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Physical Chemistry     60



                             The standard reaction free energy,   , is the change in the Gibbs free
                             energy which accompanies the conversion of reactants in their standard
                             states into products in their standard states. It may be calculated from the
                             enthalpy and entropy changes for a reaction using


                  composition. The reaction free energy varies markedly with composition through the
                  expression                ln Q where Q is the reaction quotient.
         Related   The first law (B1)             Entropy (B4)
         topics
                  Enthalpy (B2)  A more general concept, the reaction free energy, is the change in free
                                                  Entropy and change (B5)
                             energy when a reaction takes place under conditions of constant
                  Thermochemistry (B3)


                                       Free energy
        The total entropy change which accompanies a process is the sum of the entropy change
        in the system and its surroundings:
           ∆S total=∆S system+∆S surroundings
        ∆S surroundings is related to the enthalpy change in the system at constant pressure through
        the relationship:  ∆S surroundings=−∆H system/T. Substitution of this expression into the
        previous one, and subsequent multiplication by −T yields the relationship:
           −T∆S total=∆H system−T∆S system

        The  Gibbs free  energy,  G, (occasionally referred to as the  Gibbs energy or  Gibbs
        function) is defined by G=H−TS. At constant pressure and temperature, finite changes
        may be expressed as:
           ∆G−∆H system−T∆S system

        ∆G is therefore equal to −T∆S total, and the free energy may be regarded as a measure of
        the total entropy change (both in the system and the surroundings) for a process. Whilst a
        spontaneous process gives rise to a positive value of ∆S, ∆G must be negative because
        of the minus sign in ∆G=−T∆S total.
           ∆G<0 for a spontaneous process at constant pressure

        A similar function, used for work at constant volume and temperature, is termed the
        Helmholtz free energy, A (also known as the Helmholtz energy or Helmholtz function).
        As ∆S surroundings=−∆U system/T, under these conditions, the Helmholtz free energy is defined
        as A=U−TS, and ∆A is therefore equal to −T∆S total at constant volume.
           ∆A<0 for a spontaneous process at constant volume

        The Helmholtz free energy is useful in closed systems where changes occur (or may be
        approximated to occur) under constant volume conditions, such as reactions or processes
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