Thermal equilibrium is a state where different parts of a system are at the same temperature, with no net energy flow between them. At this point, the system's properties, including temperature, distribute uniformly across it.
In thermodynamics, reaching thermal equilibrium is crucial for understanding distribution laws like Boltzmann distribution
- Boltzmann distribution describes how energy states are populated in such a system.
- While energy varies with temperature, at thermal equilibrium the probability of finding a system in a specific energy state is predictable.
- This predictability aids in calculating concentration ratios, such as seen in different RNA structures under certain conditions.
Achieving thermal equilibrium ensures calculations, like those involving Gibbs free energy, are accurate and reflective of real biological systems.