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University Physics Volume 2

3.3 First Law of Thermodynamics

University Physics Volume 23.3 First Law of Thermodynamics
  1. Preface
  2. Unit 1. Thermodynamics
    1. 1 Temperature and Heat
      1. Introduction
      2. 1.1 Temperature and Thermal Equilibrium
      3. 1.2 Thermometers and Temperature Scales
      4. 1.3 Thermal Expansion
      5. 1.4 Heat Transfer, Specific Heat, and Calorimetry
      6. 1.5 Phase Changes
      7. 1.6 Mechanisms of Heat Transfer
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    2. 2 The Kinetic Theory of Gases
      1. Introduction
      2. 2.1 Molecular Model of an Ideal Gas
      3. 2.2 Pressure, Temperature, and RMS Speed
      4. 2.3 Heat Capacity and Equipartition of Energy
      5. 2.4 Distribution of Molecular Speeds
      6. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    3. 3 The First Law of Thermodynamics
      1. Introduction
      2. 3.1 Thermodynamic Systems
      3. 3.2 Work, Heat, and Internal Energy
      4. 3.3 First Law of Thermodynamics
      5. 3.4 Thermodynamic Processes
      6. 3.5 Heat Capacities of an Ideal Gas
      7. 3.6 Adiabatic Processes for an Ideal Gas
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    4. 4 The Second Law of Thermodynamics
      1. Introduction
      2. 4.1 Reversible and Irreversible Processes
      3. 4.2 Heat Engines
      4. 4.3 Refrigerators and Heat Pumps
      5. 4.4 Statements of the Second Law of Thermodynamics
      6. 4.5 The Carnot Cycle
      7. 4.6 Entropy
      8. 4.7 Entropy on a Microscopic Scale
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
  3. Unit 2. Electricity and Magnetism
    1. 5 Electric Charges and Fields
      1. Introduction
      2. 5.1 Electric Charge
      3. 5.2 Conductors, Insulators, and Charging by Induction
      4. 5.3 Coulomb's Law
      5. 5.4 Electric Field
      6. 5.5 Calculating Electric Fields of Charge Distributions
      7. 5.6 Electric Field Lines
      8. 5.7 Electric Dipoles
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
    2. 6 Gauss's Law
      1. Introduction
      2. 6.1 Electric Flux
      3. 6.2 Explaining Gauss’s Law
      4. 6.3 Applying Gauss’s Law
      5. 6.4 Conductors in Electrostatic Equilibrium
      6. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    3. 7 Electric Potential
      1. Introduction
      2. 7.1 Electric Potential Energy
      3. 7.2 Electric Potential and Potential Difference
      4. 7.3 Calculations of Electric Potential
      5. 7.4 Determining Field from Potential
      6. 7.5 Equipotential Surfaces and Conductors
      7. 7.6 Applications of Electrostatics
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    4. 8 Capacitance
      1. Introduction
      2. 8.1 Capacitors and Capacitance
      3. 8.2 Capacitors in Series and in Parallel
      4. 8.3 Energy Stored in a Capacitor
      5. 8.4 Capacitor with a Dielectric
      6. 8.5 Molecular Model of a Dielectric
      7. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    5. 9 Current and Resistance
      1. Introduction
      2. 9.1 Electrical Current
      3. 9.2 Model of Conduction in Metals
      4. 9.3 Resistivity and Resistance
      5. 9.4 Ohm's Law
      6. 9.5 Electrical Energy and Power
      7. 9.6 Superconductors
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    6. 10 Direct-Current Circuits
      1. Introduction
      2. 10.1 Electromotive Force
      3. 10.2 Resistors in Series and Parallel
      4. 10.3 Kirchhoff's Rules
      5. 10.4 Electrical Measuring Instruments
      6. 10.5 RC Circuits
      7. 10.6 Household Wiring and Electrical Safety
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    7. 11 Magnetic Forces and Fields
      1. Introduction
      2. 11.1 Magnetism and Its Historical Discoveries
      3. 11.2 Magnetic Fields and Lines
      4. 11.3 Motion of a Charged Particle in a Magnetic Field
      5. 11.4 Magnetic Force on a Current-Carrying Conductor
      6. 11.5 Force and Torque on a Current Loop
      7. 11.6 The Hall Effect
      8. 11.7 Applications of Magnetic Forces and Fields
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    8. 12 Sources of Magnetic Fields
      1. Introduction
      2. 12.1 The Biot-Savart Law
      3. 12.2 Magnetic Field Due to a Thin Straight Wire
      4. 12.3 Magnetic Force between Two Parallel Currents
      5. 12.4 Magnetic Field of a Current Loop
      6. 12.5 Ampère’s Law
      7. 12.6 Solenoids and Toroids
      8. 12.7 Magnetism in Matter
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    9. 13 Electromagnetic Induction
      1. Introduction
      2. 13.1 Faraday’s Law
      3. 13.2 Lenz's Law
      4. 13.3 Motional Emf
      5. 13.4 Induced Electric Fields
      6. 13.5 Eddy Currents
      7. 13.6 Electric Generators and Back Emf
      8. 13.7 Applications of Electromagnetic Induction
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    10. 14 Inductance
      1. Introduction
      2. 14.1 Mutual Inductance
      3. 14.2 Self-Inductance and Inductors
      4. 14.3 Energy in a Magnetic Field
      5. 14.4 RL Circuits
      6. 14.5 Oscillations in an LC Circuit
      7. 14.6 RLC Series Circuits
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    11. 15 Alternating-Current Circuits
      1. Introduction
      2. 15.1 AC Sources
      3. 15.2 Simple AC Circuits
      4. 15.3 RLC Series Circuits with AC
      5. 15.4 Power in an AC Circuit
      6. 15.5 Resonance in an AC Circuit
      7. 15.6 Transformers
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    12. 16 Electromagnetic Waves
      1. Introduction
      2. 16.1 Maxwell’s Equations and Electromagnetic Waves
      3. 16.2 Plane Electromagnetic Waves
      4. 16.3 Energy Carried by Electromagnetic Waves
      5. 16.4 Momentum and Radiation Pressure
      6. 16.5 The Electromagnetic Spectrum
      7. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
  4. A | Units
  5. B | Conversion Factors
  6. C | Fundamental Constants
  7. D | Astronomical Data
  8. E | Mathematical Formulas
  9. F | Chemistry
  10. G | The Greek Alphabet
  11. Answer Key
    1. Chapter 1
    2. Chapter 2
    3. Chapter 3
    4. Chapter 4
    5. Chapter 5
    6. Chapter 6
    7. Chapter 7
    8. Chapter 8
    9. Chapter 9
    10. Chapter 10
    11. Chapter 11
    12. Chapter 12
    13. Chapter 13
    14. Chapter 14
    15. Chapter 15
    16. Chapter 16
  12. Index

