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(1)

Chapter 3 (1

st

law of thermodynamics)

Lecture 10

(2)

Find work done by the gas in this cycle.

P

2

P

1

V

1

V

2

Note: work is equal to

the area:

2

1



2

1

+ for clockwise d

-irectio

for anticlockwise

n

(3)

Configuration work and processes

Often, something is held constant. Examples:

dV

= 0

isochoric or isovolumic process

dQ

= 0

adiabatic process

dP

= 0

isobaric process

dT

= 0

isothermal process

(4)

Work done by a gas

f

i

V

V

W

PdV

For isochoric process

dV

= 0, so

W =

0

For isobaric process

dP

= 0, so

W = P(V

f

-V

i

)

(5)

Work done by an ideal gas

For isothermal process

dT

= 0, so

T =

constant

.

P

nRT

V

 

ln

ln

f i f i

V

V

V

V

f

i

dV

W

nRT

V

W

nRT

V

V

W

nRT

V

f i V V

PdV

W

isothermal

C

5
(6)

Free Expansion of a Gas

W=0

There is no

(7)

Example:

3 3

4000 Pa 0.3m

0.2

400

f i

W

P V

P V

V

W

m

J

  

Calculate work done by expanding gas of 1 mole if initial

pressure is 4000 Pa, initial volume is 0.2 m

3

, and initial

temperature is 96.2 K. Assume a two processes:

isobaric

expansion to 0.3 m

3

, T

f

=144.3 K

isothermal

expansion to 0.3 m

3

.

5

.

1

2

.

0

3

.

0

3

3

m

m

V

V

nR

V

P

nR

V

P

T

T

i

f

i

i

f

f

i

f

V

P

i f

V

i

V

f

P

(8)

isothermal

expansion to 0.3 m

3

.

 

ln

ln

3

8.31 96.2 ln

324

2

f i f i

V

V

V

V

f

i

dV

W

nRT

V

W

nRT

V

V

W

nRT

V

W

i

f

P

V

P

i

P

f

V

i

V

f

(9)

It depends on the path!

When heat enters a system, what happens

to the system’s

internal energy?

When work is done on a system, what

happens to the system’s

internal energy?

(10)

The first law of thermodynamics

U is a state function , so one can take the system

from an initial state to final state (state I to state F

by two methods :

a) By an adiabatic process (Q=0)

b) By non adiabatic pr0cess (Q

≠0)

)

)

ad

In a

U

W

In b

U

Q W

  

(11)
(12)

The first law of thermodynamics

Two ways to exchange energy between

a closed

system

and its surroundings (reservoir):

heat and work

Such exchanges only modify the internal energy of

the system

The first law of thermodynamics: conservation of energy

Heat

Work

reservoir

W

Q

U

Q > 0: energy enters the system

Q < 0: energy leaves the system

W > 0: work done

by

the system is positive;

energy leaves the system

W < 0: work done

by

the system is negative;

work done

on

the system

energy enters the system

• For infinitesimal processes:

pdV

dQ

dW

dQ

(13)

Adiabatic processes

W

U

Q

0

Insulating

wall

Expansion:

U

decreases

Compression:

U

increases

Isolated systems:

f

i

U

U

U

W

Q

0

0

The internal energy

of an isolated systems

remains constant

Several examples

initial state = final state

Cyclic processes

P

i, f

V

W

Q

U

0

Energy exchange between

“heat” and “work”

(14)

Idea gas-isochoric process

Isochoric process: V = constant

0

2

1

V

V

PdV

W

T

C

T

T

C

Q

V V

(

2 1

)

(C

V:

heat capacity

at constant volume)

T

C

Q

U

W

Q

U

V

P

v

T

1

T

2

Heat

reservoir

During an isochoric process, heat enters

(15)

Idea gas-isobaric process

Isobaric process: P = constant

V

P

V

V

P

PdV

W

V

V

2

(

2 1

)

1

T

C

T

T

C

Q

p p

(

2 1

)

(C

P:

heat capacity

at constant pressure)

V

P

T

C

W

Q

U

P

During an isobaric expansion process,

heat enters the system. Part of the heat is

used by the system to do work on the

environment; the rest of the heat is used

to increase the internal energy.

