Thermodynamics: Entropy and Spontaneity - Detailed Study Notes

The Second Law of Thermodynamics

  • Focus: The degree of disorder (entropy) of a system.

Entropy: Qualitative Description

  • Entropy is a measure of how spread out a system’s energy is in space.

  • For a given system, the greater the volume it occupies, the greater its entropy.

Entropy: Quantitative Description — 1st Approach (Boltzmann)

  • Boltzmann’s definition: S = k \, \ln W

    • where S is entropy, k = 1.38 \times 10^{-23}\ \mathrm{J\,K^{-1}} is the Boltzmann constant.

    • W = number of energetically equivalent ways the molecules in a system can be arranged.

  • In the slide: W = X^N where

    • X = number of cells (or microstates per molecule)

    • N = number of molecules

  • Concept: More microstates (larger W) -> larger entropy.

Entropy and Microstates (Illustrative Example)

  • Figure description (conceptual): two-compartment container separated by a barrier.

    • Before barrier removal: molecules confined to left side; 2 cells, 2 molecules → 4 possible arrangements.

    • After barrier removal: volume (and number of cells) doubles; new number of possible arrangements is 4^2 = 16, of which eight place molecules on opposite sides (the most probable outcome).

  • Key takeaway: Increasing volume increases the number of microstates, hence increases entropy.

Entropy: Three Possible States for a Two-Molecule System (Qualitative Count)

  • Three states discussed:
    1) One molecule on each side (8 possible arrangements).
    2) Both molecules on the left side (4 possible arrangements).
    3) Both molecules on the right side (4 possible arrangements).

  • Principle: The state with the largest number of possible arrangements (microstates) has the greatest entropy.

  • General rule: Entropy increases with the number of microstates of the system.

Entropy Changes in Reactions: Phase Transitions

  • Predicting ΔS for reactions:

    • Melting: S{\text{liquid}} > S{\text{solid}}

    • Vaporization: S{\text{gas}} > S{\text{liquid}}

    • Dissolving: S{\text{solution}} > S{\text{solute}} + S_{\text{solvent}}

Sample Exercise 2: Sign of ΔS for Various Processes

  • a) Decomposition of CaCO₃(s) → CaO(s) + CO₂(g) → ΔS positive.

  • b) Heating bromine vapor from 450°C to 800°C → ΔS positive.

  • c) Condensation of water vapor on a cold surface → ΔS negative.

  • d) NH₂(g) + HCl(g) → NH₄Cl(s) → ΔS negative.

  • e) Dissolution of sugar in water → ΔS positive.

  • Answers: +, +, -, -, +.

Sample Exercise 3: Positive ΔS Determination

  • Which reactions have ΔS > 0?

    • a) 2 O₃(g) → 3 O₂(g) → likely positive (more gas molecules).

    • b) 4 Fe(s) + 3 O₂(g) → 2 Fe₂O₃(s) → negative (formation of a solid).

    • c) 2 H₂O₂(aq) → 2 H₂O(l) + O₂(g) → positive (gas produced, liquids decreased).

    • d) 2 Li(s) + 2 H₂O(l) → 2 LiOH(aq) + H₂(g) → positive (gas produced + ions in solution).

    • e) 2 NH₃(g) → N₂(g) + 3 H₂(g) → positive.

  • Answer: All except b (i.e., a, c, d, e have ΔS > 0).

Entropy: 2nd Approach — Clausius Equation

  • Rudolph Clausius extended Carnot’s work:

    • \Delta S = \frac{q_{\text{rev}}}{T}

    • where q_{\text{rev}} is the heat released or absorbed in a reversible process and T is the temperature (K) at which the heat transfer occurred.

  • This equation encapsulates the core idea that entropy increases in spontaneous processes (for the universe).

Entropy and the Second Law (Fundamental Statement)

  • The entropy change of the universe for a reversible process is zero; for an irreversible (spontaneous) process it is positive:

    • \Delta S{\text{universe}} = \Delta S{\text{sys}} + \Delta S_{\text{surr}}

    • Reversible: \Delta S_{\text{universe}} = 0

    • Irreversible: \Delta S_{\text{universe}} > 0

  • The overarching principle: “The entropy of the universe increases for any spontaneous process.”

