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Lecture 2: Heat Capacities/State functions • Reading: Zumdahl 9.3 • Outline Definition of Heat Capacity (C v and C p ) Calculating E and H using C v and C p – Example of Thermodynamic Pathways – State Functions

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Page 1: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Lecture 2: Heat Capacities/State functions

• Reading: Zumdahl 9.3

• Outline– Definition of Heat Capacity (Cv and Cp)

– Calculating E and H using Cv and Cp

– Example of Thermodynamic Pathways – State Functions

Page 2: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Heat Capacity at Constant V• Recall from Chapter 5 (section 5.6):

(KE)ave = 3/2RT (ideal monatomic gas)

• Temperature is a measure of molecular speed

• In thermodynamic terms, an increase in system temperature corresponds to an increase in system kinetic energy ( i.e., q is proportional to <KE>)

Page 3: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Heat Capacity at Constant V• (KE)ave = 3/2RT (ideal monatomic gas)

• How much energy in the form of heat is required to change the gas temperature by an amount T?

Heat required = 3/2R T = 3/2R (for T = 1K)

• Therefore, Cv = 3/2 R is the heat required to raise one mole of an ideal gas by 1K. Cv is called constant volume molar heat capacity.

Page 4: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Heat Capacity at Constant P

• What about at constant pressure? In this case, PV type work can also occur:

PV = nRT = RT (for 1 mole)

= R (for T = 1 K)

• Cp = “heat into translation” + “work to expand the gas” = Cv + R = 5/2R (for ideal monatomic gas)

Page 5: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Cv for Monatomic Gases

• What are the energetic degrees of freedom for a monatomic gas?

• Just translations, which contribute 3/2R to Cv.

z

x

y

1/2 mv2 = 3/2 RT

Page 6: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Cv for Polyatomics

• What are the energetic degrees of freedom for a polyatomic gas?

Translations, rotations, and vibrations. All of which may contribute to Cv (depends on T).

IzIy

IzIy

Ix

N2 Cv = 5/2 R (approx.)

NO2 Cv = 7/2 R (approx.)

Page 7: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Cv for Polyatomics

• When heat is provided , molecules absorb energy and the translational kinetic energy increases

• In polyatomic gases, rotational and vibrational kinetic energies increase as well (depending on T).

IzIy

IzIy

Ix

N2 Cv = 5/2 R (approx.)

NO2 Cv = 7/2 R (approx.)

Page 8: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Cv for Polyatomics

• T measures the average translational kinetic energy

• Increases in rotational and vibrational kinetic energies do not increase T directly

• It takes more heat to increase T by the same amount (Cv/Cp larger)

IzIy

IzIy

Ix

N2 Cv = 5/2 R (approx.)

NO2 Cv = 7/2 R (approx.)

Page 9: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Variation in Cp and Cv

• Monatomics: – Cv = 3/2 R

– Cp = 5/2 R

• Polyatomics: – Cv > 3/2 R

– Cp > 5/2 R

– But….Cp = Cv + R

H2

Ar, He, Ne

Cv Cp

CO2

12.47 20.8

20.54 28.86

28.95 37.27

Units: J/mol.K

Page 10: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Energy and Cv

• Recall from Chapter 5:

Eave = 3/2 nRT (average translational energy)

E = 3/2 nR T

E = n Cv T (since 3/2 R = Cv)

• Why is Cv=E/T

When heating our system at constant volume, all heat goes towards increasing E (no work).

Page 11: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Enthalpy and Cp

• What if we heated our gas at constant pressure? Then, we have a volume change such that work occurs:

q p = n Cp T

= n (Cv + R) T

= E + nRT = E + PV

= H or H = nCpT

Page 12: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Keeping Track

Ideal Monatomic Gas

• Cv = 3/2R

• Cp = Cv + R = 5/2 R

Polyatomic Gas

• Cv > 3/2R

• Cp > 5/2 R

All Ideal Gases

• E = nCvT

• H = nCpT

Page 13: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Example

• What is q, w, E and H for a process in which one mole of an ideal monatomic gas with an initial volume of 5 l and pressure of 2.0 atm is heated until a volume of 10 l is reached with pressure unchanged?

