Thermodynamics - Entropy and Heat Capacities

Heat Capacities and Poison's Ratio of Gases

The heat capacity of a gas depends on its atomicity and molecular structure. For an ideal gas, the molar heat capacity at constant volume is denoted as CvC_v and at constant pressure as CpC_p. The relationship between them is defined by Mayer's formula: CpCv=RC_p - C_v = R. The Poison's Ratio (γ\gamma) is the ratio of these two heat capacities, defined as γ=CpCv\gamma = \frac{C_p}{C_v}.

For Monoatomic gases (such as HeHe, NeNe, and ArAr), the molar heat capacity at constant volume is Cv=32RC_v = \frac{3}{2}R and at constant pressure is Cp=52RC_p = \frac{5}{2}R. This results in a Poison's Ratio of γ=5/2R3/2R1.67\gamma = \frac{5/2 R}{3/2 R} \approx 1.67.

For Diatomic gases (such as O2O_2, N2N_2, and H2H_2) and Linear Polyatomic gases (such as CO2CO_2 and HCNHCN), the molar heat capacity at constant volume is Cv=52RC_v = \frac{5}{2}R and at constant pressure is Cp=72RC_p = \frac{7}{2}R. This results in a Poison's Ratio of γ=7/2R5/2R=1.40\gamma = \frac{7/2 R}{5/2 R} = 1.40.

For Non-linear Polyatomic gases (such as CH4CH_4, H2OH_2O, and NH3NH_3), the molar heat capacity at constant volume is Cv=3RC_v = 3R and at constant pressure is Cp=4RC_p = 4R. This results in a Poison's Ratio of γ=4R3R1.33\gamma = \frac{4R}{3R} \approx 1.33.

Entropy Changes in Temperature and Phase Transformations

The entropy change of a system (ΔSsys\Delta S_{sys}) during a temperature change without a phase transition is calculated using the formula: ΔSsys=nCmlnT2T1\Delta S_{sys} = n C_m \text{ln} \frac{T_2}{T_1}, where nn is the number of moles, CmC_m is the molar heat capacity (either CvC_v or CpC_p depending on the process), and T1T_1 and T2T_2 are the initial and final temperatures in Kelvin. The entropy change of the surroundings (ΔSsurr\Delta S_{surr}) is defined as ΔSsurr=qsysTsurr\Delta S_{surr} = \frac{-q_{sys}}{T_{surr}}. In constant pressure processes, this becomes ΔSsurr=ΔHsysTsurr\Delta S_{surr} = \frac{-\Delta H_{sys}}{T_{surr}}, where ΔHsys=nCp(T2T1)\Delta H_{sys} = n C_p (T_2 - T_1).

Phase transformations occur at constant temperature (the transition temperature, TtransT_{trans}). The entropy change for the system during a phase transition is given by ΔSsys=ΔHtransTtrans\Delta S_{sys} = \frac{\Delta H_{trans}}{T_{trans}}. There are three primary types covered: melting (fusion), boiling (vaporization), and sublimation.

For Melting (Solid to Liquid): ΔSfus=ΔHfusTmp\Delta S_{fus} = \frac{\Delta H_{fus}}{T_{mp}}, where TmpT_{mp} is the melting point temperature.

For Boiling (Liquid to Vapour): ΔSvap=ΔHvapTbp\Delta S_{vap} = \frac{\Delta H_{vap}}{T_{bp}}, where TbpT_{bp} is the boiling point temperature.

For Sublimation (Solid to Vapour): ΔSsub=ΔHsubTsub\Delta S_{sub} = \frac{\Delta H_{sub}}{T_{sub}}, where TsubT_{sub} is the sublimation temperature.

Numerical Examples of Entropy and Phase Change

Example 1: Given that 30.4×103J30.4 \times 10^3 J of heat is required to melt one mole of sodium chloride and the entropy change at the melting point is 28.4JK1mol128.4 J K^{-1} mol^{-1}, find the melting point (TT). Using the formula T=ΔHΔST = \frac{\Delta H}{\Delta S}, we calculate T=30.4×10328.4T = \frac{30.4 \times 10^3}{28.4}. This results in a melting point of approximately 1070K1070 K.