Sample Exercise 4: Condensation of Ethanol at its Boiling Point

  • Given: Normal boiling point of ethanol, C2H5OH, is 78.30^{\circ}C; enthalpy of vaporization \Delta H_{vap} = 38.56\ \text{kJ/mol}; 68.3 g of ethanol at 1 atm condenses to liquid at the normal boiling point.

  • Steps (as shown):

    • Moles of ethanol: n = \frac{68.3\ \text{g}}{46.07\ \text{g/mol}} \approx 1.4835\ \text{mol}

    • Heat released reversibly (condensation): q{rev} = -n \Delta H{vap} = -1.4835 \times 38.56\ \text{kJ} \approx -57.2\ \text{kJ}

    • Temperature at condensation: T = 351.3\ \text{K}

    • Entropy change of system: \Delta S{sys} = \frac{q{rev}}{T} \approx \frac{-57.2\ \text{kJ}}{351.3\ \text{K}} \approx -0.163\ \text{kJ K}^{-1}

    • Therefore: \Delta S_{system} \approx -0.163\ \text{kJ K}^{-1}

  • Note: Some slides show units as kJ/mol, but standard practice for entropy is J/(mol·K).

Entropy Changes in the Universe: Surroundings and System

  • Definitions:

    • The system is the portion of the universe being studied; the surroundings are everything else.

    • The universe is the sum: \Delta S{\text{universe}} = \Delta S{\text{system}} + \Delta S_{\text{surroundings}}

  • For a reversible process: \Delta S_{\text{universe}} = 0

  • For an irreversible process: \Delta S_{\text{universe}} > 0

  • Insight: These relationships underpin the second law: the total entropy of the universe increases for spontaneous processes.

Sample Exercise 5: Entropy Change and Surroundings

  • Reaction: Na(s) + Cl₂(g) → NaCl(s). Spontaneous with a decrease in the entropy of the system.

  • Conclusion: Since the reaction is spontaneous but reduces system entropy, the entropy change of the surroundings must increase: \Delta S_{\text{surroundings}} > 0.

  • Answer: a. ΔSsurroundings increases.

Entropy Changes in Everyday Processes (Universe Perspective)

  • Ice melts at room temperature (endothermic):

    • Heat flows from surroundings to system.

    • Surroundings temperature decreases; \Delta S{sys} > 0; \Delta S{surroundings} < 0.

  • Hot cocoa cools spontaneously to room temperature (exothermic):

    • Heat flows from system to surroundings.

    • Surroundings temperature increases; \Delta S{sys} < 0; \Delta S{surroundings} > 0.

ΔS°rxn (Standard Entropy of Reaction)

  • Definition: \Delta S^{\circ}{\mathrm{rxn}} = \sum\limits{\text{products}} \nui S^{\circ}{i,\text{products}} - \sum\limits{\text{reactants}} \nuj S^{\circ}_{j,\text{reactants}}

  • Note: S^{\circ} are standard molar entropies (units: J mol⁻¹ K⁻¹).

  • Hess’s Law can be applied to standard entropies of reaction.

Sample Exercise 6: Be(OH)₂(s) → BeO(s) + H₂O(g)

  • Given: S^{\circ} Be(OH)₂(s) = 50.21 J mol⁻¹ K⁻¹, BeO(s) = 13.77 J mol⁻¹ K⁻¹, H₂O(g) = 188.83 J mol⁻¹ K⁻¹.

  • Calculation:

    • \Delta S^{\circ}_{\mathrm{rxn}} = [1\cdot S^{\circ}(\text{BeO}) + 1\cdot S^{\circ}(\text{H₂O(g)})] - [1\cdot S^{\circ}(\text{Be(OH)₂(s)})]

    • = (13.77 + 188.83) - 50.21 = 152.39\ \text{J K}^{-1}\text{ mol}^{-1}

  • Result: \Delta S^{\circ}_{\mathrm{rxn}} \approx +152.4\ \text{J K}^{-1}\text{ mol}^{-1}

Sample Exercise 7: CO₂(g) + H₂O(g) → CH₃OH(g) + O₂(g)

  • Given: S° values (units shown as kJ/mol in slides, but treated as J mol⁻¹ K⁻¹):

    • CO₂(g) = 213.6; H₂O(g) = 188.83; CH₃OH(g) = 237.6; O₂(g) = 205.0.

