Free Energy Functions
What
are free energy functions?
Significance
of Gibbs free energy and Helmholtz free energy.
Free
Energy Functions:
In natural processes there are two factors involved when a
system approaches equilibrium. One is the tendency to minimum energy and other
is the tendency to maximum entropy. In many cases these two tendencies are in
competition. If entropy or energy changes were only involved in deciding the
direction of change, some strange phenomena would be observed.
For example, if the approach to equilibrium were governed
solely by the criterion of lowest energy, all liquids would simultaneously
freeze at any temperature, since energy is liberated on freezing. On the other
hand, criterion of approach to equilibrium as the state of maximum disorder or
entropy would result in all solids spontaneously melting or even evaporating
since both processes involve an increase in disorder.
In practice, two tendencies often reached a compromise,
which usually depends on temperature. For example solids are the stable form of
a substance below the melting point, whereas above the melting point, the
liquid is more stable. The factors which relate the energy changes, entropy
changes and temperature to the direction of spontaneous change are the free
energy functions.
These functions are the Helmholtz free energy or the work
function denoted by A (from German Arbeit which means work) and Gibbs free
energy represented by F.
These are defined as
A = E – TS
G = H – TS
Where E and H are the energies and enthalpy content of system respectively and S is the entropy.
Helmholtz
Free Energy:
A = E- TS
Since E, T and S are functions of state , A will be state
function. Hence dA is an exact differential. Moreover E and S are extensive
properties, it follows that A must also be an extensive property. State
function A is more useful when the process takes place at constant volume and constant
temperature.
Change
in Helmholtz free energy for an Isothermal process:
The change in A for an isothermal process is given by
∆A = ∆E - T∆S
Significance
of Helmholtz Free Energy:
For an isothermal infinitesimal change (T = constant)
dA
= dE – TdS
dA = dE – δQrev (TdS = δQrev
)
But δQrev
= dE + Wrev (first law of thermodynamics)
Hence dA = dE – (dE + Wrev)
dA = - Wrev
Or - dA = Wrev
We know that work done in reversible process is maximum hence
Wrev=
Wmax
And - dA = Wmax
Where - dA =
decrease in work function
Wmax includes both
mechanical and non mechanical work. In fact it is for this reason that this
thermodynamic quantity has been termed as work function.
Work Function Formula
From
the definition of thermodynamic work function,
A
= E − TS
For
a small change in the system,
dA
= dE− TdS − SdT
When
the work is mechanical,
TdS
= q (heat) = dE + PdV
∴ dA = − PdV − SdT
The
above equation is the basic thermodynamic work function equation.
Reversible Isothermal
Process
For
the reversible isothermal process,
dT = 0
Therefore, dA = − PdV (Wmax=PdV)
If the system contains ideal gas,
dA
= − nRT/V
Integrating
within the limits,
ΔA
= nRT ln(V1/V2)
Therefore,
with the increase of the volume of the system, work function decreases.
Isochoric
Process
For
the reversible isochoric system,
dV
= 0
∴ dA = −
SdT
Since
entropy is always a positive quantity. It implies that Helmholtz’s free energy
or work function A decreases with the increasing temperature of the isochoric
process.
Gibbs
Free Energy
Gibbs
Function:
F = H – TS
H, T and S are functions of state, it follows F will also be a
state function. Moreover, since H and S are extensive properties, F will also
be an extensive property. That is the value of F will be based on the mass of the
substance. This function is useful in explaining the process at constant P and
constant T.
Change
in Gibbs Free Energy for an Isothermal Process:
The change in Gibbs free energy for an isothermal process is
given by
∆G = ∆H -T∆S
Significance
of Gibbs Free Energy as useful work:
For an infinitesimal change
dG= dH – TdS
Or
dG = dE +PdV +VdP –TdS –SdT (H =
E + PV)
For a reversible process occurring at
constant temperature and pressure we have
dT = 0 and dP = 0
Hence dG = dE + PdV – TdS
Also TdS =
δQrev and δQrev =
dE + Wrev (first law of thermodynamics)
δQrev
= dE + Wmax (Wrev=
Wmax)
dG = dE + PdV – (dE + Wmax)
dG = PdV -– Wmax
-dG = Wmax
-– PdV
Wmax = maximum work obtained in a reversible process
PdV = work wasted against constant pressure
Useful work = maximum work – work wasted
Wuseful
= Wmax – PdV
Hence definition of F is as follows
“ The function of total energy which is
isothermally available for converting into useful work is called Gibbs free
energy of the system.”Or decrease in free energy is a measure of all kinds of
work except the PV work or work of expansion.
Gibbs Free Energy Equation
From
the definition of Gibbs free energy,
G
= H − TS = U + PV − TS
or, dG = dU + PdV + VdP − TdS − SdT
When
the work is mechanical work only,
TdS = q = dU + PdV
Combining
the above two equations,
dG
= dU + PdV + VdP − dU − PdV − SdT
∴ dG = VdP
− SdT
The
above equation provides another basic thermodynamic Gibbs free energy formula.
For Isothermal Process
For an isothermal process,
dT = 0
∴ dG = VdP
For n moles ideal gas,
V = nRT/P
∴ dG = nRTdP/P
Integrating the above energy equation,
G = nRTlnP + G0 (integration
constant)
When dividing by n,
μ = μ0 + RTlnP
Where μ = G/n = free energy per mole =
chemical potential
For Isobaric Process
For the reversible isobaric process,
dP = 0
∴ dG = − SdT
Since the entropy of the system is always
positive. Therefore, free energy decreases with increasing the temperature of
the system at constant pressure. The rate of decrease
of G with temperature is highest for gases and lowest for
solids.
Some
related questions:
Q: For the process H2O(l) (1 bar, 373) H2O
(g) (1 bar, 373), the correct set of thermodynamic parameters is
(a) ∆G = 0,∆S = +ve
(b) ∆G = 0,∆S = -ve
(c) ∆G = +ve,∆S = 0
(d) ∆G = -ve,∆S = 0
Ans: a
At 373 H20(l) is in equilibrium with H2O(g).
Hence ∆G =0. Since liquid molecules are converted into gaseous molecules, ∆S =
+ve.
Q: ∆H vapour is equal to 30 kJ mol-1 and , ∆S =
75 kJ mol-1. Find the temperature of vapour at 1 atmosphere
(a) 400K
(b) 350K
(c) 298K
(d) 250K
Ans: a
∆G = ∆H - T∆S; at equilibrium ∆G = 0; T = ∆H/∆S = 30 ×
103/75 = 400K
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