Thermodynamics Review

Heat Capacity (c)

  • The amount of heat needed to change the temperature of an object.

Molar Heat Capacity

  • Amount of substance in moles.

Specific Heat Capacity

  • Amount of substance in grams.

Constants and Values

  • R=0.08206LatmmolKR = 0.08206 \frac{L \cdot atm}{mol \cdot K}
  • 1LatmmolK=101.3J1 \frac{L \cdot atm}{mol \cdot K} = 101.3 J
  • R=8.3145JmolKR = 8.3145 \frac{J}{mol \cdot K}

Heat Capacity at Constant Volume and Pressure

  • C_M = \frac{#J}{mol \cdot K}
  • C_V = \frac{#J}{g \cdot K}
  • Constant Volume: CVC_V
  • Constant Pressure: CPC_P
  • For monatomic gases: CP=52RC_P = \frac{5}{2} R
  • Because ΔT\Delta T (in Kelvin) = ΔT\Delta T (in Celsius), K and °C can be interchanged when calculating temperature differences.

Heat Capacity at Constant Volume (Cᵥ)

  • Ideal Gas: (KE)avg=32RT(KE)_{avg} = \frac{3}{2} RT
  • No change in volume (ΔV\Delta V) means no work is done.
  • Translational movement:
    CV=32RC_V = \frac{3}{2} R

Heat Capacity at Constant Pressure (Cₚ)

  • CP=C_P = translational + work
  • C<em>P=C</em>V+R=52RC<em>P = C</em>V + R = \frac{5}{2}R

Heat Capacity Problem (Non-Monoatomic Ideal Gas)

  • Water has a heat capacity of 4.18Jg°C4.18 \frac{J}{g \cdot °C}.
  • A 20.0g20.0 g block of iron heated to 234°C234 °C is added to 100.g100. g of water at 25.0°C25.0 °C.
  • The water's final temperature is 29.4°C29.4 °C.
  • Goal: Find the heat capacity of iron.
  • Final temperature of iron & water is the same due to the 0th Law Consequence.
  • q<em>H</em>2O=qFeq<em>{H</em>2O} = -q_{Fe}
  • 1st Law Consequence:
    m<em>FeC</em>S,FeΔT<em>Fe=m</em>H<em>2OC</em>S,H<em>2OΔT</em>H<em>2Om<em>{Fe} \cdot C</em>{S,Fe} \cdot \Delta T<em>{Fe} = - m</em>{H<em>2O} \cdot C</em>{S,H<em>2O} \cdot \Delta T</em>{H<em>2O}C</em>S,Fe=m<em>H</em>2OC<em>S,H</em>2OΔT<em>H</em>2Om<em>FeΔT</em>FeC</em>{S,Fe} = \frac{m<em>{H</em>2O} \cdot C<em>{S,H</em>2O} \cdot \Delta T<em>{H</em>2O}}{- m<em>{Fe} \cdot \Delta T</em>{Fe}}
  • This calculates the heat needed to change the temperature of a mass of a substance.
  • CS,Fe=100.g4.18Jg°C(29.425.0)°C20.0g(29.4234)°C=0.450Jg°CC_{S,Fe} = \frac{100.g \cdot 4.18 \frac{J}{g \cdot °C} \cdot (29.4 - 25.0)°C}{-20.0g \cdot (29.4 - 234)°C} = 0.450 \frac{J}{g \cdot °C}.

State Functions 9.1

  • A state function depends only on its present position, not how it got there.
  • Also called pathway-independent functions.

Examples of State Functions

  • P, V, T, E, H, G, S (Entropy)

Examples of Non-State Functions

  • q and w

  • If ab=\frac{a}{b} = Not state function, but ΔaΔb=\frac{\Delta a}{\Delta b} = state function.

State Functions

  • ΔE=q+w\Delta E = q + w
  • If w=0Jw = 0 J, ΔE=q\Delta E = q
  • q and w are pathway dependent.
  • Conclusion: ΔE\Delta E is a state function, while q and w are not.

ΔE\Delta E, q, w, and Pathways

  • ΔE=q+w\Delta E = q + w
  • w=PΔVw = -P \Delta V
  • The work is the area under the curve on a P-V diagram.
  • Pathways 1 and 2:
    • ΔE<em>1=ΔE</em>2\Delta E<em>1 = \Delta E</em>2 because ΔE\Delta E is path independent
    • q<em>1q</em>2q<em>1 \neq q</em>2

ΔE\Delta E, q, w, and Pathways

  • System: 1.0 mole of monatomic ideal gas in a 5.0 L cylinder at 5.0 atm.
  • Final state: 1.0 L and 7.0 atm.
  • Calculate q, w, and ΔE\Delta E (in J) for two paths:
    1. Compression in volume, then increase in pressure.
    2. Increase in pressure, then compression in volume.
  • Important Equations:
    • CV=32RC_V = \frac{3}{2} R
    • CP=52RC_P = \frac{5}{2} R
    • R=8.314JmolKR = 8.314 \frac{J}{mol \cdot K}
    • ΔE=q+w\Delta E = q + w
    • w=PΔVw = -P \Delta V
    • q=nCΔTq = nC \Delta T
    • ΔT=Δ(PV)nR\Delta T = \frac{\Delta (PV)}{nR}
    • R=0.08204LatmmolKR = 0.08204 \frac{L \cdot atm}{mol \cdot K}