  • Stoichiometry shown in slides (note: actual balancing in slides appears inconsistent; use the exact given calculation for consistency):

    • Products: 2 CH₃OH and 3 O₂ → 2\cdot 237.6 + 3\cdot 205.0 = 1090.2\,\text{J mol}^{-1}\text{K}^{-1}

    • Reactants: 2 CO₂ and 4 H₂O → 2\cdot 213.6 + 4\cdot 188.83 = 1182.52\,\text{J mol}^{-1}\text{K}^{-1}

    • \Delta S^{\circ}_{\mathrm{rxn}} = 1090.2 - 1182.52 = -92.3\ \text{J K}^{-1}\text{ mol}^{-1}

  • Note: The exact stoichiometric balancing for the listed transformation may differ; the slide’s calculation yields \Delta S^{\circ}_{\mathrm{rxn}} \approx -92.3\ \text{J K}^{-1}\text{ mol}^{-1} for the given coefficients.

Unfolded vs Folded; Active vs Inactive (Biological Context)

  • Slides show a schematic of enzyme catalysis: unfolded (active catalysis) → folded state (active catalysis) → chain of enzyme conformations; highlights that entropy changes in immediate surroundings for biological processes can be difficult to determine.

  • Key takeaway: In biology, local entropy changes can be hard to measure; overall universe considerations still apply.

Gibbs Free Energy and Spontaneity

  • Relationships that connect enthalpy, entropy, and spontaneity at constant temperature and pressure:

    • Entropy of the universe: \Delta S{\mathrm{univ}} = \Delta S{\mathrm{sys}} + \Delta S_{\mathrm{surr}}

    • Surroundings at constant pressure: \Delta S{\mathrm{surr}} = \frac{q{\mathrm{sys}}}{T} = \frac{-\Delta H_{\mathrm{sys}}}{T}

    • Therefore: \Delta S{\mathrm{univ}} = \Delta S{\mathrm{sys}} - \frac{\Delta H_{\mathrm{sys}}}{T}

  • Rearrange to connect with Gibbs free energy:

    • -T\,\Delta S{\mathrm{univ}} = \Delta H{\mathrm{sys}} - T\,\Delta S{\mathrm{sys}} = \Delta G{\mathrm{sys}}

    • Thus, \Delta G = \Delta H - T\Delta S

  • Condition for spontaneity at constant temperature and pressure:

    • If \Delta G < 0, the process is spontaneous in the forward direction.

    • If \Delta G > 0, the process is nonspontaneous in the forward direction (the reverse is spontaneous).

    • If \Delta G = 0, the system is at equilibrium.

Sign Table: How AH and AS Affect Spontaneity

  • A compact summary (signs of \Delta H and \Delta S determine spontaneity at different temperatures):

    • If \Delta H > 0 and \Delta S > 0: spontaneous at high T, nonspontaneous at low T.

    • If \Delta H < 0 and \Delta S < 0: spontaneous at low T, nonspontaneous at high T.

    • If one sign is positive and the other negative, spontaneity depends on the magnitude of T.

    • The formula to use is: \Delta G = \Delta H - T\Delta S.

Sample Exercise 1: Melting Ice at Room Temperature

  • Given: \Delta H{sys} = 53.6\ \text{kJ}, \Delta S{sys} = 132\ \text{J K}^{-1}\text{mol}^{-1}, room temperature T = 25^{\circ}C = 298\ \text{K}.

  • Compute \Delta G = \Delta H - T\Delta S:

    • Convert entropy to kJ: \Delta S = 0.132\ \text{kJ K}^{-1}\text{mol}^{-1}.

    • \Delta G = 53.6 - (298\ \text{K})(0.132) \approx 53.6 - 39.3 \approx 14.3\ \text{kJ}

  • Result: Nonspontaneous at room temperature (positive \Delta G).

