By contacting two bodies that are at different temperatures, the one that is warmer yields part of its energy to the one with the lowest temperature, to the point where both temperatures are equal.
See also: Difference between Heat and Temperature
Theoretically, thermal equilibrium is fundamental in what is known as the Zero Law or the Zero Principle of Thermodynamics, which explains that if two separate systems are at the same moment in thermal equilibrium with a third system, they are in thermal equilibrium one with another. This Law is fundamental to the entire discipline of thermodynamics, which is the branch of physics that deals with describing the states of equilibrium at a macroscopic level.
The equation that gives rise to the quantification of the amount of heat that is exchanged in the transfers between the bodies has the form:
Q = M * C * ΔT
Let Q be the amount of heat expressed in calories, M the mass of the body under study, C the specific heat of the body, and ΔT the temperature difference.
In an equilibrium situation, the mass and the specific heat retain their original value, but the temperature difference becomes 0 because the equilibrium situation where there are no temperature changes was precisely defined.
Another important equation for the idea of thermal equilibrium is the one that seeks to express the temperature that the unified system will have. It is accepted that when a system of N1 particles, which is at temperature T1, comes into contact with another system of N2 particles, which is at temperature T2, the equilibrium temperature is obtained by the formula:
(N1 * T1 + N2 * T2) / (N1 + N2) .
In this way, it can be seen that when both subsystems have the same number of particles, the equilibrium temperature is reduced to an average between the two initial temperatures. This can be generalized for relationships between more than two subsystems.
See Also: Types of temperature Scales
Here are some examples of situations where thermal equilibrium occurs:
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