2. Chemical
Thermodynamics
Thermodynamics: The study of the flow of heat or any other
form of energy into or out of a system as it undergoes a
physical or chemical transformation, is called
Thermodynamics.
Most of the important laws of Physical Chemistry can be
derived from the laws of thermodynamics.
It tells whether a particular physical or chemical change can
occur under a given set of conditions of temperature, pressure
and concentration.
It also helps in predicting how far a physical or chemical
change can proceed, until the equilibrium conditions are
established.
3. Chemical
Thermodynamics
SYSTEM, BOUNDARY, SURROUNDINGS
A system is that part of the universe which is under
thermodynamic study and the rest of the universe is
surroundings.
The real or imaginary surface separating the system from
the surroundings is called the boundary.
5. Chemical
Thermodynamics
STATE OF A SYSTEM
A thermodynamic system is said to be in a certain state when
all its properties are fixed.
The fundamental properties which determine the state of
a system are pressure (P), temperature (T), volume (V), mass
and composition. Since a change in the magnitude of such
properties alters the state of the system, these are referred to
as State variables or State functions or Thermodynamic
parameters. It also stands to reason that a change of system
from the initial state to the final state (2nd state) will be
accompanied by change in the state variables.
6. Chemical
Thermodynamics
THERMODYNAMIC PROCESSES
When a thermodynamic system changes from one state
to another, the operation is called a Process.
(1) Isothermal Processes
Those processes in which the temperature remains
fixed, are termed isothermal processes. dT = 0
(2) Adiabatic Processes
Those processes in which no heat can flow into or out of
the system, are called adiabatic processes. dq = 0
(3) Isobaric Processes
Those processes which take place at constant pressure
are called isobaric processes. dp = 0
7. First Law of Thermodynamics
• The law of conservation of
energy: energy cannot be
created nor destroyed.
(James Joule in 1843 )
E = q - w
Esys + Esurr = 0
Esys = -Esurr
• Therefore, the total energy of
the universe is a constant.
Energy can, however, be converted
from one form to another or transferred
from a system to the surroundings or
vice versa.
q = the amount of heat supplied to the system
w = work done by the system
Heat adds to internal energy,
while work subtracts
8. Chemical
Thermodynamics
Some Special Forms of First Law of
Thermodynamics
ΔE = q – w
Case 1 : For a cyclic process q = w
Case 2 : For an isochoric process
w = 0. Hence
ΔE = qv
Case 3 : For an adiabatic process
q = 0
ΔE = – w
Case 4 : For an isobaric process
ΔE = q – w
or ΔE = q – PΔV
9. Chemical
Thermodynamics
ENTHALPY OF A SYSTEM
The total heat content of a system at constant pressure is
equivalent to the internal energy E plus the PV energy. This is called
the Enthalpy (Greek en = in; thalpos = heat) of the system and is
represented by the symbol H.
Change in Enthalpy
If Δ H be the difference of enthalpy of a system in the final state
(H2) and that in the initial state (H1),
ΔH = H2 – H1
ΔH = (E2 + P2V2) – (E1 + P1V1)
= (E2 – E1) + (P2V2 – P1V1)
= ΔE + ΔPV
H = E + PV
10. Second Law of
Thermodynamics
Do all processes that loose energy
occur spontaneously (by
themselves, without external
influence)??????
First Law of
Thermodynamics
Stone
E1
E2
E = E2 – E1
Spontaneity
+ Work
- (work + heat)
11. Spontaneous Processes
• can proceed without any outside intervention.
{Spontaneity}
Processes that are
spontaneous in one
direction are
nonspontaneous in
the reverse
direction.
12. Spontaneous Processes
• Processes that are spontaneous at one temperature may be
nonspontaneous at other temperatures.
• Above 0 C it is spontaneous for ice to melt.
• Below 0 C the reverse process is spontaneous.
Is the
spontaneity of
melting ice
dependent on
anything?
Spontaneous @ T > 0ºC
Spontaneous @ T < 0ºC
13. Stone
+ Work
Irreversible Processes
• Heat energy is lost to dissipation and
that energy will not be recoverable if the
process is reversed.
• Irreversible processes cannot be undone
by exactly reversing the change to the
system.
• Spontaneous processes are irreversible.
In a reversible process the system
changes in such a way that the system
and surroundings can be put back in their
original states by exactly reversing the
process.
E1
E2
- (work + heat)
Reversible Processes
14. Entropy (S)
• Entropy (S) is a term coined by Rudolph Clausius in the 1850’s.
Clausius chose "S" in honor of Sadi Carnot (who gave the first successful
theoretical account of heat engines, now known as the Carnot cycle, thereby laying the foundations of the
second law of thermodynamics).
• Clausius was convinced of the significance of the ratio of heat
delivered and the temperature at which it is delivered,
q
T
Entropy (S) =
Entropy is a measure of the energy
that becomes dissipated and unavailable
(friction, molecular motion = heat).
15. Entropy (S)
• Entropy can be thought of
as a measure of the
randomness (disorder) of
a system.
• It is related to the various
modes of motion in
molecules.
{Entropy.WaterBoiling}
• Like total energy, E, and
enthalpy, H, entropy is a
state function.
• Therefore,
S = Sfinal Sinitial
Solid
Liquid
Gas
E
N
T
R
O
P
Y
16. Second Law of
Thermodynamics
• The entropy of the universe increases for spontaneous
(irreversible) processes.
• The entropy of the universe does not
change for reversible processes.
Suniv = Ssystem + Ssurroundings > 0
Suniv = Ssystem + Ssurroundings = 0
18. Gibbs Free Energy (G)
• When Suniv is positive, G is negative.
• When G is negative, the process is spontaneous.
Gibbs Energy (-TΔS) measures the "useful" or process-initiating work
obtainable from an isothermal, isobaric thermodynamic system. Technically, the
Gibbs free energy is the maximum amount of non-expansion work which can be
extracted from a closed system or this maximum can be attained only in a
completely reversible process.
Guniv = Hsys TSsys
19. Free Energy Changes
At temperatures other than 25°C,
G° = H TS
How does G change with temperature?
• There are two parts to the free energy equation:
H— the enthalpy term
TS — the entropy term
• The temperature dependence of free energy, then comes from
the entropy term.
20. Spontaneity: Enthalpy & Entropy
G° = H TS
Spontaneous @ all T
NonSpontaneous @ all T
Spontaneous @ high T
Spontaneous @ low T