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Fundamental thermodynamic relation

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In thermodynamics, the combined law of thermodynamics is simply a mathemtical summation of the first law of thermodynamics and the second law of thermodynamics subsumed into a single concise mathematical statement as shown below:

d U T d S + P d V 0 {\displaystyle dU-TdS+PdV\leq 0}

Here, U is internal energy, T is temperature, S is entropy, P is pressure, and V is volume.

Derivation

Starting from the first law, and neglecting differential details:

d U = d Q d W {\displaystyle dU=dQ-dW\,}

From the second law we have:

d S = d Q / T {\displaystyle dS=dQ/T\,}

Hence:

d Q = T d S {\displaystyle dQ=TdS\,}

By substituting this into the first law, we have:

d U = T d S d W {\displaystyle dU=TdS-dW\,}

Rearranging we have:

d U + d W T d S = 0 {\displaystyle dU+dW-TdS=0\,}

Letting dW be pressure-volume work, we have:

d U + P d V T d S = 0 {\displaystyle dU+PdV-TdS=0\,}

By assigning the quantity to the left of the equals sign the symbol G, as Willard Gibbs did in 1876, this reduces to the following at thermodynamic equilibrium:

d G = 0 {\displaystyle dG=0\,}

Or for a spontaneous process:

d G 0 {\displaystyle dG\leq 0\,}

Thus, this expression is referred to by many as the combined law of thermodynamics; Gibbs showed that deviations of this quantity could be used to predict the direction of various natural chemical processes.

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