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Auxiliary Functions

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Auxiliary Functions
Introduction
• The study of thermodynamics provides the criteria for equilibrium in
systems and the determination of the effect, on an equilibrium state, of
changes in the external influences acting on the system.
• This provision is determined by the practicality of the equations of state
for the system.
• To achieve this, it is desirable to develop simple expressions which contain
convenient choice of independent variables which can be easily controlled
and measured.
• It’s is often found that some required thermodynamic expressions which
are not easily amenable to experimental measurement are related in a
simpler manner to some measurable quantities.
• New thermodynamic functions are introduced and their properties and
interrelationships are examined:
Helmholtz and Gibbs Free Energies
• The Helmholtz free energy, A, is defined as
𝐴 = π‘ˆ + 𝑇𝑆
(5.1)
• The Gibbs free energy, G, is defined as
𝐺 = π‘ˆ + 𝑃𝑉 − 𝑇𝑆
= 𝐻 − 𝑇𝑆
(5.2)
• For a system undergoing a change of state from 1 to 2,
𝐺2 − 𝐺1 = 𝐻2 − 𝐻1 − 𝑇2𝑆2 − 𝑇1𝑆1
= π‘ˆ2 − π‘ˆ1 + 𝑃2𝑉2 − 𝑃1𝑉1 − (𝑇2𝑆2 − 𝑇1𝑆1)
• For a closed system, the first law gives,
π‘ˆ2 − π‘ˆ1 = π‘ž − 𝑀
and thus
𝐺2 − 𝐺1 = π‘ž − 𝑀 + 𝑃2𝑉2 − 𝑃1𝑉1 − (𝑇2𝑆2 − 𝑇1𝑆1)
(5.6)
• If the processes is carried out such that 𝑇1 = 𝑇2 = 𝑇, the constant
temperature of the heat reservoir which supplies or withdraws heat from
the system, and also if 𝑃1 = 𝑃2 = 𝑃, the constant pressure at which the
system undergoes a change in volume , then
(𝐺2 − 𝐺1) = π‘ž − 𝑀 + 𝑃 𝑉2 − 𝑉1 − 𝑇(𝑆2 − 𝑆1)
• If the system preforms chemical or electrical work in addition to 𝑃 − 𝑉
work, the work terms are included in 𝑀, i.e.
𝑀 = 𝑀′ + 𝑃 𝑉2 − 𝑉1
in which 𝑀′ is the sum of all non 𝑃 − 𝑉 forms of work done. Substituting into
the above eqn. gives,
𝐺2 − 𝐺1 = π‘ž − 𝑀′ − 𝑇 𝑆2 − 𝑆1
and from the second law as,
π‘ž ≤ 𝑇(𝑆2 − 𝑆1)
then,
𝑀′ ≤ −(𝐺2 − 𝐺1)
(5.7)
The equality can be written as,
−𝑀 ′ = 𝐺2 − 𝐺1 + π‘‡βˆ†π‘†π‘–π‘Ÿπ‘Ÿ
• Thus, for an isothermal, isobaric process, during which no form of work
other than P-V work is performed i.e. 𝑀′ = 0,
𝐺2 − 𝐺1 + π‘‡βˆ†π‘†π‘–π‘Ÿπ‘Ÿ = 0
(5.8)
Such a process can only occur spontaneously (with an increase in entropy) if
the Gibbs free energy decreases. As π‘‘π‘†π‘–π‘Ÿπ‘Ÿ = 0 is a criterion for a reversible
process, thermodynamic equilibrium requires that,
𝑑𝐺 = 0
(5.9)
• Thus for a system undergoing a process at constant 𝑇 and constant 𝑃, the
Gibbs free energy can only decrease or remain constant, and the
attainment of equilibrium in the system coincides with the system having
the minimum value of 𝐺 consistent with the values of 𝑃 and 𝑇.
• Since
π‘‘π‘ˆ = 𝑇𝑑𝑆 − 𝑃𝑑𝑉
and
𝐻 = π‘ˆ + 𝑃𝑉
and thus
𝑑𝐻 = 𝑇𝑑𝑆 + 𝑉𝑑𝑃
(5.10)
𝐴 = π‘ˆ − 𝑇𝑆
and thus
𝑑𝐴 = −𝑆𝑑𝑇 − 𝑃𝑑𝑉
(5.11)
𝐺 = 𝐻 − 𝑇𝑆
and thus
𝑑𝐺 = −𝑆𝑑𝑇 + 𝑉𝑑𝑃
(5.12)
Variation of Composition and Size of System
• If the size and composition of a system can vary during a process, the
specification of only two variables will be no longer sufficient to fix the
state of the system.