Learning Objectives

By the end of this section, you will be able to:
  • State the first law of thermodynamics and explain how it is applied
  • Explain how heat transfer, work done, and internal energy change are related in any thermodynamic process

Now that we have seen how to calculate internal energy, heat, and work done for a thermodynamic system undergoing change during some process, we can see how these quantities interact to affect the amount of change that can occur. This interaction is given by the first law of thermodynamics. British scientist and novelist C. P. Snow (1905–1980) is credited with a joke about the four laws of thermodynamics. His humorous statement of the first law of thermodynamics is stated “you can’t win,” or in other words, you cannot get more energy out of a system than you put into it. We will see in this chapter how internal energy, heat, and work all play a role in the first law of thermodynamics.

Suppose Q represents the heat exchanged between a system and the environment, and W is the work done by or on the system. The first law states that the change in internal energy of that system is given by QWQW. Since added heat increases the internal energy of a system, Q is positive when it is added to the system and negative when it is removed from the system.

When a gas expands, it does work and its internal energy decreases. Thus, W is positive when work is done by the system and negative when work is done on the system. This sign convention is summarized in Table 3.1. The first law of thermodynamics is stated as follows:

First Law of Thermodynamics

Associated with every equilibrium state of a system is its internal energy Eint.Eint. The change in EintEint for any transition between two equilibrium states is

ΔEint=QWΔEint=QW
(3.7)

where Q and W represent, respectively, the heat exchanged by the system and the work done by or on the system.

