Thermodynamics: Fundamental Equations, Entropy, and Gibbs Free Energy

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Vocabulary practice flashcards covering entropy calculations, cyclic thermodynamic paths, fundamental Gibbs equations, Maxwell relations, Gibbs-Helmholtz equations, and the pressure/temperature dependence of thermodynamic potentials.

29 Terms

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Entropy Change (ΔS\Delta S)

The thermodynamic property defined by ΔS=∫dqrevT\Delta S = \int \frac{\text{d}q_{\text{rev}}}{T}, which must be evaluated along a reversible path between the initial and final states; because entropy is a state function, ΔS\Delta S has the same value for an irreversible path between those same states.

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Constant-Volume Entropy Change of Heating

The entropy change for heating one mole of substance at constant volume, defined as ΔS=∫T1T2CVT dT\Delta S = \int_{T_1}^{T_2} \frac{C_V}{T}\,\text{d}T, which simplifies to ΔS=CVln⁡(T2T1)\Delta S = C_V \ln\left(\frac{T_2}{T_1}\right) when the constant-volume heat capacity CVC_V is independent of temperature.

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Constant-Pressure Entropy Change of Heating

The entropy change for heating one mole of substance at constant pressure, defined as ΔS=∫T1T2CPT dT\Delta S = \int_{T_1}^{T_2} \frac{C_P}{T}\,\text{d}T, where CPC_P is the constant-pressure heat capacity of the substance.

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Phase Change Entropy Change

The entropy change during a phase transition occurring at constant temperature and pressure, expressed as ΔS=ΔHT\Delta S = \frac{\Delta H}{T}, where ΔH\Delta H represents the enthalpy of transition (such as the heat of vaporization).

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Isothermal Entropy Change of an Ideal Gas

The entropy change for an ideal gas transitioning at constant temperature from (P,V,T)(P, V, T) to (P′,V′,T)(P', V', T), given by ΔS=Rln⁡(V′V)=Rln⁡(PP′)\Delta S = R \ln\left(\frac{V'}{V}\right) = R \ln\left(\frac{P}{P'}\right), which is positive whenever the volume increases.

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Path-Dependent Quantities

Thermodynamic quantities such as work (ww) and heat (qq) whose values depend on the pathway taken between states, characterized by non-zero cyclic integrals: ∮Dw≠0\oint D w \neq 0 and ∮Dq≠0\oint D q \neq 0.

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State Function

A thermodynamic property whose change depends only on the initial and final states and whose cyclic integral over any closed path equals zero: ∮dy=0\oint \text{d}y = 0.

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<p>Indicator Diagram</p>

Indicator Diagram

A pressure-volume diagram introduced by James Watt where the area under the trajectory represents the work done by the gas during an expansion or compression.

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Maximum Work Principle

The thermodynamic principle stating that the work performed by a system in an expansion from state A to state B is maximized when carried out reversibly (wrev>wirrevw_{\text{rev}} > w_{\text{irrev}}), because pushing power is wasted when internal pressure exceeds external pressure.

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Isothermal Reversible Expansion Work

The work done by an ideal gas during a reversible expansion at constant temperature, calculated as w=−nRT∫ViVfdVV=−nRTln⁡(VfVi)w = -nRT \int_{V_i}^{V_f} \frac{\text{d}V}{V} = -nRT \ln\left(\frac{V_f}{V_i}\right).

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Mechanical Properties

The macroscopic mechanical variables that define the physical dimensions and force state of a thermodynamic system: pressure (PP) and volume (VV).

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Fundamental Thermodynamic Properties

The core thermodynamic variables directly defined by the fundamental laws of thermodynamics: temperature (TT), internal energy (UU), and entropy (SS).

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Composite Thermodynamic Properties

Properties formulated by combining fundamental and mechanical properties: enthalpy (H=U+PVH = U + PV), Helmholtz free energy (A=U−TSA = U - TS), and Gibbs free energy (G=H−TSG = H - TS).

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Gibbs Equations (Four Fundamental Equations)

The four exact differential expressions for a closed system undergoing a reversible process with P–VP\text{--}V work only: dU=TdS−PdV\text{d}U = T\text{d}S - P\text{d}V, dH=TdS+VdP\text{d}H = T\text{d}S + V\text{d}P, dA=−PdV−SdT\text{d}A = -P\text{d}V - S\text{d}T, and dG=VdP−SdT\text{d}G = V\text{d}P - S\text{d}T.