Heat

Work

reservoir

P

v

T

1

T

2

v

1

v

2

(16)

Idea gas-isothermal process

Isothermal process: T = constant

PV

nRT

2 2 1 1 2 1 2 1

ln

V V V V V V

nRT

W

PdV

dV

V

dV

nRT

V

V

nRT

V

0

2

f

U

nRT

  

U

2

ln

V

Q

W

nRT

 

During an isothermal expansion process,

heat enters the system and all of the heat

is used by the system to do work on the

environment.

During an isothermal compression process,

energy enters the system by the work done

on the system, but all of the energy leaves

the system at the same time as the heat

P

v

T

(17)

dU

dQ

dW

(18)

Ideal gas-adiabatic process

Adiabatic process:

Q

= 0

2

2

2

2

f

f

U

nRT

dU

nRdT

dU

dQ dW

PdV

f

PdV

nRdT

nRdT

PdV

f

 

 

(

)

(

)

nRT

PV

d nRT

d PV

nRdT

PdV

V dP

2

PdV

VdP

 

PdV

P

v

T

i

T

f

(19)

( , )

P

P V T

0

)

2

1

(

2

PdV

f

VdP

PdV

f

VdP

PdV

1 1

1

1

0

ln

ln

0

P

V

P

V

dP

dV

P

V

P

V

 

P

V

Idea gas adiabatic process

P

v

T

1

T

v

1

v

2

1

dP

dV

0

Let

f

P

V

 

1 1

1 1

constant

ln

PV

0

V

PV

PV

P

 

(20)

2

2

1

1

V

P

V

P

1

2

2

1

V

V

P

P

2 1 1 1 1 2

T

T

V

V

Idea gas-adiabatic process

1

1

1

1

2

2

T V

T

V

constant

PV

P

v

T

1

T

2

v

1

v

2

1

1

1

2

2

2

P V

T

P V

T

(21)

2 1 2 1

1

1

V

V

V

V

V

dV

V

P

PdV

W

1

1

1 1

2

1

1

(1

)

W

PV

V

V

Work done by an idea gas in an adiabatic process

1 1

constant

PV

PV

constant

PV

P

v

T

1

T

2

v

1

v

2

2

1

(1

)

nR

W

T

T

2

2

1 1

1

(1

)

W

PV

PV

(22)

Idea gas adiabatic process

During an adiabatic

compression

process, the

environment does work on the system and increases the

internal energy.

P

v

T

1

T

2

v

1

v

2

During an adiabatic

expansion

(23)

Summary

Internal energy, heat, and work:

internal energy is the energy of the system.It is a state function.

heat and work are two ways to exchange energy between the system and the environment.

They are not state functions and depend on the path.

The first law of thermodynamics connects the internal energy with heat and

work:

  

U

Q W

Quasi-static

process

Character

U

Q

W

adiabatic

Q

0

U

W

isothermal

T = constant

 

U

0

isovolumetric

isobaric

V = constant

P = constant

U

Q

 

Q

C

V

T

W

0

V

P

W

W

Q

U

Q

C

P

T

2 1

ln

V

W

nRT

V

Q

W

0

Q

2 1

(1

)

nR

W

T

T

23

(24)

Latent Heat (enthalpy)

12

2

1

2

1

During Phase change, lets say from solid to liquid phase

at constant T and P, l

    

q

u w

u

 

u

P v

(

v

)

12

2

2

1

1

12

2

1

(

) (

)

Where h ca

l

u

pv

u

pv

l

h

h

lled the enthalp

y

23

3

2

From liquid to gas

l

h

h

13

3

1

From solid to gas

l

h

h

(25)

Enthalpy (history of the name)

Over the

history of thermodynamics

, several terms have been used to denote

what is now known as the

enthalpy

of a system.

