Introduction to Thermodynamics and Processes

  • Central question: What makes physical processes occur?

    • Examples of processes: melting of ice, a bird singing, clouds raining.

    • Initial hypothesis: Energy changes might explain spontaneity (e.g., exothermic vs. endothermic reactions).

    • Observation: Some exothermic reactions are non-spontaneous and some isothermal reactions are spontaneous. Thus, energy alone is not a sufficient explanation.

Probability and Entropy

  • Gas expansion thought experiment:

    • Scenario: Gas particles in a chamber are on one side; the other side is a vacuum.

    • When a partition is opened, gas spreads into the vacuum.

    • Reason for expansion: Not energetic repulsion, but probability; gas particles are more likely to occupy available space.

  • Definition of Entropy in thermodynamics:

    • Entropy (symbol: s) is associated with the number of configurations of a system.

    • Boltzmann's equation for mathematical representation:
      S=kimesextln(W)S = k imes ext{ln}(W)

    • Where W is the number of ways to achieve a certain configuration, and k is the Boltzmann constant.

    • More distributed gas configurations lead to higher entropy.

  • Relation of entropy change to gas expansion:

    • Expansion increases entropy since gas particles can occupy more positions.

    • Expression for change in entropy, extΔSext{ΔS}, during a gas expansion:
      extΔSextisproportionaltoextlnracVfinalVinitialext{ΔS} ext{ is proportional to } ext{ln} rac{V_{final}}{V_{initial}}

    • This applies to isothermal (constant temperature) gas expansions.

Types of Gas Processes

  • Isothermal Processes: Constant temperature.

  • Isochoric Processes: Constant volume.

  • Isobaric Processes: Constant pressure.

  • Key Insights:

    • In isochoric conditions, heat increases temperature (work done is zero).

    • In isobaric conditions, heat causes both temperature increase and work done due to gas expansion.

Work and Heat Relationship in Isothermal Expansion

  • Isothermal expansion involves applying heat to gas which results in expansion:

    • Heat increases gas volume, doing work against surroundings.

    • In isothermal expansion at zero external pressure, no work is done (free expansion).

    • If expanding against some pressure, the work done by the gas is based on external pressure:
      W=PextexternalimesextΔVW = -P_{ ext{external}} imes ext{ΔV}

    • Work is maximized when expanding against pressure equal to the internal pressure of the gas.

Reversible vs. Free Expansion

  • Free Expansion: Gas expands into a vacuum with zero work; W=0W = 0.

  • Reversible Expansion: Gas expands against an equal opposing pressure at every infinitesimal step.

    • Work done during a reversible expansion defined as:
      W=nRTextlnracVfinalVinitialW = -nRT ext{ln} rac{V_{final}}{V_{initial}}

  • Heat absorbed during isothermal expansion defined as: Q=WQ = -W

    • Where QQ and WW are equal in magnitude but opposite in sign.

Reversible Compression

  • For isothermal compressions, work done is the same in form, W=nRTextlnracVfinalVinitialW = -nRT ext{ln} rac{V_{final}}{V_{initial}}

    • External pressure must be greater than internal pressure to compress.

  • For reversibility, apply infinitesimal pressure adjustments for compression.

  • Heat released during compression is related as inversely:
    Q=WQ = -W

Entropy Change During Isothermal Processes

  • Entropy Change:

    • For isothermal expansions:
      extΔS=racQextrevText{ΔS} = rac{Q_{ ext{rev}}}{T}

    • Analogously applicable to state changes, constant pressure, and volume processes.

Applications of Thermodynamic Principles

  • Example: Melting of ice.

    • Phase transition for ice to water indicates greater entropy for liquid state.

    • Use enthalpy of fusion (Hfusion=6.01extkJ/molH_{fusion} = 6.01 ext{ kJ/mol}) to quantify the entropy change.

    • Equation for entropy during phase change:
      extΔS=racΔHText{ΔS} = rac{ΔH}{T}

    • Calculate entropy change for ice melting at 273 K thus:

    • extΔSmelting=rac6.01imes103extJ/mol273extK=22extJ/molKext{ΔS}_{melting} = rac{6.01 imes 10^3 ext{ J/mol}}{273 ext{ K}} = 22 ext{ J/mol K}

Second Law of Thermodynamics

  • The Second Law states:

    • The total entropy of the universe always increases in a spontaneous process.

    • In a spontaneous process, ΔS_{universe} > 0 .

    • Spontaneity can be affected by surroundings:

    • Exothermic processes gain entropy in surroundings, endothermic processes lose it.

Gibbs Free Energy

  • Definition of Gibbs Free Energy (G):
    G=HTSG = H - TS

  • Relationship to spontaneity:

    • If ΔG < 0 , the process is spontaneous; if ΔG > 0 , non-spontaneous.

    • ΔSextuniverse=racΔGTΔS_{ ext{universe}} = - rac{ΔG}{T}

    • Determine spontaneous behavior based on enthalpy and entropy values.

Summary of Thermodynamic Parameters


  • Table for combinations of ΔHΔH, ΔSΔS, and ΔGΔG to classify processes:

    ΔH

    ΔS

    ΔG

    Spontaneity


    Negative

    Positive

    Negative

    Spontaneous


    Positive

    Negative

    Positive

    Non-spontaneous


    Positive

    Positive

    Depends on Temp

    Spontaneous at High Temp


    Negative

    Negative

    Depends on Temp

    Spontaneous at Low Temp

    Conclusion

    • Entropy is linked to the directionality of time, affecting spontaneity in processes.

    • Importance of understanding thermodynamics for predicting chemical behavior in reactions and processes.