Thermodynamic Sign Conventions for Heat and Work
Process Convention
Heat added to system Q>0Q>0
Heat removed from system Q<0Q<0
Work done by system W>0W>0
Work done on system W<0W<0
Table 3.1

The first law is a statement of energy conservation. It tells us that a system can exchange energy with its surroundings by the transmission of heat and by the performance of work. The net energy exchanged is then equal to the change in the total mechanical energy of the molecules of the system (i.e., the system’s internal energy). Thus, if a system is isolated, its internal energy must remain constant.

Although Q and W both depend on the thermodynamic path taken between two equilibrium states, their difference QWQW does not. Figure 3.7 shows the pV diagram of a system that is making the transition from A to B repeatedly along different thermodynamic paths. Along path 1, the system absorbs heat Q1Q1 and does work W1;W1; along path 2, it absorbs heat Q2Q2 and does work W2,W2, and so on. The values of QiQi and WiWi may vary from path to path, but we have

Q1W1=Q2W2==QiWi=,Q1W1=Q2W2==QiWi=,

or

ΔEint1=ΔEint2==ΔEinti=.ΔEint1=ΔEint2==ΔEinti=.

That is, the change in the internal energy of the system between A and B is path independent. In the chapter on potential energy and the conservation of energy, we encountered another path-independent quantity: the change in potential energy between two arbitrary points in space. This change represents the negative of the work done by a conservative force between the two points. The potential energy is a function of spatial coordinates, whereas the internal energy is a function of thermodynamic variables. For example, we might write Eint(T,p)Eint(T,p) for the internal energy. Functions such as internal energy and potential energy are known as state functions because their values depend solely on the state of the system.

The figure is a graph of p on the vertical as a function of V on the horizontal axis. Six different curves are shown, all connecting a point A on the graph to a point B. The pressure at A is larger than at B, and the volume at A is lower than at B. Curve 1 goes up and curves around to reach B from above. Curve 2 is  similar to 1 but not as curved. Curve 3 is a straight line from A to B. Curve 4 wiggles a bit below the straight line of curve 3. Curve 5 bends down and around to B, reaching it from below. Curve 6 is similar to curve 5 but goes farther out.
Figure 3.7 Different thermodynamic paths taken by a system in going from state A to state B. For all transitions, the change in the internal energy of the system ΔEint=QWΔEint=QW is the same.

Often the first law is used in its differential form, which is

dEint=dQdW.dEint=dQdW.
(3.8)

Here dEintdEint is an infinitesimal change in internal energy when an infinitesimal amount of heat dQ is exchanged with the system and an infinitesimal amount of work dW is done by (positive in sign) or on (negative in sign) the system.

Example 3.2

Changes of State and the First Law During a thermodynamic process, a system moves from state A to state B, it is supplied with 400 J of heat and does 100 J of work. (a) For this transition, what is the system’s change in internal energy? (b) If the system then moves from state B back to state A, what is its change in internal energy? (c) If in moving from A to B along a different path, WAB=400JWAB=400J of work is done on the system, how much heat does it absorb?

Strategy The first law of thermodynamics relates the internal energy change, work done by the system, and the heat transferred to the system in a simple equation. The internal energy is a function of state and is therefore fixed at any given point regardless of how the system reaches the state.

Solution

  1. From the first law, the change in the system’s internal energy is
    ΔEintAB=QABWAB=400J100J=300J.ΔEintAB=QABWAB=400J100J=300J.
  2. Consider a closed path that passes through the states A and B. Internal energy is a state function, so ΔEintΔEint is zero for a closed path. Thus
    ΔEint=ΔEintAB+ΔEintBA=0,ΔEint=ΔEintAB+ΔEintBA=0,

    and
    ΔEintAB=ΔEintBA.ΔEintAB=ΔEintBA.

    This yields
    ΔEintBA=−300J.ΔEintBA=−300J.
  3. The change in internal energy is the same for any path, so
    ΔEintAB=ΔEintAB=QABWAB;300J=QAB(−400J),ΔEintAB=ΔEintAB=QABWAB;300J=QAB(−400J),

    and the heat exchanged is
    QAB=−100J.QAB=−100J.

    The negative sign indicates that the system loses heat in this transition.

Significance When a closed cycle is considered for the first law of thermodynamics, the change in internal energy around the whole path is equal to zero. If friction were to play a role in this example, less work would result from this heat added. Example 3.3 takes into consideration what happens if friction plays a role.

