Second law of thermodynamics Knowledge-Based Study

Chemistry · Thermochemistry & Thermodynamics · Chemistry · Entropy & Free Energy

Chemistry topic explanations on Second law of thermodynamics.

Study notes

  1. In thermodynamics, the first law establishes the conservation of energy, stating that energy cannot be created or destroyed. However, the first law does not predict the direction in which a process naturally occurs. For example, a drop of ink spontaneously disperses in water, but dispersed ink never spontaneously gathers back into a single drop, even though energy would be conserved in both directions.

    The Second Law of Thermodynamics provides the fundamental criterion for determining whether a physical or chemical process can occur spontaneously. It states that for any spontaneous (irreversible) process, the total entropy of the universe must increase:

    ΔSuniv=ΔSsys+ΔSsurr>0\Delta S_{\text{univ}} = \Delta S_{\text{sys}} + \Delta S_{\text{surr}} > 0

    Key consequences of this statement include:

    • Spontaneous process: ΔSuniv>0\Delta S_{\text{univ}} > 0. The process proceeds naturally without continuous external intervention.
    • Reversible (equilibrium) process: ΔSuniv=0\Delta S_{\text{univ}} = 0. The system and its surroundings are in a state of dynamic balance.
    • Non-spontaneous process: ΔSuniv<0\Delta S_{\text{univ}} < 0. The process cannot occur spontaneously under the specified conditions; rather, the reverse process is spontaneous.

    While the entropy change of the system (ΔSsys\Delta S_{\text{sys}}) can be calculated from standard molar entropy values (S∘S^\circ), determining the direction of spontaneity requires evaluating the entropy change of the surroundings (ΔSsurr\Delta S_{\text{surr}}).

    When a system undergoes a chemical or physical change at constant temperature (TT) and pressure, it exchanges heat (qsys=ΔHsysq_{\text{sys}} = \Delta H_{\text{sys}}) with its surroundings. The heat absorbed by the surroundings is −qsys-q_{\text{sys}}. Therefore, the entropy change of the surroundings is defined quantitatively as:

    ΔSsurr=−ΔHsysT\Delta S_{\text{surr}} = -\frac{\Delta H_{\text{sys}}}{T}

    This relationship highlights two important principles:

    • Exothermic processes (ΔHsys<0\Delta H_{\text{sys}} < 0): Heat flows into the surroundings, causing ΔSsurr>0\Delta S_{\text{surr}} > 0. This positive contribution can drive a reaction spontaneously even if the system becomes more ordered (ΔSsys<0\Delta S_{\text{sys}} < 0), such as the freezing of water below 0 °C.
    • Endothermic processes (ΔHsys>0\Delta H_{\text{sys}} > 0): Heat flows out of the surroundings into the system, causing ΔSsurr<0\Delta S_{\text{surr}} < 0. Such processes can only be spontaneous if the increase in system entropy (ΔSsys>0\Delta S_{\text{sys}} > 0) is large enough to outweigh this negative contribution.
    • Temperature dependence: Transferring a given quantity of heat causes a greater fractional change in entropy at lower temperatures than at higher temperatures, as reflected by TT in the denominator.

    Directly monitoring the entropy of the entire universe is impractical in laboratory conditions. To focus exclusively on state functions of the system, we can substitute the expression for ΔSsurr\Delta S_{\text{surr}} into the second law inequality:

    ΔSuniv=ΔSsys−ΔHsysT>0\Delta S_{\text{univ}} = \Delta S_{\text{sys}} - \frac{\Delta H_{\text{sys}}}{T} > 0

    Multiplying both sides of the inequality by −T-T (recalling that absolute temperature TT in kelvins is always positive, which reverses the inequality sign) gives:

    −TΔSuniv=ΔHsys−TΔSsys<0-T\Delta S_{\text{univ}} = \Delta H_{\text{sys}} - T\Delta S_{\text{sys}} < 0

    The quantity ΔHsys−TΔSsys\Delta H_{\text{sys}} - T\Delta S_{\text{sys}} defines the change in Gibbs free energy (ΔGsys\Delta G_{\text{sys}}) at constant temperature and pressure:

    ΔGsys=−TΔSuniv\Delta G_{\text{sys}} = -T\Delta S_{\text{univ}}

    Because ΔGsys\Delta G_{\text{sys}} has the opposite algebraic sign of ΔSuniv\Delta S_{\text{univ}}, the criteria for spontaneity under constant temperature and pressure translate directly:

    • ΔGsys<0\Delta G_{\text{sys}} < 0: The process is spontaneous in the forward direction (ΔSuniv>0\Delta S_{\text{univ}} > 0).
    • ΔGsys=0\Delta G_{\text{sys}} = 0: The system is at equilibrium (ΔSuniv=0\Delta S_{\text{univ}} = 0).
    • ΔGsys>0\Delta G_{\text{sys}} > 0: The forward process is non-spontaneous; work must be done on the system to drive it (ΔSuniv<0\Delta S_{\text{univ}} < 0).

    Thus, Gibbs free energy provides a convenient, system-focused expression of the Second Law of Thermodynamics.