Energy Changes and Equilibrium Principles
This section delves deeper into the relationship between energy changes, entropy, and chemical equilibrium. It emphasizes that equilibrium is the result of competing tendencies towards minimum energy and maximum disorder.
Definition: Equilibrium in chemical reactions is achieved when the system reaches a balance between the tendencies for minimum energy and maximum disorder.
The chapter outlines key conditions for equilibrium:
- The system must be closed, allowing for heat exchange but no mass transfer.
- The temperature must be constant.
Different types of systems are introduced:
- Open systems: Allow both energy and matter exchange
- Closed systems: Allow energy exchange but not matter
- Isolated systems: Allow neither energy nor matter exchange
Highlight: In a chemical equilibrium, macroscopic (visible) changes cease, but microscopic processes continue.
An important characteristic of equilibrium is that the concentrations of reactants and products remain constant over time. This is illustrated using the example of the Haber process for ammonia synthesis:
N₂(g) + 3H₂(g) ⇌ 2NH₃(g)
The chapter explains how the concentrations of N₂, H₂, and NH₃ change initially but remain constant once equilibrium is reached.
Example: In the Haber process, the concentrations of N₂, H₂, and NH₃ change until equilibrium is reached, after which they remain constant despite ongoing microscopic reactions.