Jump to content

Fundamental thermodynamic relation

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Sadi Carnot (talk | contribs) at 18:52, 26 July 2006 (started article (needs more work)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

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:

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:

From the second law we have:

Hence:

By substituting this into the first law, we have:

Rearranging we have:

Letting dW be pressure-volume work, we have:

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:

Or for a spontaneous process:

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.