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Chemistry 231 Work, Heat and Internal Energy: The First Law
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Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Dec 18, 2015

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Page 1: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Chemistry 231Work, Heat and Internal

Energy: The First Law

Page 2: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

System – the specific part of the universe of interest to us

Surroundings – the part of the universe not contained in the system

Systems and Surroundings

Page 3: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

3 types of Systems• open system – exchanges mass and energy• closed system – exchanges energy but no

mass• isolated system – no exchange of either

mass or energy

State of a System (Continued)

Page 4: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Types of Systems (Continued)

Open system Closed System

corkinsulation

Isolated System

Page 5: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

State of a system• the system is in a definite state when each of its

properties has a definite value. Change in state

• initial state• final state

Path• initial and final states• intermediate states

Some Definitions

Page 6: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Process• reversible or irreversible transformation

Cyclic transformation• begins and ends at the same state variables.

Some Definitions (Continued)

Page 7: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Isothermal• dT = 0

Isochoric• dV = 0

Isobaric• dP = 0

Some Definitions (Continued)

Page 8: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Work (w)• any quantity that flows across the system’s

boundary and is completely convertible into the lifting of a mass in the surroundings.

How much work was done?

Work

Unit of work = J = 1 kg m/s2

dzFdw z

Page 9: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

0

20

40

60

80

100

120

0 10 20 30 40 50 60

Distance / m

Fo

rce

/ N

A Force Vs. Displacement Curve

Page 10: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

A single-stage expansion process

Work Done in a Closed, Fluid System

State 1 State 2

Piston(T, P1, V1)

mass (m)

Piston(T, P2, V2)

mass (m)

Dir

ecti

on

of p

isto

n

h2

h1

Page 11: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The work done in the surroundings• wsurr= Pext DV

The work done by the system• wsys = - wsurr = - Pext DV

For an infinitesimal volume change• dwsys = - Pext dV

System and Surroundings

Page 12: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

If the system is in equilibrium• Fsys = -Fext

• P = Pext

For a simple system• d wrev = - P dV

Reversible (Multistage) Expansion

Page 13: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Ideal gas as the working fluid.

Reversible Transformation in an Ideal Gaseous System

cc revrev PdVdww

VnRT

P

Page 14: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

For an isothermal process (ideal gas as working fluid)

Reversible Transformation (Continued)

1

2lnVV

nRTdwwc revrev

Page 15: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

dwirr = -Pext dV for a constant external pressure

Irreversible Transformations

12

2

1

VVP

dVPdww

ext

extc irrirr

Page 16: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Heat - the quantity that flows across the boundary of the system during a change in state• due to temperature difference between

system and surroundings• HOT to COLD (never the other way

around)!!!

Heat

Page 17: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Measured by determining the temperature change of some known object

'Amount of Heat'

C - the heat capacity of the system.

CdTdq

Page 18: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Integrate the infinitesimal heat flow

Macroscopic Heat Flows

2

1

T

Tc c

CdTCdTdqq

TCq

Page 19: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Exothermic - system to surroundings Endothermic – surroundings to system

Heat Flows

surroundingssystem

heat

Page 20: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Heat flows during phase changes - latent heats• Latent heat of vapourisation• Latent heat of fusion

Latent Heats

Page 21: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Subject our system to a cyclic transformation

The Internal Energy

CdTCdTqcycle

cycle

dwdwwcycle

cycle

Page 22: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The following would be true for an exact differential

Cyclic Integrals of Exact Differentials

exact is df if 0df

Page 23: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The infinitesimal change in the internal energy

The Internal Energy

dwdqdU

wqdwdqUc

For a general process

Page 24: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

In general, we write U as a function of T and V

The Properties of U

dVVU

dTTU

dUTV

Page 25: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Examine the first partial derivative

Isochoric Changes in U

0

dTTU

dUV

Page 26: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Define the constant volume heat capacity, CV

The Constant Volume Heat Capacity

VVV T

UdTdq

C

Page 27: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

For a system undergoing an isochoric temperature change

Heat Flows Under Constant Volume Conditions

For a macroscopic system

dTCdU V

2

1

T

TVV dTCqU

Page 28: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Examine the second partial derivative

