Lecture Notes on Thermodynamics and Entropy

Second Law of Thermodynamics (10.3, 10.5)

  • It is impossible to obtain an equal amount of work out of a system relative to the energy put into it under isothermal reversible conditions.
    • W_{rev}
  • For a real system:
    • Any spontaneous process occurring without outside intervention must increase the entropy of the Universe.
    • \Delta S{univ} = \Delta S{sys} + \Delta S_{surr}
      • \Delta S_{univ} will always increase for a real process until it reaches a max: Heat death of the Universe
    • Reversible:
      • \Delta S{sys} = -\Delta S{surr}

Enthalpy

  • Real processes that are both spontaneous
  • H₂O(g) ⇌ H₂O(l)
    • \Delta H_{vap}: H₂O(l) → H₂O(g)
    • \Delta H{cond}: H₂O(g) → H₂O(l) = -\Delta H{vap}
    • \Delta S{sys} > 0: \Delta S{vap}
      • Heat is stolen from the surroundings, increasing disorder, the system gains more order
      • Endothermic
    • H₂O(g) → H₂O(l)
      • \Delta S{sys} < 0: \Delta S{cond}
      • Heat is dumped into the surroundings in the form of disordered thermal motion
      • Exothermic

Entropy Problem

  • Methane (CH₄) has a heat of vaporization of 8.17 kJ/mole and a boiling point of -162 °C.
  • Calculate the entropy change methane undergoes associated with going from a gas to liquid.
    • Condensation: gas → liquid
    • T{surr} = T{B.P.}
    • \Delta S{sys} = \frac{q{rev}}{T{surr}} = \frac{\Delta H{cond}}{T_{B.P.}}
    • \Delta S{sys} = \frac{-\Delta H{vap}}{T_{B.P.}}
    • \Delta S_{sys} = \frac{-8170 \frac{J}{mol}}{111 K} = -73.6 \frac{J}{mol \cdot K}

Microscopic View of Entropy

  • Assumed Kinetic Molecular Theory (KMT):
    • Atoms exist, they have mass + velocity
    • KE → velocity
  • Result:
    • Energies of a gas follows a Gaussian Distribution
  • Ludwig Boltzmann showed over time any distribution of gas energies will evolve to a gaussian
    • Entropy on a molecular level evolves over time to a max value

Microscopic View of Entropy (10.1)

  • Boltzmann realized the more "positions" (Energy + locations) available to a system, the more likely that state is.
  • Boltzmann Equation:
    • S = k_B \ln \Omega
      • S = Entropy
      • \Omega = # of microstates representing that state
      • kB= Boltzmann Constant: \frac{R}{NA} = \frac{8.314 \frac{J}{K \cdot mol}}{6.022 \times 10^{23} \frac{molecules}{mol}}
    • Microstate: Arrangement of position & Energy of a system
    • \Delta S = S2 - S1 = kB \ln \frac{\Omega2}{\Omega_1}

Microscopic View of Entropy (10.3)

  • Example 1: 1 atom in an expanding Box
    • Ideal gas expands thermally
    • Double the volume
      • V2 = 2 \cdot V1
      • \Omega2 = 2 \cdot \Omega1
    • \Delta S = kB \ln (\frac{2\Omega1}{\Omega1}) = kB \ln (2)
    • This is why gases expand to fill their containers; \Delta S increases

Microscopic View of Entropy (Table 10.2)

  • Example 2
  • State I: AB CD
  • State II: A B C D
  • Microstates (\Omega)
    • I: [AB, CD]
    • II: [AC, BD], [AD, BC], [A,B,C,D]
  • \Delta S{I \rightarrow II} = kB \ln (4)

Microscopic View of Entropy and 2nd Law (10.5)

  • Entropy is a measure of the # of Equivalent Configurations (Energy & location) of a State
    • More configurations, higher S → More configurations, more likely
  • Over time, \Delta S becomes more positive
  • 2nd Law:
    • \Delta S{univ} = \Delta S{sys} + \Delta S_{surr}
    • \Delta S_{univ} increases

Entropy Changes At the Molecular Level (10.8)

  • H₂O(g) → H₂O(s) : \Delta S -
  • NaCl(s) → Na⁺(aq) + Cl⁻(aq) : \Delta S +
  • N₂(g) + 3H₂(g) → 2NH₃(g) : \Delta S -
  • Need to know something about the molecule

Degrees of Freedom and Entropy

  • # degrees of freedom = #ways a molecule can move
    • translate
    • rotate
    • vibrate
  • Linear: 3N-5
  • Non-Linear: 3N-6
  • N = # nuclei in molecule
  • More degrees of freedom → higher S
    • H₂O larger S than H₂