Path 1

  • Path 1: A -> B -> D

    • A -> B: (5.0 L, 5.0 atm) -> (1.0 L, 5.0 atm) *constant P
    • B -> D: (1.0 L, 5.0 atm) -> (1.0 L, 7.0 atm) *constant V
  • Step IA: A → B

    • w1=PΔV=5.0atm(4.0L)=+20.0Latmw_1 = -P \Delta V = -5.0 atm \cdot (-4.0 L) = +20.0 L \cdot atm
    • q<em>1=nC</em>PΔT=n(52R)(Δ(PV)nR)=52(20.0Latm)=50.0Latmq<em>1 = nC</em>P \Delta T = n (\frac{5}{2}R) (\frac{\Delta (PV)}{nR}) = \frac{5}{2} (-20.0 L \cdot atm) = -50.0 L \cdot atm
  • Step IB: B → D

    • w2=PΔV=0Latmw_2 = -P \Delta V = 0 L \cdot atm
    • q<em>2=nC</em>VΔT=n(32R)(Δ(PV)nR)=32(2.0Latm)=3.0Latmq<em>2 = nC</em>V \Delta T = n (\frac{3}{2}R) (\frac{\Delta (PV)}{nR}) = \frac{3}{2} (2.0 L \cdot atm) = 3.0 L \cdot atm
  • Total:

    • q=q<em>1+q</em>2=(50.0+3.0)Latm=47Latm=4800Jq = q<em>1 + q</em>2 = (-50.0 + 3.0) L \cdot atm = -47 L \cdot atm = -4800 J
    • w=w<em>1+w</em>2=20+0=20Latm=2000Jw = w<em>1 + w</em>2 = 20 + 0 = 20 L \cdot atm = 2000 J
    • ΔE=q+w=4800J+2000J=2800J\Delta E = q + w = -4800 J + 2000 J = -2800 J

Path 2

  • Path 2: A -> C -> D

  • C<em>V=(32)R;C</em>P=(52)R;w=PΔV;q=nCΔTC<em>V = (\frac{3}{2})R; C</em>P = (\frac{5}{2})R; w = -P\Delta V; q = nC\Delta T

  • a) 5.0 L, 5.0 atm to 5.0 L, 7.0 atm

  • b) 5.0 L, 7.0 atm to 1.0 L, 7.0 atm

  • Step 2A: A→C

    • (5.0L, 5.0 atm) -> (5.0L, 7.0 atm) *const V
    • w1=PDV=0Latmw_1 = -PDV = 0 L \cdot atm
    • q1=32(ΔPV)=32(10Latm)=15Latmq_1 = \frac{3}{2} (\Delta PV) = \frac{3}{2} (10 L \cdot atm) = 15 L \cdot atm
  • Step 2B: C→D

    • (5.0L, 7.0 atm) -> (1.0L, 7.0 atm) *const P
    • w2=PAV=(7.0atm)(4.0L)=28Latmw_2 = -PAV = -(7.0 atm) (-4.0L) = 28 L \cdot atm
    • q2=52(ΔPV)=52(27Latm)=70.Latmq_2 = \frac{5}{2} (\Delta PV) = \frac{5}{2} (-27 L \cdot atm) = -70. L \cdot atm
  • Total

    • q=q<em>1+q</em>2=55Latm=5400Jq = q<em>1 + q</em>2 = -55 L \cdot atm = -5400 J
    • w=w<em>1+w</em>2=28Latm=2800Jw = w<em>1 + w</em>2 = 28 L \cdot atm = 2800 J
    • ΔE=q+w=2800J\Delta E = q + w = -2800J

Enthalpy (H) and Its Relationship to Internal Energy (E) 9.2

Enthalpy

  • By definition: H=E+PVH = E + PV. Thus, ΔH=ΔE+Δ(PV)\Delta H = \Delta E + \Delta (PV). E, P, and V are all state functions, so H is also a state function.

Work

  • w=PΔVw = -P \Delta V
  • \Delta E = q + w => q_P = \Delta E + P \Delta V
  • ΔH=qP\Delta H = q_P This is why enthalpy is sometimes called a heat.

Hess's Law 9.5

  • Hess's Law states that because ΔH\Delta H is a state function, we can calculate an unknown ΔHr\Delta H_r by generating a thermocycle from a series of known ΔH\Delta H values.
  • ΔH<em>r=ΔH</em>1+ΔH<em>2+ΔH</em>3\Delta H<em>r = \Delta H</em>1 + \Delta H<em>2 + \Delta H</em>3