CHEM 156: Basic Physical Chemistry II - Second and Third Laws of Thermodynamics

Overview of Spontaneous and Nonspontaneous Processes

  • Spontaneous Process:     * Definition: A spontaneous process is one that proceeds of its own accord without any external assistance.     * Spontaneity: Generally, the natural tendency of a process to occur is referred to as its spontaneity.     * Examples provided:         * Heat flow (from hot to cold).         * Gas flow.         * Melting of ice.         * Rusting of iron.

  • Nonspontaneous Process:     * Definition: A process that does not proceed on its own and requires external intervention or energy input.     * Examples provided:         * Charging of a battery.         * Photosynthesis.         * Electrolysis of water.

Characteristics of a Spontaneous Process

  • 1. Unidirectional Process:     * A spontaneous change is a one-way process that occurs naturally in a specific direction.     * To reverse a spontaneous process, external work must be performed, making the reverse direction nonspontaneous.

  • 2. Time Independence:     * Spontaneity is distinct from the rate of reaction; being spontaneous does not necessarily mean a process is fast.     * Spontaneous processes can occur at varying speeds: combustion is very quick, while the rusting of iron is very slow.

  • 3. Driven by Instability (Away from Equilibrium):     * If a system is not currently at equilibrium, it will undergo a spontaneous change toward the state of equilibrium.     * This movement toward equilibrium is inevitable unless there is external interference.

  • 4. Equilibrium as the Final State:     * Once a system reaches equilibrium, no further spontaneous changes will occur if the system remains undisturbed.     * Disrupting this equilibrium requires the application of external energy or work.

  • 5. Relation to Free Energy (ΔG\Delta G) and Enthalpy (ΔH\Delta H):     * Most spontaneous changes are accompanied by a decrease in the free energy of the system (\Delta G < 0).     * A decrease in enthalpy (ΔH\Delta H) often accompanies spontaneous processes, but it is not a requirement.     * Processes can be spontaneous even with an increase in enthalpy if the increase in entropy (ΔS\Delta S) is sufficiently large to ensure that the overall Gibbs free energy remains negative.

Concept of Entropy (SS)

  • Definition:     * Entropy is a thermodynamic state quantity that measures the randomness or disorder of the molecules within a system.     * It can also be defined as the measure of the extent to which energy is dispersed throughout a system.     * Changes or processes that increase randomness or disorder are more likely to occur spontaneously than those that bring about order.

  • Properties of Entropy:     * Entropy is a state function, meaning its value depends only on the initial state (ii) and the final state (ff) of the system.     * The change in entropy is denoted as ΔS\Delta S:         * ΔS=SfSi\Delta S = S_f - S_i     * A process accompanied by an increase in entropy tends to be spontaneous.     * For spontaneous processes: S_f > S_i, therefore ΔS\Delta S is positive (\Delta S > 0).

  • Discussion Point:     * Is entropy an intensive or extensive property of a system? (Extensive properties depend on the amount of matter in a sample; intensive properties do not).

The Second Law of Thermodynamics

  • Core Statement:     * The second law states that whenever a spontaneous process occurs, it is accompanied by an increase in the entropy of the universe.     * The "universe" is defined as the combination of the system and its surroundings.     * ΔSuniv=ΔSsys+ΔSsurr\Delta S_{univ} = \Delta S_{sys} + \Delta S_{surr}

  • Principles of Entropy Change:     * Irreversible Spontaneous Processes: When these occur, the total entropy of the system and the surroundings increases (\Delta S_{univ} > 0).     * Reversible Processes: When a reversible process occurs, the total entropy of the system remains constant (ΔSuniv=0\Delta S_{univ} = 0).     * Concise Statement: The entropy of the universe is constantly increasing.

Consequences of the Second Law of Thermodynamics

  • 1. Irreversibility of Natural Processes:     * Natural processes are one-way (e.g., heat flows from hot to cold spontaneously).     * Entropy prevents the spontaneous "un-mixing" of substances, such as milk from coffee, or the "un-burning" of wood.

  • 2. Limits on Heat-to-Work Conversion:     * Heat cannot be fully converted into useful work. No heat engine can achieve 100%100\% efficiency; some energy is always lost as waste heat.     * This principle limits the efficiency of power plants, turbines, and engines.

  • 3. Tendency Toward Greater Disorder:     * Systems naturally move toward high entropy states. Examples include gases spontaneously expanding to fill a volume and ice melting at room temperature.

  • 4. Direction of Time ("Arrow of Time"):     * The Second Law assigns a direction to time, moving from low entropy (order) to high entropy (disorder). In a thermodynamic sense, time cannot be reversed.