Example 2: Calculate ΔSsys\Delta S_{sys}, ΔSsurr\Delta S_{surr}, and ΔSuniv\Delta S_{univ} for the melting of 2 moles2 \text{ moles} of ice at 0C0^{\circ} C (273K273 K). Given ΔHfus=6.01kJ/mol\Delta H_{fus} = 6.01 kJ/mol. Since the process is at equilibrium at the melting point: ΔSsys=2×6.01×103273J/K\Delta S_{sys} = \frac{2 \times 6.01 \times 10^3}{273} J/K. For a reversible process, ΔSsurr=(2×6.01×103)273J/K\Delta S_{surr} = \frac{-(2 \times 6.01 \times 10^3)}{273} J/K. Thus, ΔSuniv=ΔSsys+ΔSsurr=0\Delta S_{univ} = \Delta S_{sys} + \Delta S_{surr} = 0.

Example 3: If the same 2 moles2 \text{ moles} of ice at 0C0^{\circ} C melt in a bath kept at a constant temperature of 3C3^{\circ} C (276K276 K), the ΔSsys\Delta S_{sys} remains the same: ΔSsys=2×6.01×103273J/K\Delta S_{sys} = \frac{2 \times 6.01 \times 10^3}{273} J/K. However, the surroundings are at a different temperature, so ΔSsurr=(2×6.01×103)276J/K\Delta S_{surr} = \frac{-(2 \times 6.01 \times 10^3)}{276} J/K. In this irreversible case, ΔSuniv=2×6.01×1032732×6.01×103276>0\Delta S_{univ} = \frac{2 \times 6.01 \times 10^3}{273} - \frac{2 \times 6.01 \times 10^3}{276} > 0, indicating a spontaneous process.

Entropy Change for Multi-Step Paths

When a substance undergoes multiple changes (e.g., heating and phase transition), the total entropy change is the sum of individual steps. Consider heating 1 mole1 \text{ mole} of ice from 10C-10^{\circ} C (263K263 K) to steam at 120C120^{\circ} C (393K393 K).

Step 1: Heating ice from 263K263 K to 273K273 K: ΔS1=nCp,iceln273263\Delta S_1 = n C_{p,ice} \text{ln} \frac{273}{263}.

Step 2: Phase transition (fusion) at 273K273 K: ΔS2=nΔHfus273\Delta S_2 = \frac{n \Delta H_{fus}}{273}.

Step 3: Heating water from 273K273 K to 373K373 K: ΔS3=nCp,waterln373273\Delta S_3 = n C_{p,water} \text{ln} \frac{373}{273}.

Step 4: Phase transition (vaporization) at 373K373 K: ΔS4=nΔHvap373\Delta S_4 = \frac{n \Delta H_{vap}}{373}.

Step 5: Heating steam from 373K373 K to 393K393 K: ΔS5=nCp,steamln393373\Delta S_5 = n C_{p,steam} \text{ln} \frac{393}{373}.

The total entropy change of the system is ΔSnet=ΔS1+ΔS2+ΔS3+ΔS4+ΔS5\Delta S_{net} = \Delta S_1 + \Delta S_2 + \Delta S_3 + \Delta S_4 + \Delta S_5. If the surroundings are at a constant temperature of 393K393 K, the total entropy change of the surroundings is calculated by dividing the total heat lost by the surroundings (ΔHnet-\Delta H_{net}) by the temperature of the surroundings (393K393 K).

Entropy Change in Ideal Gas Processes

For an ideal gas undergoing a process, the change in entropy of the system is derived from the First Law (dq=dudwdq = du - dw). Using ΔS=dqrevT\Delta S = \frac{dq_{rev}}{T}, we arrive at the general state function equation: ΔSsys=nCvlnT2T1+nRlnV2V1\Delta S_{sys} = n C_v \text{ln} \frac{T_2}{T_1} + n R \text{ln} \frac{V_2}{V_1}. Alternatively, in terms of pressure: ΔSsys=nCplnT2T1+nRlnP1P2\Delta S_{sys} = n C_p \text{ln} \frac{T_2}{T_1} + n R \text{ln} \frac{P_1}{P_2}.