Notice that in Example 3.2, we did not assume that the transitions were quasi-static. This is because the first law is not subject to such a restriction. It describes transitions between equilibrium states but is not concerned with the intermediate states. The system does not have to pass through only equilibrium states. For example, if a gas in a steel container at a well-defined temperature and pressure is made to explode by means of a spark, some of the gas may condense, different gas molecules may combine to form new compounds, and there may be all sorts of turbulence in the container—but eventually, the system will settle down to a new equilibrium state. This system is clearly not in equilibrium during its transition; however, its behavior is still governed by the first law because the process starts and ends with the system in equilibrium states.

Example 3.3

Polishing a Fitting A machinist polishes a 0.50-kg copper fitting with a piece of emery cloth for 2.0 min. He moves the cloth across the fitting at a constant speed of 1.0 m/s by applying a force of 20 N, tangent to the surface of the fitting. (a) What is the total work done on the fitting by the machinist? (b) What is the increase in the internal energy of the fitting? Assume that the change in the internal energy of the cloth is negligible and that no heat is exchanged between the fitting and its environment. (c) What is the increase in the temperature of the fitting?

Strategy The machinist’s force over a distance that can be calculated from the speed and time given is the work done on the system. The work, in turn, increases the internal energy of the system. This energy can be interpreted as the heat that raises the temperature of the system via its heat capacity. Be careful with the sign of each quantity.

Solution

  1. The power created by a force on an object or the rate at which the machinist does frictional work on the fitting is F·v=FvF·v=Fv. Thus, in an elapsed time ΔtΔt (2.0 min), the work done on the fitting is
    W=FvΔt=(20N)(1.0m/s)(1.2×102s)=−2.4×103J.W=FvΔt=(20N)(1.0m/s)(1.2×102s)=−2.4×103J.
  2. By assumption, no heat is exchanged between the fitting and its environment, so the first law gives for the change in the internal energy of the fitting:
    ΔEint=W=2.4×103J.ΔEint=W=2.4×103J.
  3. Since ΔEintΔEint is path independent, the effect of the 2.4×103J2.4×103J of work is the same as if it were supplied at atmospheric pressure by a transfer of heat. Thus,
    2.4×103J=mcΔT=(0.50kg)(3.9×102J/kg·°C)ΔT,2.4×103J=mcΔT=(0.50kg)(3.9×102J/kg·°C)ΔT,

    and the increase in the temperature of the fitting is
    ΔT=12°C,ΔT=12°C,

    where we have used the value for the specific heat of copper, c=3.9×102J/kg·°Cc=3.9×102J/kg·°C.

Significance If heat were released, the change in internal energy would be less and cause less of a temperature change than what was calculated in the problem.

Check Your Understanding 3.2

g The quantities below represent four different transitions between the same initial and final state. Fill in the blanks.

Q (J) W (J) ΔEint(J)ΔEint(J)
–80 –120
90
40
–40
Table 3.2

Example 3.4

An Ideal Gas Making Transitions between Two States Consider the quasi-static expansions of an ideal gas between the equilibrium states A and C of Figure 3.6. If 515 J of heat are added to the gas as it traverses the path ABC, how much heat is required for the transition along ADC? Assume that p1=2.10×105N/m2,p2=1.05×105N/m2,V1=2.25×10−3m3,p1=2.10×105N/m2,p2=1.05×105N/m2,V1=2.25×10−3m3, and V2=4.50×10−3m3.V2=4.50×10−3m3.

Strategy The difference in work done between process ABC and process ADC is the area enclosed by ABCD. Because the change of the internal energy (a function of state) is the same for both processes, the difference in work is thus the same as the difference in heat transferred to the system.

Solution For path ABC, the heat added is QABC=515JQABC=515J and the work done by the gas is the area under the path on the pV diagram, which is

WABC=p1(V2V1)=473J.WABC=p1(V2V1)=473J.

Along ADC, the work done by the gas is again the area under the path:

WADC=p2(V2V1)=236J.WADC=p2(V2V1)=236J.

Then using the strategy we just described, we have

QADCQABC=WADCWABC,QADCQABC=WADCWABC,

which leads to

QADC=QABC+WADCWABC=(515+236473)J=278J.QADC=QABC+WADCWABC=(515+236473)J=278J.

