z state the third law of thermodynamics; z state the relationship between G, H and S ; z derive the relation Δ Gsystem = T Δ Ssystem ; z state Gibbs energy criterion for spontaneous process Δ G < 0 for a spontaneous process Δ G = 0 at equilibrium Δ G > 0 for a non-spontaneous process z define standard Gibbs energy of formation of a subtance; z relate the standard Gibbs energy change with the equilibrium constant and z solve numerical problems
Question
z state the third law of thermodynamics; z state the relationship between G, H and S ; z derive the relation Δ Gsystem = T Δ Ssystem ; z state Gibbs energy criterion for spontaneous process Δ G < 0 for a spontaneous process Δ G = 0 at equilibrium Δ G > 0 for a non-spontaneous process z define standard Gibbs energy of formation of a subtance; z relate the standard Gibbs energy change with the equilibrium constant and z solve numerical problems
Solution
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The third law of thermodynamics states that the entropy of a perfect crystal at absolute zero is exactly equal to zero. This law provides an absolute reference point for the determination of entropy.
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The relationship between Gibbs free energy (G), enthalpy (H), and entropy (S) is given by the equation: G = H - TS. This equation is known as the Gibbs-Helmholtz equation.
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To derive the relation ΔGsystem = TΔSsystem, we start from the Gibbs-Helmholtz equation. We know that ΔG = ΔH - TΔS. For a system at equilibrium, ΔG = 0, so 0 = ΔH - TΔS. Rearranging this equation gives us ΔH = TΔS. Since ΔH is the change in the system's enthalpy, we can write this as ΔGsystem = TΔSsystem.
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The Gibbs energy criterion for a spontaneous process is as follows:
- ΔG < 0 for a spontaneous process
- ΔG = 0 at equilibrium
- ΔG > 0 for a non-spontaneous process
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The standard Gibbs energy of formation of a substance is the change in Gibbs free energy that accompanies the formation of 1 mole of that substance from its component elements, at their standard states (the most stable form of the element at 25 °C and 1 bar).
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The standard Gibbs energy change is related to the equilibrium constant by the equation ΔG° = -RTlnK, where R is the gas constant, T is the temperature in Kelvin, and K is the equilibrium constant.
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To solve numerical problems involving these concepts, you would typically be given some of the variables in the equations above and asked to solve for the others. For example, you might be given ΔH, T, and ΔS and asked to calculate ΔG. You would use the Gibbs-Helmholtz equation to do this. Or you might be given ΔG° and T and asked to calculate K. You would use the equation ΔG° = -RTlnK to do this.
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