In an Isothermal Process (T1=T2T_1 = T_2), the temperature factor becomes zero (ln1=0\text{ln} 1 = 0). Therefore, ΔSsys=nRlnV2V1=nRlnP1P2\Delta S_{sys} = n R \text{ln} \frac{V_2}{V_1} = n R \text{ln} \frac{P_1}{P_2}. If the process is reversible, ΔSsurr=ΔSsys\Delta S_{surr} = -\Delta S_{sys} and ΔSuniv=0\Delta S_{univ} = 0. If the process is irreversible, the state function ΔSsys\Delta S_{sys} remains the same, but ΔSsurr=qirrevT\Delta S_{surr} = \frac{-q_{irrev}}{T}, and ΔSuniv>0\Delta S_{univ} > 0.

In an Adiabatic Process, for a reversible path, dqrev=0dq_{rev} = 0, so ΔSsys=0\Delta S_{sys} = 0. This is consistent with the adiabatic relationship T1V1γ1=T2V2γ1T_1 V_1^{\gamma-1} = T_2 V_2^{\gamma-1}, which makes the sum of the temperature and volume terms in the entropy equation zero. For an irreversible adiabatic process, ΔSsurr=0\Delta S_{surr} = 0 because no heat is exchanged, but ΔSsys>0\Delta S_{sys} > 0. Although ΔS\Delta S is a state function and the formula remains the same, the final temperature T2T_2 achieved in an irreversible adiabatic expansion is different from that in a reversible one, leading to a non-zero entropy change.

Advanced Numerical Questions

Question: Calculate the total entropy change for the transition at 368K368 K of 1 mole1 \text{ mole} of sulphur from monoclinic to rhombic solid state, if ΔH=40.17J/mol\Delta H = -40.17 J/mol for this transition and the surroundings is an ice-water bath at 0C0^{\circ} C (273K273 K).

ΔSsys=ΔHTtrans=40.17J/mol368K=0.109JK1mol1\Delta S_{sys} = \frac{\Delta H}{T_{trans}} = \frac{-40.17 J/mol}{368 K} = -0.109 J K^{-1} mol^{-1}. ΔSsurr=ΔHsysTsurr=+40.17273=0.147JK1mol1\Delta S_{surr} = \frac{-\Delta H_{sys}}{T_{surr}} = \frac{+40.17}{273} = 0.147 J K^{-1} mol^{-1}. ΔStotal=ΔSsys+ΔSsurr=0.109+0.147=0.38JK1mol1\Delta S_{total} = \Delta S_{sys} + \Delta S_{surr} = -0.109 + 0.147 = 0.38 J K^{-1} mol^{-1}. The answer is (C).

Question: 1 mole1 \text{ mole} of an ideal gas expands freely from 1L1 L to 2L2 L at 300K300 K into a vacuum. Calculate ΔSuniverse\Delta S_{universe}. In free expansion, w=0w = 0 and q=0q = 0, so TT remains constant. ΔSsys=RlnV2V1=8.314×ln25.76J/K\Delta S_{sys} = R \text{ln} \frac{V_2}{V_1} = 8.314 \times \text{ln} 2 \approx 5.76 J/K. Since qsurr=0q_{surr} = 0, ΔSsurr=0\Delta S_{surr} = 0. Thus, ΔSuniv=5.76J/K\Delta S_{univ} = 5.76 J/K.

Question: 2 moles2 \text{ moles} of an ideal gas (Cv=32RC_v = \frac{3}{2}R) are heated from 300K300 K to 600K600 K and expanded from 10L10 L to 20L20 L. Calculate ΔS\Delta S. ΔS=nCvlnT2T1+nRlnV2V1=2×32Rln600300+2×Rln2010\Delta S = n C_v \text{ln} \frac{T_2}{T_1} + n R \text{ln} \frac{V_2}{V_1} = 2 \times \frac{3}{2} R \text{ln} \frac{600}{300} + 2 \times R \text{ln} \frac{20}{10}. ΔS=3Rln2+2Rln2=5Rln2=5×8.314×0.693×2×0.528.8J/K\Delta S = 3 R \text{ln} 2 + 2 R \text{ln} 2 = 5 R \text{ln} 2 = 5 \times 8.314 \times 0.693 \times 2 \times 0.5 \approx 28.8 J/K.