neglecting V-V interactions. This also means that we are, at this point, neglecting the presence of diacancies, which are actually present in the material.

If we consider that the number of acancies is ery small then the increase of enthalpy because of formation of acancies can be written as H H H is the mole fraction of acancy and is the increase in enthalpy because of one mole of acancies There will be the change in the pattern of ibration of atoms next to acancies because of extra free space. The increase in (thermal) entropy because of the extra freedom of ibration can be written as S thermal = S SS is the increase in entropy for one mole of acancies In both the cases, we are actually assuming linear relationship because of ery small concentration of acancies. Note: In the case of entropy change of A-B mixture, we did not consider the thermal entropy change, since we are considering the change at a particular temperature. Howeer, in this case, although we are considering again at a particular temperature, we still need to consider the contribution because of the change in ibration pattern of atoms next to acancies.

Further there will be change in configurational entropy considering the mixing of A and V and can be expressed as (Note that we are considering A =1 ) config [ ln + ln ] = R[ ln + ( 1 ) ln( )] S = R 1 A A + Total entropy of mixing mix [ ln + ( 1 ) ln( )] S = S R 1 Total free energy in the presence of acancies G = G A + G = G = G A A + H T S + H T (Total contribution from thermal and configurational entropy) { S R[ ln + ( 1 ) ln( 1 )]} Note here that G of element A when acancies are present decreases. So always there will be acancies present in materials. Further G decreases to a minimum alue and then increases with the further increase in acancy concentration. So, in equilibrium condition, certain concentration of acancies will be present, which corresponds to G e.

Since the slope is zero at the minima, we can find the equilibrium acancy concentration from dg d H = 0 T S 1 1 + RT ln + ln 1 = 1 ( ) ( 1 ) 0 ( ) Since the number of acancies that can be present in the system is ery small 1 1 H T S + RT ln = 0 The relation for equilibrium concentration of acancies can be written as e = = exp H T S RT G = exp RT Although there is increase in configurational entropy because of the presence of acancies, it is not included in the actiation energy barrier, G Although there is actiation energy barrier present because of formation, acancies will still be present because of oerall decrease in free energy of the materials.

From the equation in the preious slide, we can also write e 0 H = exp RT H is the actiation enthalpy for the formation of acancies and 0 S = exp is the pre-exponential factor. R 10-2 Vacancy concentration (m mole fraction ) 10-4 10-6 10-8 10-10 10-12 10-14 The change in concentration of acancies in pure Cu is shown in the graph, considering actiation energy for acancy formation to be 83.7 kj/mole. 10-16 0 200 400 600 800 1000 Temperature, T ( o C) The concentration of acancies in mole fraction at 1000 C is 3.68x10-4. That means in a cube of 14 atoms in each direction, only one acancy will be present in Cu at this temperature!!!

Experimental determination of acancy concentrations There are few techniques aailable following which one can measure the concentration of acancies at certain temperature to determine the actiation energy for acancy formation In practice, mainly three techniques are followed: by thermal expansion measurements, by measuring resistiity after quenching and using positron annihilation technique. We shall consider these techniques in our discussion one by one. From thermal expansion experiments Expansion of olume of a metal because of increasing temperature happens mainly because of two reasons: (i) expansion in lattice parameter and (ii) creation of more acancies. Volume expansion means the increase in lattice sites. Fraction of olume change is actually equal to the fraction of change in lattice sites, n/n. The fraction of change in linear dimension is l/l and the fraction of change in lattice parameter is a/a. So the linear change because of creation of extra sites/acancies is ( l/l - a/a).

In an isotropic structure, the change in olume is three times to the linear change and we can write n/n = 3( l/l - a/a) We are just adding from eery linear change. If acancies are added in x direction only, there will be no change in other directions. So if we add the changes from eery direction it will gie total number of change in the sites. Although it seems ery straightforward equation, it is ery difficult to determine experimentally. We hae preiously explained that the concentration of acancies een near the melting point is in the order of 10-4. So een if we show higher tolerance and ready to accept 5% (0.05 fraction) error, we need to be able to measure the length of the material and lattice parameter change in the range of 5x10-6! Further, the change in length and lattice parameter should be measured simultaneously at a particular temperature. Typical deiation is seen as shown in the figure. l/l In aluminium it was measured and the relation was found a/a n/n = exp(2.4)exp(-0.76/kt) It can be seen as or V GV S = exp = exp RT R SV HV exp exp k kt V H exp RT per atom So enthalpy of acancy formation is 0.76 ev/atom equialent to 73 kj/mol. V per mol

The relation described aboe can be used in polycrystalline material with random orientation of grains or single crystals with cubic lattice. In a polycrystal it can gie some error, because we neglect the presence of grain boundaries and grain growth. This relation should be modified to use in non cubic single crystals. For example Sn has tetragonal structure and the relations used should be V n L = = 2 n L a a a + L L c c c where a and c are the lattice parameters.

From resistiity measurements Equilibrium concentration of acancies depend on temperature. Higher the temperature higher the concentration of acancies. Similarly resistance of a material is also a function of temperature. Resistance comes mainly from two contributions: lattice ibrations and defects. If we are able to control other defects like impurities, dislocation, grain boundaries etc., we can write ρ = ρ T + ρ V where ρ is the change in total resistiity, ρ T is the change in resistiity because of lattice ibration with increasing temperature and ρ V is the change in resistiity because of the change in acancy concentrations. When the temperature is increased at higher temperature, material will hae higher equilibrium concentration of acancies. Vacancies are originated from dislocations of grain boundaries, which act as source. Vacancies get dispersed by the diffusion process.

When temperature is decreased the equilibrium concentration decreases and acancies are absorbed by the dislocations or the grain boundaries. These then act as sink. If the metal is suddenly quenched (for example in liquid nitrogen at 77 K) from high temperature to a lower temperature, acancies will not be able to diffuse to sinks. Een at low temperature diffusion rate is much lower. So the metal will hae extra acancies. So when resistiity is measured in a metal first at low temperature, it will hae resistance from lattice ibration and equilibrium concentration of acancies. Further when resistance is measured on the same metal at the same temperature but after quenching from a high temperature, resistance from lattice ibration will be the same but the resistance from the acancies will be higher. So the difference is resistance will be proportional to the difference in acancy concentration. N = α ρ α is the proportionality constant V Since the difference in acancy concentration at these two different temperatures will be in many orders of magnitude we can write S α ρv = N N = exp R H ρ = Aexp RT H exp RT A is a constant So measurements after quenching from different temperature will gie the alue for actiation enthalpy for acancy formation.

Positron annihilation measurements Because of decay of a radioactie isotope, positrons with equal mass but opposite sign to electron emit. These positrons combine with electron to produce gamma rays with particular energies. When these positrons are bombarded on a solid material it may trael for some time in the range of pico seconds before it combines with electrons. Positrons hae a tendency to get trapped in a bound state in a acancy. Since acancies do not hae core electrons compared to other atoms, it takes longer time for annihilation in a acancy. So higher the concentration of acancies, higher the half life time for annihilation. If at a particular temperature half life does not increase beyond a certain point, it indicates the equilibrium concentration of acancies. Based on this half life time one can calculate the equilibrium concentration of acancies. Since the relations are bit complex, we shall not discuss it here. It is found that the positron annihilation technique is one of the most accurate techniques to measure the concentration of acancies. Thermal expansion technique is rather least reliable.