Sample Exercise 2: Free Energy of a Reaction

  • Given: \Delta H{sys} = -35.4\ \text{kJ}, \Delta S{sys} = -85.5\ \text{J K}^{-1}\text{mol}^{-1}, T = 25^{\circ}C = 298\ \text{K}.

  • Compute \Delta G = \Delta H - T\Delta S:

    • Convert entropy to kJ: \Delta S = -0.0855\ \text{kJ K}^{-1}\text{mol}^{-1}.

    • \Delta G = -35.4 - (298)(-0.0855) \approx -35.4 + 25.5 \approx -9.92\ \text{kJ}

  • Result: Spontaneous reaction.

ΔG°rxn and Formation Energies

  • Standard Gibbs energy change of reaction:

    • \Delta G^{\circ}{\mathrm{rxn}} = \sum{\text{products}} \nui \Delta G^{\circ}{f,i} - \sum{\text{reactants}} \nuj \Delta G^{\circ}_{f,j}

    • where \Delta G^{\circ}_{f} is the standard free energy of formation (in J mol⁻¹).

  • Important note: For pure solids, pure liquids, and elements in their standard states, \Delta G^{\circ}_{f} = 0 by convention (Hess’s Law applied to standard free energies).

Sample Exercise 3: Standard Gibbs Energy Changes

  • Reaction: \mathrm{CH}4(g) + 2\ \mathrm{O}2(g) \rightarrow \mathrm{CO}2(g) + 2\ \mathrm{H}2\mathrm{O}(l)

  • Given: \Delta G^{\circ}{f}(\mathrm{CH4}) = -50.4\ \text{kJ/mol}, \Delta G^{\circ}{f}(\mathrm{CO2}) = -394.4\ \text{kJ/mol}, \Delta G^{\circ}{f}(\mathrm{H2O(l)}) = -237.1\ \text{kJ/mol}

  • Compute: \Delta G^{\circ}_{\mathrm{rxn}} = [(-394.4) + 2(-237.1)] - [(-50.4) + 2(0)]

  • Result (given): -818.2\ \text{kJ/mol}; spontaneous.

Sample Exercise 4: MgO Decomposition

  • Reaction: \mathrm{MgO(s)} \rightarrow \mathrm{Mg(s)} + \mathrm{O_2(g)}

  • Given: \Delta G^{\circ}_{f}(\mathrm{MgO(s)}) = -569.3\ \text{kJ/mol}; Mg(s) and O₂(g) have 0 formation energy in their standard states.

  • Result (given): \Delta G^{\circ}_{\mathrm{rxn}} = +1139\ \text{kJ/mol}; nonspontaneous.

Pop Quiz: Haber Process (N₂ + 3 H₂ ⇌ 2 NH₃)

  • Given: \Delta H^{\circ} = -92.38\ \text{kJ}, \Delta S^{\circ} = -198.3\ \text{J K}^{-1}.

  • Assume these don’t change with temperature.

  • Tasks:

    • a) Predict how \Delta G^{\circ} changes with increasing temperature.

    • b) Compute \Delta G^{\circ} at 25°C (298 K).

    • c) Compute \Delta G^{\circ} at 5000°C (5273 K).

  • Answers (from slides):

    • a) \Delta G^{\circ} becomes more positive or less negative with increasing temperature (i.e., less favorable at higher T).

    • b) \Delta G^{\circ} \approx -33.3\ \text{kJ} (spontaneous at 25°C).

    • c) \Delta G^{\circ} \approx 61\ \text{kJ} (nonspontaneous at 5000°C).

End of Module 1: Thermochemistry

  • This module covers the Second Law, entropy, and Gibbs free energy with qualitative and quantitative frameworks, key equations, and multiple worked examples to illustrate spontaneity and the role of temperature.

  • Real-world relevance includes phase transitions, dissolution, biological entropy questions, and energetic considerations in chemical processes.


Notes on notation and units
  • In several worked examples, standard entropy values were shown with units of kJ mol⁻¹ K⁻¹ in slides, but the conventional unit for standard molar entropies is J mol⁻¹ K⁻¹.

  • Always verify unit consistency when performing computations: convert to a consistent unit before calculating \Delta S or $$\Delta G).