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The Second and Third Laws of Thermodynamics                                  89

            is constant (at atmospheric pressure) in a laboratory setting unless the system is sealed. Thus,
            J.W. Gibbs (1839–1903) defined what is now known as the ‘‘Gibbs free energy, G,’’ which has
            proved to be very useful. Gibbs defined G   H   TS and once again all the terms are in terms of
            energy units. This time we add and subtract VdP as well as SdT to the first law:

                  dU ¼ TdS   PdV þ SdT   Sdt þ VdP   VdP ¼ d(TS)   SdT   d(PV) þ VdP
            so that we find

                    dU þ d(PV)   d(TS) ¼ SdT þ VdP ¼ d(U þ PV   TS) ¼ d(H   TS) ¼ dG

            and so we obtain

                                           dG ¼ SdT þ VdP:

            The equation of G ¼ H   TS is a better indicator of an equilibrium so that when dT and, especially,
            when dP are zero, then dG ¼ 0 indicating an equal trade-off between increasing entropy and
            decreasing energy. Next, consider the definition of H   U þ PV and use the two conditions
            above to find that that there is a fourth equation for dH as found from

                     dH ¼ dU þ PdV þ VdP ¼ (TdS   PdV) þ PdV þ VdP ¼ TdS þ VdP:

            We have just rushed over more than 100 years of developments in thermodynamics by focusing on
            key equations, and we can consolidate the ‘‘essential’’ knowledge for this text as


                                                      qT      qV
                               dH ¼ TdS þ VdP   and       ¼        ,
                                                      qP      qS
                                                          S       P

                                                      qT        qP
                               dU ¼ TdS   PdV   and        ¼         ,
                                                      qV        qS
                                                          S        V

                                                          qS      qV
                               dG ¼ SdT þ VdP    and           ¼       ,
                                                          qP      qT
                                                              T       P

                                                        qS      qP
                               dA ¼ SdT   PdV    and        ¼        :
                                                        qV      qT
                                                           T        V
            This is pretty much the jackpot of equations for thermodynamics and now reveals why we chose to
            prove the Carnot cycle relationship so that we could get to dq rev ¼ TdS. Note the alternating pattern
            of signs and the variables when assembled in the order ‘‘HUGA,’’ which may help organize the
            equations in your mind. We could spend a lot more time on the history of the Helmholtz and Gibbs
            free energy derivations, but in this course on ‘‘essentials,’’ we swam through a narrow intellectual
            cave (Carnot cycle) to reach a beautiful expansive blue grotto of valuable knowledge with these
            eight equations. The four auxiliary partial derivative equations are called the ‘‘Maxwell relation-
            ships.’’ They result from the fact that H, U, G, and A are all state variables with ‘‘exact differentials.’’
            Since it does not matter, which of the two variables change in either order for the basic four
            ‘‘HUGA’’ equations, we can do the second derivatives in either order.
                                                       2
                                   qH                 q H       qT
              dH ¼ TdS þ VdP so         ¼ T and then        ¼        where we have used the
                                   qS                 qP qS     qP
                                       P                            S
            convention that the most recent derivative is with respect to the lower left variable in the second
            derivative.
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