Isothermal Changes in U

dVVU

dUT

Page 29: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Joule Experiment

AT1, Vm,1, P1

B

Stirrer

Valve

Thermal insulationFFOO

CO

CO

50

40302010 01020304050

120

100

80

0

20

20

40

60

60

40

Page 30: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The partial derivative

The Joule Coefficient

is known as the Joule coefficient, J. UV

T

Page 31: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The change in the internal energy under isothermal conditions is related to the Joule Coefficient

Internal Energy and the Joule Coefficient

VUT TU

VT

VU

JVT

CVU

Page 32: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

For an adiabatic process, q = 0!! The first law becomes

Adiabatic Processes

wU

dTCdwdU V

Page 33: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Adiabatic Processes for an Ideal Gas

For an ideal gas undergoing a reversible, adiabatic process

1

2

/

2

1,

TT

VV

mvCR

,2 2

1 1

v m

RC RP T

P T

Page 34: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Defining the enthalpy of the system Re-examine the piston with the weight

on top

State Changes Under Constant Pressure Conditions

Piston(T, P, V)

mass (m)

Page 35: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The first law

A Constant Pressure Process

Integrating

PdVdqdU P

2

1

2

1

V

VcP dVPdqdU

Page 36: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Define the enthalpy of the system, H

Enthalpy

PVUH

Page 37: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

In general, we write H as a function of T and P

The Properties of H

dPPH

dTTH

dHTP

Page 38: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Examine the first partial derivative

Isobaric Changes in H

0

dTTH

dHP

Page 39: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Define the constant pressure heat capacity, CP

The Constant Pressure Heat Capacity

PPP T

HdTdq

C

Page 40: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

For a system undergoing an isobaric temperature change

Heat Flows Under Constant Pressure Conditions

For a macroscopic system

dTCdH P

2

1

T

TPP dTCqH

Page 41: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

For an ideal gas

Relating CP and CV

nRCC VP

In general

TVP

TVCC

2

Page 42: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Examine the second partial derivative

Isothermal Changes in H

dPPH

dHT

0

Page 43: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Joule-Thomson Experiment

Porous Plug

Thermal insulation

T1, P1, Vm,1T2, P2, Vm,2

FFOO

CO

CO

50

40302010 01020304050

120

100

80

0

20

20

40

60

60

40

FFOO

CO

CO

50

40302010 01020304050

120

100

80

0

20

20

40

60

60

40

Page 44: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The partial derivative

The Joule-Thomson Coefficient

is known as the Joule-Thomson coefficient, JT.

HPT

Page 45: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The change in the enthalpy under constant pressure conditions is related to the Joule-Thomson Coefficient

Relating H to the Joule-Thompson Coefficient

PHT TH

PT

PH

JTPT

CPH

Page 46: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Enthalpy Changes for Reactions

The shorthand form for a chemical reaction

J

JJ0

J = chemical formula for substance JJ = stoichiometric coefficient for J

Page 47: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Reaction Enthalpy Changes

The enthalpy change for a chemical reaction

JHnHJ

mJr

Hm [J] = molar enthalpies of substance J

nJ = number of moles of J in the reaction

Page 48: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Enthalpy Change

Reaction beginning and ending with equilibrium or metastable states

JHn

HHH

JmJ

initialfinalr

Note – Initial and final states have the same temperature and pressure!

Page 49: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Reaction Enthalpies (cont’d)

We note that 1 mole of a reaction occurs if

JJn

JHHJ

mJr

Page 50: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

A Standard State Reaction

A reaction that begins and ends with all substances in their standard states

The degree sign, either or

• P = 1.00 bar• [aqueous species] = 1.00 mol/ kg• T = temperature of interest (in data tables -

25C or 298 K).

Page 51: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Standard Reaction Enthalpies

We note that for 1 mole of a reaction under standard conditions

JHHJ

mJr

Page 52: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Formation Reaction

A "chemical thermodynamic reference point."

For CO and CO2

C (s) + O2 (g) CO2 (g)

C (s) + ½ O2 (g) CO (g)

Page 53: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Formation Reaction

The formation reaction• 1 mole of a compound • constituent elements • stable state of aggregation at that temperature.