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Maxwell Relations

(∂T∂V)S=−(∂P∂S)V\left(\frac{\partial T}{\partial V}\right)_S = -\left(\frac{\partial P}{\partial S}\right)_V, (∂T∂P)S=(∂V∂S)P\left(\frac{\partial T}{\partial P}\right)_S = \left(\frac{\partial V}{\partial S}\right)_P, (∂S∂V)T=(∂P∂T)V\left(\frac{\partial S}{\partial V}\right)_T = \left(\frac{\partial P}{\partial T}\right)_V, and −(∂S∂P)T=(∂V∂T)P-\left(\frac{\partial S}{\partial P}\right)_T = \left(\frac{\partial V}{\partial T}\right)_P.

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Constant-Volume Heat Capacity (CVC_V)

The heat capacity defined at constant volume by the partial derivatives CV=(∂U∂T)V=T(∂S∂T)VC_V = \left(\frac{\partial U}{\partial T}\right)_V = T\left(\frac{\partial S}{\partial T}\right)_V.

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Constant-Volume Heat Capacity (CVC_V)

The heat capacity defined at constant volume by the partial derivatives CV=(∂U∂T)V=T(∂S∂T)VC_V = \left(\frac{\partial U}{\partial T}\right)_V = T\left(\frac{\partial S}{\partial T}\right)_V.

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Constant-Pressure Heat Capacity (CPC_P)

The heat capacity defined at constant pressure by the partial derivatives CP=(∂H∂T)P=T(∂S∂T)PC_P = \left(\frac{\partial H}{\partial T}\right)_P = T\left(\frac{\partial S}{\partial T}\right)_P.

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Gibbs-Helmholtz Equation

The thermodynamic relation (∂(G/T)∂T)P=−HT2\left(\frac{\partial (G/T)}{\partial T}\right)_P = -\frac{H}{T^2} (or (∂(ΔG/T)∂(1/T))P=ΔH\left(\frac{\partial (\Delta G/T)}{\partial (1/T)}\right)_P = \Delta H), used to calculate enthalpy changes without calorimetry and to find ΔG\Delta G at varying temperatures.

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<p>Gibbs-Helmholtz Plot</p>

Gibbs-Helmholtz Plot

A graphical representation plotting ΔGT\frac{\Delta G}{T} against 1T\frac{1}{T}, where the slope of the tangent to the curve equals the enthalpy change ΔH\Delta H.

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Temperature Dependence of Gibbs Energy

The thermodynamic relationship (∂G∂T)P=−S\left(\frac{\partial G}{\partial T}\right)_P = -S, which indicates that an increase in temperature decreases the Gibbs free energy when pressure is kept constant.

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Pressure Dependence of Gibbs Energy

The thermodynamic relationship (∂G∂P)T=V\left(\frac{\partial G}{\partial P}\right)_T = V, which indicates that an increase in pressure increases the Gibbs free energy when temperature is kept constant.

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<p>Temperature Dependence of $$G$$ and $$H$$ Plot</p>

Temperature Dependence of GG and HH Plot

A graphical plot of enthalpy HH and Gibbs energy GG versus temperature TT at constant pressure, illustrating that G(0)=H(0)G(0) = H(0), the slope of HH is CPC_P, the slope of GG is −S-S, and the vertical difference equals TSTS.

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Gibbs Energy Pressure Dependence for Incompressible Phases

The relation G2=G1+V(P2−P1)G_2 = G_1 + V(P_2 - P_1), valid for liquids and solids where the volume VV is nearly independent of pressure.

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Gibbs Energy Pressure Dependence for an Ideal Gas

The equation G=G∘+nRTln⁡(PP∘)G = G^\circ + nRT \ln\left(\frac{P}{P^\circ}\right) or ΔG=nRTln⁡(P2P1)\Delta G = nRT \ln\left(\frac{P_2}{P_1}\right), relating Gibbs free energy to pressure relative to a standard state pressure P∘P^\circ.

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Isothermal Free Expansion of an Ideal Gas

An irreversible expansion into a vacuum where w=0w = 0, ΔU=0\Delta U = 0, and q=0q = 0, but all state function changes (ΔH=0\Delta H = 0, ΔS\Delta S, ΔA\Delta A, and ΔG\Delta G) are identical to those of a reversible isothermal expansion between the same initial and final states.

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Gibbs Free Energy Spontaneity Criteria

Spontaneity guidelines governed by ΔG=ΔH−TΔS\Delta G = \Delta H - T\Delta S: a transformation is always spontaneous if ΔH<0\Delta H < 0 and ΔS>0\Delta S > 0, never spontaneous if ΔH>0\Delta H > 0 and ΔS<0\Delta S < 0, and governed by the relative magnitudes of ΔH\Delta H and TΔST\Delta S in other cases.