Page 97 - Essentials of physical chemistry
P. 97

The First Law of Thermodynamics                                              59

            thermodynamics is not complicated but more thinking is required as to the sign of the quantities.
            Thermodynamics encourages thinking more with less automatic use of formulas.
              We have mentioned the relationship U ¼ (3RT=2) and DU ¼ (3R=2)DT. For a Boltzmann
            atomic gas, we can take the derivative with respect to temperature while holding the volume
            constant, recognizing that the laboratory relationships would involve P, V, T, n so maybe at least
            one other variable is involved assuming that knowledge of two of the three variables would
            determine the third under some equation of state for a fixed amount (moles) of gas:


                                    qU         qU                qU
                                                                      dV,
                             dU ¼        dT þ       dV ¼ C v dT þ
                                    qT         qV                qV
                                        V          T                 T
            assuming constant moles.
                                                   qU
                                                        . This also brings up the realization that for
              Thus, we introduce the new quantity C V
                                                   qT
                               qU       qU             V
            an ideal gas we have    ¼        ¼ 0, since the energy of the ideal gas only depends on
                                qV      qP
                                   T        T
            temperature. In fact we can enlarge the definition of an ideal (monoatomic) gas to mean:
            Ideal Gas
              1. PV ¼ nRT

                  qU       qU
              2.       ¼       ¼ 0
                  qV       qP
                      T       T
            We note that these conditions of energy independence from T and P may not be true for real gases or
            even for the van der Waals gas but they are a reasonable approximation at low pressure and high
            temperature where the ideal gas equation is good.
            ENTHALPY AND HEAT CAPACITIES

            Next we come to a practical problem: What happens even in household kitchens when a sealed container
            is opened? Soft drinks are under some pressure in their containers, so pressure is released when the
            container is opened. Old fashioned glass milk bottles brought in from the cold would often pop out their
            cardboard top plugs when warmed in a kitchen environment due to the Charles–Gay-Lussac relation-
            ship. Thus, we see opening storage containers involves a small but nonzero pressure push from the
            interior of a container against the nominal one atmosphere pressure in the environment. This relatively
            small pressure change occurs in the laboratory as well for every process that is open to the atmosphere
            and we know that any PV product is energy, even if it is small. Thus, it has proven practical to define
            another energy quantity called the ‘‘enthalpy,’’ which is defined so that the atmospheric pressure and any
            volume change due to ambient conditions is added to the internal energy as a definition:

                                              H   U þ PV:
            Note that H is also a state variable because the PV product is energy and U is already a state
            variable. This does make some things more complicated even though the new terms may be small in
            magnitude so that we now have:
                                         dH ¼ dU þ PdV þ VdP:

            Again we appeal to practical conditions in that the external atmospheric pressure is essentially
            constant depending only on the weather variations. The atmosphere of the planet is so huge that
            opening a pressurize vessel or a vacuum chamber will not change the pressure of the atmosphere.
            Thus, we see that to a good approximation:
                                          dH ¼ dU þ PdV þ 0:
   92   93   94   95   96   97   98   99   100   101   102