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Entropy is a thermodynamic state variable that quantifies the probabilistic distribution of a system’s accessible microscopic configurations (microstates). In classical thermodynamics it is defined through measurable macroscopic quantities and appears naturally in reversible heat transfer, while in statistical mechanics it is linked to the number (and probabilities) of microstates consistent with the system’s macroscopic constraints. Because entropy depends only on the system’s equilibrium state—not on the path taken to reach it—it functions as a state function. Entropy is central to the second law of thermodynamics: for an isolated system, the total entropy cannot decrease and spontaneous processes drive the system toward equilibrium, where entropy is maximized. “Higher” entropy corresponds to energy being more dispersed (more ways to arrange microstates), while “lower” entropy corresponds to more concentrated or ordered energy. As a result, entropy increase is tied to irreversibility and the direction of time, and it also limits how much work a system can produce. Although entropy cannot be directly observed, it can be calculated from heat capacity data and from statistical descriptions of microstates; its different definitions (thermodynamic and statistical) are consistent under the appropriate ensembles.
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