• It is therefore necessary to specify the number of moles within the
system.
• Gibbs free energy is thus a function of 𝑇, 𝑃 and the numbers of moles of
all the species present in the system:
𝐺 = 𝐺(𝑇, 𝑃, 𝑛𝑖 , 𝑛𝑗, π‘›π‘˜, … )
(5.13)
Where 𝑛𝑖, 𝑛𝑗, π‘›π‘˜, … . are the number of moles of the species 𝑖, 𝑗, π‘˜, … present
in the system and the state of the system is only fixed when all the
independent variables are fixed. Differentiation of (5.13) gives:
πœ•πΊ
πœ•πΊ
πœ•πΊ
𝑑𝐺 =
𝑑𝑇 +
𝑑𝑃 +
𝑑𝑛𝑖 +
πœ•π‘‡ 𝑃, 𝑛𝑖, 𝑛𝑗 …
πœ•π‘ƒ 𝑇, 𝑛𝑖, 𝑛𝑗, …
πœ•π‘›π‘– 𝑇, 𝑃, 𝑛𝑗, π‘›π‘˜, …
πœ•πΊ
𝑑𝑛𝑗
πœ•π‘›π‘— 𝑇, 𝑃 , 𝑛𝑖, π‘›π‘˜, …
+β‹―
(5.14)
• If the numbers of moles of all of the individual species remain constant
during the process the above eqn. simplifies to eqn. (5.12) i.e.
𝑑𝐺 = −𝑆𝑑𝑇 + 𝑉𝑑𝑃
from which it is seen that
πœ•πΊ
πœ•π‘‡
𝑃 , 𝑛𝑖, 𝑛𝑗, …
= −𝑆
and
πœ•πΊ
πœ•π‘ƒ
Substituting into eqn. (5.14) gives
𝑇, 𝑛𝑖, 𝑛𝑗, …
𝑖=π‘˜
𝑑𝐺 = −𝑆𝑑𝑇 + 𝑉𝑑𝑃 +
𝑖=1
=𝑉
πœ•πΊ
πœ•π‘›π‘–
𝑇, 𝑃, 𝑛𝑗, …
𝑑𝑛𝑖
(5.15)
where
𝑖=π‘˜
𝑖=1
πœ•πΊ
πœ•π‘›π‘–
𝑇, 𝑃, 𝑛𝑗, …
𝑑𝑛𝑖
is the sum of π‘˜ terms, one for each species of the π‘˜ species, each of which is
determined by partial differentiation of 𝐺 w.r.t the number of moles of the 𝑖th
species at constant 𝑇, 𝑃, and 𝑛𝑗, where 𝑛𝑗 represents the number of moles of
every species other than the 𝑖th species.
Chemical Potential
• The term πœ•πΊ πœ•π‘›π‘– 𝑇, 𝑃, 𝑛𝑗… is called the chemical potential of the species 𝑖,
designated 𝑖 , i.e.
πœ•πΊ
πœ•π‘›π‘– 𝑇, 𝑃, 𝑛𝑗, …
= 𝑖
(5.16)
• The chemical potential of 𝑖 in a homogeneous phase is the rate of increase
of 𝐺 with 𝑛𝑖 when the species 𝑖 is added to the system at constant
𝑇, 𝑃 and number of moles of all the other species.
• If the system is large enough that the addition of 1 mole of 𝑖, at constant 𝑇
and 𝑃, does not measurably change the composition of the system, then
𝑖 is the increase in 𝐺 of the system caused by the addition.
• Eqn (5.15) can thus be written as
𝑑𝐺 = −𝑆𝑑𝑇 + 𝑉𝑑𝑃 + π‘˜1 πœ‡π‘–π‘‘π‘›π‘–
(5.17)
•
•
Eqn (5.17) can be applied to open systems which exchange matter and heat
with their surroundings, and to closed systems which undergo changes in
composition caused by chemical reactions.
