Page 11 - Partition & Adsorption of Organic Contaminants in Environmental Systems
P. 11

2    IMPORTANT THERMODYNAMIC PROPERTIES

           and pressure (where there is no net exchange of mass) is governed by the
           equality or inequality of its chemical potentials with the (various) phases. The
           chemical potentials being referred to are the molar Gibbs free energies of
           the component in individual phases. There is a natural tendency of a chemi-
           cal to come to a state of equilibrium between all contacted phases, where the
           chemical potential gradient across phase boundaries is zero. The chemical
           potentials are derived from the first and second laws of thermodynamics. In
           the derivation of Gibbs free energy, the reader will also be introduced to two
           other important thermodynamic properties, enthalpy (heat) and entropy, by
           which one can distinguish a surface process from a solution process, as shown
           later. For a more detailed treatment of the thermodynamic quantities and their
           relationships, the reader is directed to a physical chemistry textbook.



           1.2 FIRST LAW OF THERMODYNAMICS

           The first law of thermodynamics is a consequence of the principle of conser-
           vation of energy: that is, that heat, kinetic energy, potential energy, and elec-
           trical energy are different forms of energy that can be interconverted but can
           be neither created nor destroyed. Consider any system enclosed in a vessel
           that can change its volume and exchange heat with its surroundings but is
           impervious to the passage of matter. We postulate a property called the inter-
           nal energy of the system, E. We will be concerned with the change in E and
           not with its absolute value. If the system absorbs an amount of heat q with no
           other changes, the conservation of energy requires that its internal energy
           increase by the amount of q; conversely, the internal energy will decrease by
           the amount of q if an amount of heat q is released to its surroundings. Simi-
           larly, if the system does work w on its surroundings with no other changes, its
           internal energy will decrease by the amount of w. If the system both exchanges
           heat and does work, the change in internal energy is then


                                               -
                                        DE =  q w                         (1.1)
           where q is here taken as positive for heat absorbed by the system and w as
           positive for work done by the system. The first law also implies that E is a state
           function: that its magnitude is solely dependent on its state variables (e.g., tem-
           perature, pressure, and volume). For any series of processes that end with a
           return to the original state variables, DE = 0.
              For a constant-pressure system involving only the work of expansion and
           contraction (i.e., no electrical work), w equals PDV, where P is the (constant)
           pressure and DV is the (finite) change in volume. In this case, the change in E
           is therefore


                                       DE =  q -  P  DV                   (1.2)
   6   7   8   9   10   11   12   13   14   15   16