Significance The work calculations in this problem are made simple since no work is done along AD and BC and along AB and DC; the pressure is constant over the volume change, so the work done is simply pΔVpΔV. An isothermal line could also have been used, as we have derived the work for an isothermal process as W=nRTlnV2V1W=nRTlnV2V1.

Example 3.5

Isothermal Expansion of an Ideal Gas Heat is added to 1 mol of an ideal monatomic gas confined to a cylinder with a movable piston at one end. The gas expands quasi-statically at a constant temperature of 300 K until its volume increases from V to 3V. (a) What is the change in internal energy of the gas? (b) How much work does the gas do? (c) How much heat is added to the gas?

Strategy (a) Because the system is an ideal gas, the internal energy only changes when the temperature changes. (b) The heat added to the system is therefore purely used to do work that has been calculated in Work, Heat, and Internal Energy. (c) Lastly, the first law of thermodynamics can be used to calculate the heat added to the gas.

Solution

  1. We saw in the preceding section that the internal energy of an ideal monatomic gas is a function only of temperature. Since ΔT=0ΔT=0, for this process, ΔEint=0.ΔEint=0.
  2. The quasi-static isothermal expansion of an ideal gas was considered in the preceding section and was found to be
    W=nRTlnV2V1=nRTln3VV=(1.00mol)(8.314J/K·mol)(300K)(ln3)=2.74×103J.W=nRTlnV2V1=nRTln3VV=(1.00mol)(8.314J/K·mol)(300K)(ln3)=2.74×103J.
  3. With the results of parts (a) and (b), we can use the first law to determine the heat added:
    ΔEint=QW=0,ΔEint=QW=0,

    which leads to
    Q=W=2.74×103J.Q=W=2.74×103J.

Significance An isothermal process has no change in the internal energy. Based on that, the first law of thermodynamics reduces to Q=WQ=W.

Check Your Understanding 3.3

Why was it necessary to state that the process of Example 3.5 is quasi-static?

Example 3.6

Vaporizing Water When 1.00 g of water at 100°C100°C changes from the liquid to the gas phase at atmospheric pressure, its change in volume is 1.67×10−3m3.1.67×10−3m3. (a) How much heat must be added to vaporize the water? (b) How much work is done by the water against the atmosphere in its expansion? (c) What is the change in the internal energy of the water?

Strategy We can first figure out how much heat is needed from the latent heat of vaporization of the water. From the volume change, we can calculate the work done from W=pΔVW=pΔV because the pressure is constant. Then, the first law of thermodynamics provides us with the change in the internal energy.

Solution

  1. With LvLv representing the latent heat of vaporization, the heat required to vaporize the water is
    Q=mLv=(1.00g)(2.26×103J/g)=2.26×103J.Q=mLv=(1.00g)(2.26×103J/g)=2.26×103J.
  2. Since the pressure on the system is constant at 1.00atm=1.01×105N/m21.00atm=1.01×105N/m2, the work done by the water as it is vaporized is
    W=pΔV=(1.01×105N/m2)(1.67×10−3m3)=169J.W=pΔV=(1.01×105N/m2)(1.67×10−3m3)=169J.
  3. From the first law, the thermal energy of the water during its vaporization changes by
    ΔEint=QW=2.26×103J169J=2.09×103J.ΔEint=QW=2.26×103J169J=2.09×103J.

Significance We note that in part (c), we see a change in internal energy, yet there is no change in temperature. Ideal gases that are not undergoing phase changes have the internal energy proportional to temperature. Internal energy in general is the sum of all energy in the system.

Check Your Understanding 3.4

When 1.00 g of ammonia boils at atmospheric pressure and −33.0°C,−33.0°C, its volume changes from 1.47 to 1130cm31130cm3. Its heat of vaporization at this pressure is 1.37×106J/kg.1.37×106J/kg. What is the change in the internal energy of the ammonia when it vaporizes?

Interactive

View this site to learn about how the first law of thermodynamics. First, pump some heavy species molecules into the chamber. Then, play around by doing work (pushing the wall to the right where the person is located) to see how the internal energy changes (as seen by temperature). Then, look at how heat added changes the internal energy. Finally, you can set a parameter constant such as temperature and see what happens when you do work to keep the temperature constant (Note: You might see a change in these variables initially if you are moving around quickly in the simulation, but ultimately, this value will return to its equilibrium value).

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