Equations (3.12), π‘‘π‘ˆ = 𝑇𝑑𝑆 − 𝑃𝑑𝑉, (5.10), 𝑑𝐻 = 𝑇𝑑𝑆 + 𝑉𝑑𝑃, and (5.11),
𝑑𝐴 = −𝑆𝑑𝑇 − 𝑃𝑑𝑉, can be made applicable to open systems by including the
terms describing the dependences on composition of, respectively, π‘ˆ, 𝐻 and
𝐴:
π‘˜
π‘‘π‘ˆ = 𝑇𝑑𝑆 − 𝑃𝑑𝑉 +
1
πœ•π‘ˆ
πœ•π‘›π‘–
𝑆 , 𝑉 , 𝑛𝑗, …
𝑑𝑛𝑖
(5.18)
π‘˜
𝑑𝐻 = 𝑇𝑑𝑆 − 𝑉𝑑𝑃 +
1
πœ•π»
πœ•π‘›π‘–
𝑆 , 𝑃 , 𝑛𝑗, …
𝑑𝑛𝑖
(5.19)
π‘˜
𝑑𝐴 = −𝑆𝑑𝑇 + 𝑃𝑑𝑉 +
1
πœ•π΄
πœ•π‘›π‘–
𝑇, 𝑉 , 𝑛𝑗, …
𝑑𝑛𝑖
(5.20)
• Inspection of Eqns. (5.16), (5.18), (5.19) and (5.20) shows that:
πœ•πΊ
πœ•π‘ˆ
πœ•π»
πœ•π΄
= πœ‡π‘– =
=
=
πœ•π‘›π‘– 𝑇, 𝑃, 𝑛𝑗
πœ•π‘›π‘– 𝑆, 𝑉 , 𝑛𝑗
πœ•π‘›π‘– 𝑆, 𝑃, 𝑛𝑗
πœ•π‘›π‘– 𝑇, 𝑉 , 𝑛𝑗
(5.21)
and hence the complete set of equations is:
π‘‘π‘ˆ = 𝑇𝑑𝑆 − 𝑃𝑑𝑉 +
πœ‡π‘–π‘‘π‘›π‘–
(5.22)
𝑑𝐻 = 𝑇𝑑𝑆 + 𝑉𝑑𝑃 +
πœ‡π‘–π‘‘π‘›π‘–
(5.23)
𝑑𝐴 = −𝑆𝑑𝑇 − 𝑃𝑑𝑉 +
πœ‡π‘–π‘‘π‘›π‘–
(5.24)
𝑑𝐺 = −𝑆𝑑𝑇 + 𝑉𝑑𝑃 +
πœ‡π‘–π‘‘π‘›π‘–
(5.25)
• The first law gives
π‘‘π‘ˆ = π›Ώπ‘ž − 𝛿𝑀
which on comparison with equation (5.22), π‘‘π‘ˆ = 𝑇𝑑𝑆 − 𝑃𝑑𝑉 + πœ‡π‘–π‘‘π‘›π‘– ,
indicates that, for a closed system undergoing a process involving a reversible
change in composition (e.g. a reversible chemical reaction),
π›Ώπ‘ž = 𝑇𝑑𝑆
and
𝛿𝑀 = 𝑃𝑑𝑉 +
𝑒𝑖𝑑𝑛𝑖
The term 𝑒𝑖𝑑𝑛𝑖 is thus the chemical work done by the system which was
denoted as 𝑀′ in Eq. (5.7), 𝑀′ ≤ −(𝐺2 − 𝐺1) .
