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S1.1 - Introduction to the particulate nature of matter S1.2 - The nuclear atom S1.3 - Electron configurations S1.4 - Counting particles by mass - The mole S1.5 - Ideal gases S2.1 - The ionic model S2.2 - The covalent model S2.3 - The metallic model S2.4 - From models to materials S3.1 - The periodic table - Classification of elements S3.2 - Functional groups - Classification of organic compounds R1.1 - Measuring enthalpy changes R1.2 - Energy cycles in reactions R1.3 - Energy from fuels R1.4 - Entropy and spontaneity AHL R2.1 - How much? The amount of chemical change R2.2 - How fast? The rate of chemical change R2.3 - How far? The extent of chemical change R3.1 - Proton transfer reactions R3.2 - Electron transfer reactions R3.3 - Electron sharing reactions R3.4 - Electron-pair sharing reactions

R1.4 - Entropy and spontaneity AHL

1.4.1 Entropy (AHL) 1.4.2 Gibbs Free Energy and Spontaneity (AHL) 1.4.3 Interpreting ∆G and Temperature Effects (AHL) 1.4.4 ∆G, Equilibrium and Reaction Quotient (AHL)

Gibbs Free Energy and Equilibrium HL Only

Specification Reference R1.4.4

Quick Notes:

  • As a reaction moves toward equilibrium, ΔG increases, becoming less negative, until ΔG = 0 at equilibrium.
  • Two key equations:
    • ΔG = ΔG + RT lnQ
    • ΔG = −RT lnK
  • Where:
    • ΔG = Gibbs energy at any point in the reaction
    • ΔG = standard Gibbs energy change
    • R = gas constant = 8.31 J mol⁻¹ K⁻¹
    • T = temperature in Kelvin
    • Q = reaction quotient
    • K = equilibrium constant
  • If ΔG < 0 then K > 1 and products favoured
  • If ΔG > 0 then K < 1and reactants favoured

Full Notes:

How Is ΔG Related to Equilibrium?

Essential ideas:

Understanding the link:
Chemical reactions tend to move toward a more stable state – in thermodynamic terms, a state of lower Gibbs free energy.

At equilibrium:

The Equation: ΔG = ΔG + RT lnQ

Most reactions don't occur under standard conditions. The equation below allows us to calculate Gibbs free energy change (ΔG) at any stage of the reaction and not just under standard conditions:

IB Chemistry formula showing ΔG = ΔG⦵ + RT lnQ with definitions of terms.

How Is Q Calculated?

Q is the reaction quotient reflects the ratio of products to reactants at a specific moment in time.

It is calculated just like K (the equilibrium constant - see here for more detail), but using the current concentrations or pressures:

Q = [products]ⁿ / [reactants]ᵐ

For example, for a general equation such as:

IB Chemistry general reaction between A + B forming C + D.

The expression for Q is:

IB Chemistry Expression for reaction quotient Q.
Photo of Matt
Matt’s exam tip

Don’t get confused about K and Q!
Q is the ratio of product to reactant concentrations at any moment in time - the system doesn't have to be at equilibrium.
K is what the ratio of product to reactant concetrations is at equilibrium.

If Q = K then that means the reaction is at equilibrium, however if Q doesn't equal K, then that the means the system isn't at equilibrium and the reaction will continue to proceed in the direction that will make Q = K and reach equilibrium.

What Does Q Tell Us About Spontaneity?

At Equilibrium: ΔG = –RT lnK

At equilibrium, ΔG = 0, so the previous equation becomes:

IB Chemistry formula showing ΔG⦵ =  - RT lnK

This links thermodynamic data (ΔG) to the equilibrium constant (K):

ΔG K value Reaction position
ΔG < 0 K > 1 Products favoured
ΔG = 0 K = 1 Equal amounts of reactants/products
ΔG > 0 K < 1 Reactants favoured

Summary

Linked Course Question

Reactivity 2.3 — Linked Course Question

What is the likely composition of an equilibrium mixture when ΔG is positive?

If ΔG is positive, the equilibrium position lies toward the reactants, meaning the equilibrium mixture is mostly reactants with only a small amount of products formed. The reaction is not spontaneous under standard conditions.