Detailed Summary of Thermal Equilibrium
In thermodynamics, thermal equilibrium refers to a state where the macroscopic variables defining a system, such as pressure, volume, temperature, mass, and composition, remain constant over time. A system is considered to be in thermal equilibrium when there are no net energy exchanges between it and its surroundings or other systems.
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Equilibrium Definition: The notion of equilibrium differs from that in mechanics; while mechanical equilibrium pertains to net forces and torque being zero, thermodynamic equilibrium involves static macroscopic properties being invariant with time. This means no changes occur in the state's defining variables.
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Diathermic vs Adiabatic Walls: The interaction between systems can be examined through the types of walls that separate them: diathermic walls allow heat flow, facilitating energy exchange and leading to thermal equilibrium, while adiabatic walls prevent energy flow.
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Example Setup: Consider two gases in separate containers. If isolated by an adiabatic wall, the pressures and volumes of both gases will stabilize without external influence. However, once the wall is replaced with a diathermic one, heat can flow, thus equalizing their temperatures over time. Ultimately, reaching thermal equilibrium requires the temperatures of both systems to equalize.
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Significance of Temperature: The concept underlying thermal equilibrium is most closely related to temperature. Two systems in thermal equilibrium with a third system exhibit equal temperature values, which is governed by the Zeroth Law of Thermodynamics. This lays the foundation for understanding a temperature scale, which is crucial for thermodynamic measurement.
Overall, the principle of thermal equilibrium is integral to thermodynamic laws, influencing heat transfer, energy conservation, and system interactions.