Thermodynamic Relations
The following relations are obtained from Eqns. (5.22)-(5.25):
𝑇=
πœ•π‘ˆ
πœ•π‘†
𝑉 , π‘π‘œπ‘šπ‘
=
πœ•π»
πœ•π‘†
𝑃 , π‘π‘œπ‘šπ‘
(5.26)
πœ•π‘ˆ
𝑃=−
πœ•π‘‰
πœ•π΄
=−
πœ•π‘‰
𝑆, π‘π‘œπ‘šπ‘
𝑇, π‘π‘œπ‘šπ‘
(5.27)
πœ•π»
𝑉=
πœ•π‘ƒ
πœ•πΊ
=
πœ•π‘ƒ
𝑆, π‘π‘œπ‘šπ‘
𝑇, π‘π‘œπ‘šπ‘
(5.28)
𝑆=−
πœ•π΄
πœ•π‘‡
𝑉 , π‘π‘œπ‘šπ‘
=−
πœ•πΊ
πœ•π‘‡
𝑃 , π‘π‘œπ‘šπ‘
(5.29)
Maxwell’s Equations
• If 𝑍 is a state function and π‘₯ and 𝑦 are chosen as the independent
variables in a closed system of fixed composition then,
𝑍 = 𝑍(π‘₯, 𝑦)
and by differentiation,
πœ•π‘
πœ•π‘
𝑑𝑍 =
𝑑π‘₯ +
𝑑𝑦
πœ•π‘₯ 𝑦
πœ•π‘¦ π‘₯
• If the partial derivative πœ•π‘ πœ•π‘₯ 𝑦 is itself a function of π‘₯ and 𝑦, being given
by πœ•π‘ πœ•π‘₯ 𝑦 = 𝐿(π‘₯, 𝑦), and similarly πœ•π‘ πœ•π‘¦ π‘₯ = 𝑀 π‘₯, 𝑦 then
𝑑𝑍 = 𝐿𝑑π‘₯ + 𝑀𝑑𝑦
Thus
πœ• πœ•π‘
πœ•π‘¦ πœ•π‘₯
and
𝑦 π‘₯
πœ•πΏ
=
πœ•π‘¦
π‘₯
πœ• πœ•π‘
πœ•π‘€
=
πœ•π‘₯ πœ•π‘¦ π‘₯ 𝑦
πœ•π‘₯ 𝑦
But, as 𝑍 is a state function, the change in 𝑍 is independent of the order of
differentiation, and thus,
πœ• πœ•π‘
πœ• πœ•π‘
πœ•2𝑍
=
=
πœ•π‘¦ πœ•π‘₯ 𝑦 π‘₯
πœ•π‘₯ πœ•π‘¦ π‘₯ 𝑦 πœ•π‘₯πœ•π‘¦
and hence
πœ•πΏ
πœ•π‘€
=
πœ•π‘¦ π‘₯
πœ•π‘₯ 𝑦
(5.30)
• Application of equation (5.30) to Eqns. (3.12) and (5.10)-(5.12) gives a set
of relations which are referred to as the Maxwell’s Equations:
πœ•π‘‡
πœ•π‘‰
πœ•π‘ƒ
=−
πœ•π‘†
𝑆
𝑉
(5.31)
πœ•π‘‡
πœ•π‘ƒ
πœ•π‘‰
=
πœ•π‘†
𝑆
𝑃
(5.32)
πœ•π‘†
πœ•π‘‰
πœ•π‘ƒ
=
πœ•π‘‡
𝑇
𝑉
(5.33)
πœ•π‘†
πœ•π‘ƒ
πœ•π‘‰
=−
πœ•π‘‡
𝑇
𝑃
(5.34)
• Consider the dependence of entropy of an ideal gas on 𝑇 and 𝑉:
𝑆 = 𝑆 𝑇, 𝑉
and by differentiation
𝑑𝑆 =
πœ•π‘†
πœ•π‘‡
𝑑𝑇 +
𝑉
πœ•π‘†
πœ•π‘‰
𝑑𝑉
𝑇
(𝑖)
Combination of the definition of the constant volume heat capacity (Eqn.
π›Ώπ‘ž
(2.6), π‘‘π‘ˆ = 𝐢𝑣 𝑑𝑇 and Eqn. (3.8), 𝑑𝑆 = π‘Ÿπ‘’π‘£ applied to a reversible constant
𝑇
volume process gives,
𝑇𝑑𝑆 = π›Ώπ‘žπ‘£ = π‘‘π‘ˆ = 𝑛𝑐𝑣 𝑑𝑇
the first P.D on the right-hand side of eqn. (i) is obtained as
πœ•π‘†
𝑛𝑐𝑣
=
πœ•π‘‡ 𝑉
𝑇
and the second P.D in eqn. (i) is obtained from Maxwell’s equation (5.33).