Formation of 1.00 mole of Na2SO3(s)

2 Na(s) + S(s) + 3/2 O2 (g) Na2SO3 (s)

‘Formation enthalpy of Na2SO3(s)’, fH°[Na2SO3 (s)]

Page 54: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Significance of the Formation Enthalpy

fH° is a measurable quantity!

Compare CO (g) with CO2 (g)

C (s) + 1/2 O2 (g) CO (g)

fH° [CO(g)] = -110.5 kJ/mole

C (s) + O2 (g) CO2 (g)

fH° [CO2(g)] = - 393.5 kJ/mole

Page 55: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Formation Enthalpies

Formation enthalpies - thermodynamic reference point! • Ho

m [J] = fH [J]

• Hm [elements] = 0 kJ / mole.

Use the tabulated values of the formation enthalpies

Page 56: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The General Equation

The enthalpy change for a given reaction is calculated from the formation enthalpies as

Notes Reverse a reaction Multiply a reaction by an integer

JHHJ

fJr

Page 57: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Calorimeter

A calorimeter - device containing water and/or another substance with a known heat capacity

Calorimeters – either truly or approximately adiabatic systems

Page 58: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Constant Volume (Bomb) Calorimeter

U = qv.

Page 59: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Constant Pressure Calorimeter

H = qp

Page 60: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Relating H and U

The enthalpy and the internal energy both represent quantities of heat.

U = qv.

H = qp.

Relate the two state functions using the following relationship

U = H - PV

Page 61: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Other Important Enthalpy Changes

Enthalpy of solution Enthalpy of dilution Enthalpy of fusion Enthalpy of vapourisation

Page 62: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Solution Enthalpy

solH - heat absorbed or released when a quantity of solute is dissolved in fixed amount of solvent

solH = Hm(sol’n) – Hm(component)• H(component) = Hm(solid) + Hm(solvent)

Two definitions• Standard• Limiting

Page 63: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Dilution Enthalpy

For the process,

HCl (aq, 6 M) HCl (aq, 1 M). The Enthalpy of dilution of the acid.

dilH = Hm(sol’n 2) – Hm(sol’n ,1)

Page 64: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Reaction Enthalpy Changes With Temperature

Differentiate the reaction enthalpy with temperature

JHHJ

mJr

JHdTd

dTHd

JmJ

r

Page 65: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

The Result

rCp

- the heat capacity change for the reaction

TCKHTH prrr 298

J

pJpr JCC

Page 66: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Internal Energy Changes in Chemical Reactions

Examine a chemical reaction.

C (s) + O2 (g) CO2 (g)

U = U[CO2 (g)] – U[C(s)] – U[O2(g)]

Note - rH = -393.5 kJ/mole

RTnUH

JUU

grr

JfJr

Page 67: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Enthalpies and Hess’s Law

Use tabulated values of formation enthalpies to obtain rH°.

May also estimate reaction enthalpies using an indirect method.

Page 68: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Hess’s Law

Hess’s Law – • the enthalpy change for a given reaction is

the same whether the reaction occurs in a single step or in many steps.

Page 69: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Bond Energies

Examine the following reactions H2 (g) ® H (g) + H (g) DU° = 433.9 kJ

Cl2 (g) ® Cl (g) + Cl (g)DU° = 239.5 kJ

Bond dissociation energies. Enthalpy changes are designated D (H-

H) and D (Cl-Cl).

Page 70: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

For Polyatomic Molecules

CO2 (g) ® C (g) + 2 O (g)DU = 740 kJ DH of this reaction D(C=O) What about dissociating methane into C

+ 4 H’s?CH4(g) ® C(g) + 4 H(g) DU° = 1640 kJ

4 C-H bonds in CH4 \ D (C-H) 410 kJ/mol

Page 71: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

Make or Break!!

Note: all chemical reactions involve the breaking and reforming of chemical bonds• Bonds break - we add energy. • Bonds form - energy is released.

rU° S D(bonds broken) - S D(bonds formed)

Page 72: Work, Heat and Internal Energy: The First Law. System – the specific part of the universe of interest to us Surroundings – the part of the universe not.

A Word of Caution

These are close but not quite exact. Why?

The bond energies we use are averaged bond energies !

This is a good approximation for reactions involving diatomic species.

Can only use the above procedure for GAS PHASE REACTIONS ONLY!!!