Pinit = 2 atm

Vinit = 5 l

Tinit = ? K

Pfinal = 2 atm

Vfinal = 10 l

Tfinal = ? K

Page 14: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Example (cont.)

• Since PV = nRT (ideal gas law) we can determine T

• ThenV = (10 l - 5 l) = 5 l

• And:

2atm 5l (1mol) .0821l.atmmol.K

121.8K T

Page 15: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Example (cont.)

• Given this:

E nCvT (1mol) 12.5J mol.K 121.8K 1522.5J

H nCpT (1mol) 20.8J mol.K 121.8K 2533.4J

w PextV 2atm 5l 101.3J l.atm 1013.0J

qE w 1522.5J 1013.0J 2535.5J

Page 16: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

To Date….

Ideal Monatomic Gas

• Cv = 3/2R

• Cp = Cv + R = 5/2 R

Polyatomic Gas

• Cv > 3/2R

• Cp > 5/2 R

All Ideal Gases

• E = q + w

• w = -PextV (for now)

• E = nCvT = qV

• H = nCpT = qP

• If T = 0, then E = 0

and q = -w

Page 17: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

State Functions

• If we start in Seattle and end in Chicago, but you take different paths to get from one place to the other ..

• Will the energy/enthalpy, heat/work we spend be the same along both paths?

United States

L. Superior

OntarioL.Michigan

L.Huron

L.

ErieL.

Gulf of Mexico

Pacific Ocean

AtlanticOcean

WashingtonDC

SanFrancisco

LosAngeles

Chicago

Miami

New York

Detroit Boston

Dallas

Seattle

DenverSt.

Louis

Tampa

Atlanta

Houston

San Diego

Philadelphia

Minneapolis

Cleveland

Portland

Phoenix

OklahomaCity

Omaha

Kansas City

Memphis Raleigh

Cincinnati

NewOrleans

Indianapolis

San Jose

SanAntonio

Salt LakeCity

Orlando

Milwaukee

Jacksonville

Honolulu

Fairbanks

Charlotte

Buffalo

Baltimore

AnchorageCanada

Canada

Cuba

Mexico TheBahamas

200 km

200 miles

1000 km

1000 miles

1000 km

1000 miles

170 160

160

20

70

60

110 90 70

30

40

50

60

Page 18: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Thermodynamic Pathways: an Example

• Example 9.2. We take 2.00 mol of an ideal monatomic gas undergo the following:

– Initial (State A): PA = 2.00 atm, VA = 10.0 L

– Final (State B): PB = 1.00 atm, VB = 30.0 L

• We’ll do this two ways:Path 1: Expansion then CoolingPath 2: Cooling then Expansion

Page 19: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Thermodynamic Jargon

• When doing pathways, we usually keep one variable constant. The language used to indicate what is held constant is:

– Isobaric: Constant Pressure– Isothermal: Constant Temperature– Isochoric: Constant Volume

Page 20: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Thermodynamic Path: A series of manipulations of a system that takes the system from an initial state to

a final state

isochoric

isobaric

Page 21: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 1

• Step 1. Constant pressure expansion (P = 2 atm) from 10.0 l to 30.0 l.

– PV = (2.00 atm)(30.0 l - 10.0 l) = 40.0 l.atm

= (40.0 l.atm)(101.3 J/l.atm) = 4.0 x 103 J

= -w (the system does work)

– AndT = PV/nR = 4.05 x 103 J/(2 mol)(8.314 J/mol.K)

= 243.6 K (from the ideal gas law)

Page 22: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 1 (cont.)• Step 1 is isobaric (constant P); therefore,

– q1 = qP = nCpT = (2mol)(5/2R)(243.6 K) = 1.0 x 104 J

= H1

– AndE1 = nCvT = (2mol)(3/2R)(243.6 K) = 6.0 x 103 J

(check: E1 = q1 + w1 = (1.0 x 104 J) -(4.0 x 103 J) = 6.0 x 103 J )

Page 23: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 1 (cont.)

• Step 2: Isochoric (const. V) cooling until pressure is reduced from 2.00 atm to 1.00 atm.

• First, calculate T:– NowT = PV/nR (note: P changes, not V)

= (-1.00 atm)(30.0 l)/ (2 mol)(.0821 l.atm/mol K)

= -182.7 K

Page 24: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 1 (cont.)