• Thus eqn. (i) can be written as,
𝑛𝑐𝑣
πœ•π‘ƒ
𝑑𝑆 =
𝑑𝑇 +
𝑇
πœ•π‘‡
𝑑𝑉
𝑉
(ii)
From the ideal gas law
πœ•π‘ƒ
πœ•π‘‡
𝑉
𝑛𝑅
=
𝑉
(iii)
and thus eqn. (ii) can be written as
𝑛𝑐𝑣
𝑛𝑅
𝑑𝑆 =
𝑑𝑇 +
𝑑𝑉
𝑇
𝑉
(iv)
integration of which between two states gives
𝑇2
𝑉2
𝑆2 − 𝑆1 = 𝑛𝑐𝑣 𝐼𝑛
+ 𝑛𝑅𝐼𝑛
𝑇1
𝑉1
•
Considering a closed system of fixed composition Eqn. (3.12) gives,
π‘‘π‘ˆ = 𝑇𝑑𝑆 − 𝑃𝑑𝑉
and thus
πœ•π‘ˆ
πœ•π‘†
=𝑇
−𝑃
πœ•π‘‰ 𝑇
πœ•π‘‰ 𝑇
Using Maxwell’s eqn. (5.33) allows this to be written as
πœ•π‘ˆ
πœ•π‘ƒ
=𝑇
−𝑃
πœ•π‘‰ 𝑇
πœ•π‘‡ 𝑉
(v)
which is an equation of state relating the internal energy of a closed system of
fixed composition to measurable quantities 𝑇, 𝑉 and 𝑃.
If the system is 1 mole of an ideal gas, substitution of eqn. (iii) into eqn. (v) gives
πœ•π‘ˆ
=0
πœ•π‘‰ 𝑇
Therefore the internal energy of an ideal gas is independent of the volume of the
gas.
• Similarly for a closed system of fixed composition, eqn. (5.10) gives,
𝑑𝐻 = 𝑇𝑑𝑆 + 𝑉𝑑𝑃
in which case
πœ•π»
πœ•π‘ƒ
πœ•π‘†
=𝑇
πœ•π‘ƒ
𝑇
𝑇
+𝑉
Substituting Maxwell’s eqn. (5.34) gives
πœ•π»
πœ•π‘‰
= −𝑇
+𝑉
πœ•π‘ƒ 𝑇
πœ•π‘‡ 𝑃
which is an equation of state which gives the dependence of enthalpy on
𝑇, 𝑃 and 𝑉. If the system is an ideal gas, this equation of state shows that the
enthalpy of an ideal gas is independent of its pressure.
The Gibbs-Helmholtz
Eqn.(5.2) gives
𝐺 = 𝐻 − 𝑇𝑆
Eqn. (5.12) gives
𝑑𝐺 = −𝑆𝑑𝑇 + 𝑉𝑑𝑃
and therefore,
πœ•πΊ
= −𝑆
πœ•π‘‡ 𝑃
Thus at constant pressure and composition,
𝑑𝐺
𝐺 =𝐻+𝑇
𝑑𝑇
or
𝐺𝑑𝑇 = 𝐻𝑑𝑇 + 𝑇𝑑𝐺
Dividing throughout by 𝑇2 and rearranging gives,
𝑇𝑑𝐺 − 𝐺𝑑𝑇
𝐻𝑑𝑇
=− 2
𝑇2
𝑇
which on comparison with the identity
π‘₯
𝑦𝑑π‘₯ − π‘₯𝑑𝑦
𝑑
=
𝑦
𝑦2
shows that
𝑑 𝐺 𝑇
𝐻
=− 2
𝑑𝑇
𝑇
(5.36)
The above equation is known as the Gibbs-Helmholtz equation and is
applicable to a closed system of fixed composition undergoing processes at
constant composition.
• For an isobaric change of state of a closed system of fixed composition,
eqn. (5.36) gives the relation of the change in 𝐺 to the change in 𝐻 as
𝑑(βˆ†πΊ 𝑇)
βˆ†π»
=− 2
𝑑𝑇
𝑇
(5.36a)
• This equation is used in experimental thermodynamics since it allows βˆ†π»,
the heat of reaction, to be obtained from a measurement of βˆ†πΊ, the free
energy change for the reaction, with temperature, or, conversely βˆ†πΊ to be
obtained from a measurement of βˆ†π».
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