Lecture 21: Complex reactions (continued) Review o Methods for determining reaction order. o Overall composition analysis o Using Excess of components o Method of initial rates o Complex processes o Bifurcation o Chain Reactions o Example: Blood clotting Today o Reversible reactions o Concept of microscopic reversibility o Analysis of complex reactions and approximations o Initial rates o Prior Equilibrium approximation o Steady state approximation o Effect of temperature o Arrhenius theory o Eyring theory: Transition State Complex o Electron transfer reaction (Marcus theory) o Effect of salts Reversible Reactions So far we have considered kinetics of irreversible reactions. But most biological reactions are controlled through reversibility. That is, when concentration of products increases significantly the rate of its formation is reduced. To describe a simple first order reversible kinetics : AB Let the rate of forward reaction be k1 and reverse reaction be k-1.. Now the let initial concentration of A and B be A0 and B0 and the equilibrium concentrations be Aeq and Beq. That is, after sufficient time is allowed to pass (5-10 half lives), the concentration of A and B will become independent of time. From mass balance considerations, we can write: x A Aeq Beq B dA k1 A k 1 B k1 [ Aeq x] k 1 [ x Beq ] dt dA dx (k1 k 1 ) x dt dt x ln (k1 k 1 )t x0 A Aeq ln A A eq 0 B Beq ln B B eq 0 (k1 k 1 )t This is still a first order equation, except that concentrations are measured with respect to equilibrium concentration. Concept of microscopic reversibility One of the key notions we must keep in mind concerning the reversible reactions is that it must be consistent with the reversibility principle we studied in thermodynamics. The principle can be adapted in following way. Every reaction, or set of reactions must be microscopically reversible at every stage. Consider a following thermodynamic path for a system involving three components A, B and C. This scheme is not consistent with the principle of microscopic reversibility since B cannot be converted back to A in the first step. Similar argument can be applied to C. So, to be consistent we must write: Analysis of complex reactions and approximations Thus, the main problem for the kinetic experiments is the number of independent rate constants that must be determined. Even for simple reactions, as seen above, this poses significant challenges. As expected, we can study the reaction for very short initial duration to determine the kinetic order. The method also yields information about how the rate of reactant disappearance depends on the concentrations of the reactants. This is, the so-called method of initial rates, useful in the initial stages and is inadequate for the later stages of complex kinetics. Therefore, to study multi-step reactions two important assumptions are evoked, namely, (1) prior equilibrium (2) steady state approximations. For a two- step reaction: A B X step 1 X P step 2 In prior equilibrium approximation method, we set step 1 to be a fast reaction and assume that step 2 is the ratedetermining step. In steady state approximation, we suggest that the concentration of the intermediate X is small (implying now that the step 1 is slow and step 2 is fast) or constant. Using these of assumptions, it is possible to simplify the kinetic equations greatly. These are such broad sweeping assumptions that leave us with several possible schemes that are consistent with a given set of experimental data. Therefore, design and selection of experimental methods to elucidate kinetics of complex reactions takes time as well as tenacity. Prior Equilibrium Approximation A B X ( fast ) X P ( slow) since the first reaction is fast, a “quasi-equilibrium’’ is established and a finite concentration of X is developed. This implies the rates of forward and reverse reactions in the first step become equal and using this equilibrium we can estimate the concentration of X readily. k1 A.B k 1 X K eq k1 X k 1 A.B dP k 2 X k 2 K eq . A.B dt v v 2 v1 v 2 v Steady State Approximation A B X ( slow) X P ( Fast ) In the case of steady state approximation, we have low concentration of X and setting it’s rate of formation to be zero: dX k1 A.B k 2 X 0 dt dP k 2 X k1 A.B dt Note the difference between the prior equilibrium case and the steady state case. Temperature dependence of rate constant Arrhenius model Transition state theory M N ( fast ) MN * ( slow ) P k T dP k 2 K eq M .N k 2 B dt h Gcomplex RT ln{ K eq ) Marcus theory of electron transfer reactions One of the most common chemical reactions is the transfer of electron (i.e. oxidation-reduction). Marcus envisioned the structure of free energy of the reaction state complex, in terms of stabilization of the complex brought about by the solvent and electrostatic interactions. Consider a simplest reaction, where the free energy of the product and the reactant is identical. Fe 3 *Fe 2 Fe 2 *Fe 3 where the star specifies a radioactive Fe species. In this case, the suggested form of the free energy of the electron Fe/Fe complex is: G 0 1 1 1 1 2 1 G 1 (e) 2 4 2a1 2a2 R n where G0 is standard free energy of the reaction, and is the reorganization energy of the complex including solvent and reacting molecular contributions. n and are solvent refractive index and dielectric constant respectively. a’s are the radii of the ions and R is the center to center distance between the reactants. e is the charge transferred. Thus, unlike the empirical Arrhenius equation, Marcus theory gives more insight about how electron transfer and solvent reorganization effects influence the rate of electron transfer processes. This approach is especially valuable in the studies of photosynthesis. Ionic Reactions and Salt effects. Eyring’s thermodynamic model for the rate constant relates the rate constant to the equilibrium constant for reactant and transition state complex. We can develop, how a given reaction will be influenced by ionic species that are commonly present in biological fluids. Here, we will borrow from our development of activities and activity coefficients from the last quarter. M N ( fast ) MN * ( slow ) P dP k 2 K eq M .N k 2 MN * dt cMN * MN * MN * K eq M .N c N N c M M v v k2 k BT h k BT N M cM c N h MN * log( k ) log( k 0 ) 2.0.51Z M Z N I Thus as ionic strength is increased, the k value increases exponentially!