• q2 = qv = nCvT = (2 mol)(3/2R)(-182.7 K)

= - 4.6 x 103 J

• and E2 = nCvT = -4.6 x 103 J

• and H2 = nCpT = -7.6 x 103 J

• Finally w2 = 0 (isochoric…no V change, no PV-type work)

Page 25: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 1 (end)

• Thermodynamic totals for this pathway are the sum of values for step 1 and step 2

q = q1 + q2 = 5.5 x 103 J

w = w1 + w2 = -4.0 x 103 J

E = E1 + E2 = 1.5 x 103 J

H = H1 + H2 = 2.5 x 103 J

Page 26: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Next Pathway

• Now we will do the same calculations for the green path.

Page 27: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 2

• Step 1: Isochoric cooling from P = 2.00 atm to P = 1.00 atm.

• First, calculate T: T = PV/nR = (-1.00 atm)(10.0 l)/ (2 mol)R

= -60.9 K

Page 28: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 2 (cont.)

• Then, calculate the rest for Step 1:

q1 = qv = nCvT = (2 mol)(3/2 R)(-60.9 K)

= -1.5 x 103 J = E1

H1 = nCPT = (2 mol)(5/2 R)(-60.9 K)

= -2.5 x 103 J

w1 = 0 (constant volume)

Page 29: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 2 (cont.)

• Step 2: Isobaric (constant P) expansion at 1.0 atm from 10.0 l to 30.0 l.

T = PV/nR = (1 atm)(20.0 l)/(2 mol)R

= 121.8 K

Page 30: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Pathway 2 (cont.)

• Then, calculate the rest:

q2 = qp = nCPT = (2 mol)(5/2 R)(121.8 K)

= 5.1 x 103 J = H2

E2 = nCvT = (2 mol)(3/2 R)(121.8 K)

= 3.1 x 103 J

w1 = -PV = -20 l.atm = -2.0 x 103 J

Page 31: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

• Thermodynamic totals for this pathway are again the sum of values for step 1 and step 2:

q = q1 + q2 = 3.6 x 103 J

w = w1 + w2 = -2.0 x 103 J

E = E1 + E2 = 1.5 x 103 J

H = H1 + H2 = 2.5 x 103 J

Pathway 2 (end)

Page 32: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Comparison of Path 1 and 2

• Pathway 1

q = 5.5 x 103 J

w = -4.1 x 103 J

E = 1.5 x 103 J

H = 2.5 x 103 J

• Pathway 2

q = 3.6 x 103 Jw = -2.0 x 103 JE = 1.5 x 103 JH = 2.5 x 103 J

Note: Energy and Enthalpy are the same,but heat and work are not the same!

Page 33: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

State Functions

• A State Function is a function in which the value only depends on the initial and final state….NOT on the pathway taken

United States

L. Superior

OntarioL.Michigan

L.Huron

L.

ErieL.

Gulf of Mexico

Pacific Ocean

AtlanticOcean

WashingtonDC

SanFrancisco

LosAngeles

Chicago

Miami

New York

Detroit Boston

Dallas

Seattle

DenverSt.

Louis

Tampa

Atlanta

Houston

San Diego

Philadelphia

Minneapolis

Cleveland

Portland

Phoenix

OklahomaCity

Omaha

Kansas City

Memphis Raleigh

Cincinnati

NewOrleans

Indianapolis

San Jose

SanAntonio

Salt LakeCity

Orlando

Milwaukee

Jacksonville

Honolulu

Fairbanks

Charlotte

Buffalo

Baltimore

AnchorageCanada

Canada

Cuba

Mexico TheBahamas

200 km

200 miles

1000 km

1000 miles

1000 km

1000 miles

170 160

160

20

70

60

110 90 70

30

40

50

60

Page 34: Lecture 2: Heat Capacities/State functions Reading: Zumdahl 9.3 Outline –Definition of Heat Capacity (C v and C p ) –Calculating  E and  H using C v

Thermodynamic State Functions

• Thermodynamic State Functions: Thermodynamic properties that are dependent on the state of the system only. (Example: E and H)

• Other variables will be dependent on pathway (Example: q and w). These are NOT state functions. The pathway from one state to the other must be defined.