Originally, it was thought that the word "enthalpy" was created by

Benoit

Paul Émile Clapeyron

and

Rudolf Clausius

through the publishing of the

Clausius-Clapeyron relation

in

The Mollier Steam Tables and Diagrams

in 1827.

Gibbs

introduced a "heat function for constant pressure" in 1875, although

the word

enthalpy

does not appear in any of Gibbs' work.

In 1909,

Keith Landler

discussed Gibbs's work on this "heat function" and

noted that

Heike Kamerlingh Onnes

had coined the modern name from the

Greek

word "enthalpos" (

ενθαλ

π

ος

) meaning "to put heat into.

H

 

U

PV

(26)

Difference between

H

and

U

: the additional term

pV

If

pV

is an additional

energy

associated with the system (say, a gas), and is not in

the

internal energy

U

, then where is it?

The energy

pV

is in the surroundings (typically, the atmosphere). When a

system (e.g.,

n

moles

of a gas of

volume

V

at

pressure

P

and

temperature

T

) is

created

(brought to its present state from

absolute zero

), energy must be

supplied equal to its internal energy

U plus pV

, where

pV

is the

work

done in

pushing against the (atmospheric) pressure.

This additional energy is therefore stored in the surroundings (atmosphere)

(27)

In

thermodynamics

and

molecular chemistry

,

enthalpy

(denoted as

H

, or specific enthalpy denoted as

h

) is a

thermodynamic property

of a

thermodynamic system

.

It can be used to calculate the heat transfer

during a

quasistatic process

taking place in a closed

thermodynamic system

under constant pressure

.

Change in enthalpy Δ

H

is frequently a more useful

value than

H

itself.

For quasistatic processes under constant pressure,

Δ

H

is equal to the change in the internal energy of the

system, plus the work that the system has done on its

surroundings.

Enthalpy

H

U W

   

(28)

Enthalpy Change

The heat content of a chemical system is called the

enthalpy

(symbol: H) .

The enthalpy change ( H) is the amount of heat released or

absorbed when a chemical reaction occurs at constant

pressure. H is total enthalpy, h is enthalpy per mole

h is specified per mole of substance as in the balanced

chemical equation for the reaction.

The units are usually given as kJ mol

-1

(kJ/mol) or sometimes

as kcal mol

-1

(kcal/mol).

2

1

product

reactant

phase

phase

H

H

H

for chemical reaction

H

H

H

for phase change

 

(29)

Latent Heat (enthalpy)

Latent Heat (enthalpy) is the "hidden" heat when a

substance absorbs or releases heat without producing a

change in the temperature of the substance, eg, during a

change of state.

Latent Heat (enthalpy) of Fusion is the heat absorbed

per mole when a substance changes state from solid to

liquid at constant temperature (melting point).

l

12

Latent Heat (enthalpy) of Vaporization is the heat

absorbed per mole when a substance changes state from

liquid to gas at constant temperature (boiling point).

l

23

Latent Heat (enthalpy) of Sublimation is the heat

absorbed per mole when a substance changes state from

solid to gas, without going through the liquid phase, at

constant temperature.

l

13

13

12

23

l

l

l

(30)

Latent Heat (enthalpy)

12

2

1

2

1

During Phase change, lets say from solid to liquid phase

at constant T and P, l

    

q

u w

u

 

u

P v

(

v

)

12

2

2

1

1

12

2

1

(

) (

)

Where h ca

l

u

pv

u

pv

l

h

h

lled the enthalp

y

23

3

2

From liquid to gas

l

h

h

13

3

1

From solid to gas

l

h

h

the history of thermodynamics Benoit Paul Émile Clapeyron Rudolf Clausius Clausius-Clapeyron relation Gibbs Keith Landler t Heike Kamerlingh Onnes Greek l energy internal energy moles of volume t pressure temperature absolute zero work thermodynamics molecular chemistry, thermodynamic property a thermodynamic system the heat transfer quasistatic process a closed

References

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