  • 5. Equilibrium as Maximum Entropy:     * Systems evolve toward thermodynamic equilibrium, the state where entropy is maximized and spontaneous change ceases.

  • 6. Work Requirement for Refrigeration:     * Heat does not flow spontaneously from cold to hot. To transfer heat "uphill" (as in air conditioners or refrigerators), external work must be performed.

  • 7. Maintenance of Living Systems:     * Living systems survive by importing energy from their environment to avoid internal disorder/entropy increase.     * Plants import energy via sunlight (photosynthesis), and animals via food.     * This energy is used to maintain order (growth, repair, reproduction, movement).     * Living systems release waste energy (heat) and products (CO2CO_2, etc.) back into the environment, increasing the environment's entropy.

  • 8. Heat Death:     * A theoretical ultimate consequence where the universe reaches maximum entropy and no more work can be performed.

The Third Law of Thermodynamics

  • Temperature Dependence:     * The entropy of a substance varies directly with its temperature.     * As temperature decreases, entropy decreases.

  • Core Statement:     * At absolute zero temperature (0K0\,K), the entropy of a pure crystal is zero.     * Mathematically: S=0S = 0 at T=0KT = 0\,K.

Numerical and Statistical Definitions of Entropy

  • Clausius’ Thermodynamic Formulation (1850-1865):     * In a system not undergoing physical/chemical changes, entropy is constant when there is no heat transfer.     * If heat (qq) flows into a system, entropy increases by qT\frac{q}{T}. If heat flows out, entropy decreases.     * For a reversible change at a fixed temperature (TT):         * ΔS=qrevT\Delta S = \frac{q_{rev}}{T}     * Signs and Interpretation:         * If heat is absorbed (+qrev+q_{rev}), ΔS\Delta S is positive (increase in entropy).         * If heat is evolved (qrev-q_{rev}), ΔS\Delta S is negative (decrease in entropy).     * Units of Entropy:         * Entropy units ('eu'): calK1mol1cal\,K^{-1}\,mol^{-1}.         * Standard SI units: JK1mol1J\,K^{-1}\,mol^{-1}.         * Conversion: 1eu=1calK1mol1=4.184JK1mol11\,eu = 1\,cal\,K^{-1}\,mol^{-1} = 4.184\,J\,K^{-1}\,mol^{-1}.

  • Boltzmann’s Statistical Formulation (1877):     * Entropy is a measure of the statistical disorder related to the number of microstates compatible with a system's energy.     * Formula:         * S=kln(W)S = k \ln(W)         * WW: The number of microstates.         * kk: Boltzmann’s constant (k=1.38×1023J/Kk = 1.38 \times 10^{-23}\,J/K).     * Microstates:         * A microstate is a specific configuration of the locations and energies of all atoms or molecules in a system.         * A system with a higher number of microstates is more disordered (higher entropy) than one with fewer microstates.

Applied Discussions and Calculations

  • Microstate and Entropy Scenarios:     * Valve Opening (Gas Expansion): Upon opening a valve between two containers, the number of available microstates (WW) increases significantly as particles occupy more volume, leading to \Delta S > 0.     * Melting of Ice: Transitioning from solid to liquid increases molecular mobility and randomness (WW increases), therefore \Delta S > 0.     * Freezing of Meat: Transitioning from liquid/flexible state to a solid crystalline structure decreases randomness, therefore \Delta S < 0.     * Hot Tea (Cooling): As heat leaves the system into the surroundings, the entropy of the tea system decreases (\Delta S < 0), though the entropy of the surroundings increases by a larger amount.

  • Standard Entropy (SS^{\circ}):     * Absolute Entropy: The actual amount of entropy a substance has at any temperature above 0K0\,K.     * Standard Entropy (SS^{\circ}): Absolute entropy at 25C25^{\circ}C (298K298\,K) and 1atm1\,atm pressure.     * The entropy of any substance above 0K0\,K is always a positive value.

  • Chemical Reaction Calculations:     * Standard Entropy Change (ΔS\Delta S^{\circ}): Calculated as the sum of standard entropies of products minus the sum of standard entropies of reactants:         * ΔS=S(products)S(reactants)\Delta S^{\circ} = \sum S^{\circ}(\text{products}) - \sum S^{\circ}(\text{reactants})     * Standard Entropy of Formation (ΔSf\Delta S^{\circ}_f): The entropy change for the formation of one mole of a compound from its constituent elements under standard conditions:         * ΔSf=S(compound)S(elements)\Delta S^{\circ}_f = \sum S^{\circ}(\text{compound}) - \sum S^{\circ}(\text{elements})