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                  The lowest temperature reached in bulk matter by using adiabatic demagnetization is      Further Reading
                  1.2   10  5  K [K. Gloos et al., J. Low. Temp. Phys., 73, 101 (1988); Discover, June
                  1989, p. 16]. Using a combination of laser light, an applied inhomogeneous magnetic
                  field, and applied radiofrequency radiation, physicists cooled a sample of 2000 low-
                          87
                  pressure  Rb gas-phase atoms to 2   10  8  K [M. H. Anderson et al., Science, 269,
                  198 (1995); jilawww.colorado.edu/bec/). Silver nuclei have been cooled to a nuclear-
                  spin temperature of 2    10  9  K by adiabatic demagnetization (O. V. Lounasmaa,
                  Physics Today, October 1989, p. 26).


                    5.12         SUMMARY
                  The standard state (symbolized by the ° superscript) of a pure liquid or solid at tem-
                  perature T is defined as the state with P   1 bar; for a pure gas, the standard state has
                  P   1 bar and the gas behaving ideally.
                      The standard changes in enthalpy, entropy, and Gibbs energy for the chemical re-
                  action 0 →   n A are defined as  H°     n H° m,T,i ,  S°     n S°  , and  G°
                                                                   T
                                                                                       T
                                                                          i m,T,i
                                                                        i
                                                          i
                                i
                                  i
                              i
                                                        i
                                                   T
                    n G° m,T,i  and are related by  G°   H°   T  S°.  H° and  G° of a reaction can
                      i
                    i
                                                      T
                                                              T
                                               T
                  be calculated from tabulated   H° and   G°values of the species involved by using
                                             f
                                                     f
                   H°     n   H° and  G°    n   G° , where the standard enthalpy and Gibbs
                           i
                                               i
                                                    f
                                                 i
                                 T,i
                                          T
                             i
                               f
                                                      T,i
                      T
                  energy of formation   H°and   G°correspond to formation of one mole of substance
                                                i
                                             f
                                     f
                                       i
                  i from its elements in their reference forms.
                      The convention that S°   0 for all elements and the third law of thermodynamics
                                         0
                  ( S   0 for changes involving only substances in internal equilibrium) lead to a con-
                      0
                  ventional S° value of zero for every substance. The conventional S° m,T  value of a sub-
                            0
                  stance can then be found by integration of C° /T from absolute zero with inclusion of
                                                        P,m
                   S of any phase transitions.
                      Using  H° (or  S°) at one temperature and C° data, one can calculate  H° (or
                                                              P
                   S°) at another temperature.
                      To avoid confusion, it is essential to pay close attention to thermodynamic sym-
                  bols, including the subscripts and superscripts. The quantities H,  H,  H°, and   H°
                                                                                       f
                  generally have different meanings.
                      Important kinds of calculations discussed in this chapter include:
                  •   Determination of  H° of a reaction by combining  H°values of other reactions
                      (Hess’s law).
                  •   Calculation of   U from adiabatic bomb calorimetry data.
                                    r
                  •   Calculation of  H° from  U°, and vice versa.
                  •   Calculation of  S° of a pure substance from  C° P,m  data, enthalpies of phase
                                     m
                                            3
                      changes, and the Debye T law.
                  •   Calculation of  H°,  S°, and  G° of chemical reactions from tabulated   H°, S° ,
                                                                                    f
                                                                                         m
                      and   G° data.
                           f
                  •   Determination of  H° (or  S°) at one temperature from  H° (or  S°) at another
                      temperature and C° (T ) data.
                                      P,m
                  •   Estimation of  H° using bond energies.
                  •   Use of a spreadsheet to fit equations to data.
                  FURTHER READING
                  Heats of reaction and calorimetry: McGlashan, pp. 17–25, 48–71; Rossiter, Hamilton,
                  and Baetzold, vol. VI, chap. 7; S. Sunner and M. Mansson (eds.),  Combustion
                  Calorimetry, Pergamon, 1979. The third law:  Eyring, Henderson, and Jost, vol. I,
                  pp. 86–96, 436–486.
                      For data sources, see Sec. 5.9.
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