Chemical Thermodynamics
Table of Contents
- 1. Internal Energy
- 2. Enthalpy
- 3. Helmholtz Free Energy
- 4. Gibbs Free Energy
- 5. Activity
- 6. Activity Coefficient
- 7. Fugacity
- 8. pH
- 9. Equilibrium Constant
- 10. Ionic Strength
- 11. Exchange Energy
- 12. Hard and Soft Acid and Base
- 13. Symmetry-Adapted Linear Combination
- 14. Ligand Field Theory
- 15. References
1. Internal Energy
- \( U \)
The definition depends greatly on the system.
In chemistry, the system is often a bulk of matter. Internal energy represents bonding energy, intermolecular energy, dispersion as well as the kinetic energy of molecules.
Keep in mind the first law of thermodynamics: \[ dU = \delta Q + \delta W, \] and the relation between state functions: \[ dU = TdS - pdV + \sum_i \mu_i dN_i. \]
2. Enthalpy
- \( H := U + pV \)
Chemical reaction is mostly done in isobaric condition in which: \[ dH = \delta Q + Vdp = \delta Q. \]
3. Helmholtz Free Energy
- \( A := U - TS \)
A for Arbeit.
4. Gibbs Free Energy
- \( G := U - TS + pV = H - TS = A + pV \)
5. Activity
Relative activity \( a_i \) of a species \( i \) is defined as: \[ a_i := \exp \left( \frac{\mu_i - \mu_i^{\circleddash}}{RT} \right) \] where \( \mu_i \) is the molar chemical potential of the species \( i \).
Equivalently, \[ \mu_i = \mu_i^{\circleddash} + RT\ln a_i. \]
Activity is indicates the deviation from the standard chemical potential \( \mu_i^{\circleddash} \). In particular, it contains the entropy of mixing: \[ \Delta S_{\rm mix} = -R \sum_i n_i \ln x_i. \] The Gibbs free energy per mole is given under isothermal condition:
\begin{align*} \left(\frac{\partial G}{\partial n_i}\right)_{T, p, N_{j\neq i}} &= \left( \frac{\partial G^{\circleddash}}{\partial n_i} \right)_{T, p, N_{j\neq i}} + \left( \frac{\partial \Delta H_{\rm mix}}{\partial n_i}\right)_{T, p, N_{j\neq i}}- T \left( \frac{\partial \Delta S_{\rm mix}}{\partial n_i} \right)_{T, p, N_{j\neq i}} \\ &= \mu_i^{\circleddash} + RT\ln \gamma_i + RT\ln x_i. \end{align*}The Helmholtz energy change can happen due to the intermolecular interaction which is not present in ideal case. Yes, \( n_i \) dependence of \( x_i \) is properly considered. Try differentiate it.
5.1. Water Activity
\[ a_w := \frac{p}{p^{*}} \] where \( p \) is the partial water vapor pressure in equilibrium with the solution, and \( p^{*} \) is the vapor pressure of pure water at the same temperature.
6. Activity Coefficient
There are different activity coefficients for each intensive quantity of amount.
\[ a_{i} = \gamma_{x,i} x_i = \gamma_{c,i} \frac{c_i}{c^{\circleddash}} \] where \( x_i \) is the mole fraction of the species \( i \), \( c_{i} \) is the molarity, and \( c^{\circleddash} \) is the standard concentration (usually 1 mol/L).
6.1. Extended Debye-Hückel Equation
At room temperature, \[ \log \gamma_c = \frac{-0.51 z^2 \sqrt{\mu}}{1+(\alpha \sqrt{\mu} / 305)} \] where \( z \) is the charge, \( \alpha \) is the size in picometers, and \( \mu \) is the ionic strength in mol/L.
6.2. Pitzer Equations
7. Fugacity
\[ a_i = \frac{f_i}{p^{\circleddash}} \]
8. pH
\[ \mathrm{pH} := - \log a_{\rm H^+}. \]
Yes, this is more exact definition.
9. Equilibrium Constant
For a reaction \[ 0 \to \sum_i\nu_i \mathrm{X}_i, \] the equilibrium constant \( K \) is defined as: \[ K := \prod_i a_i^{\nu_i}. \]
9.1. Acid Dissociation Constant
\[ K_\mathrm{a} := \frac{a_{\mathrm{H}^+} a_{\mathrm{A}^-}}{a_{\mathrm{HA}}}. \]
9.2. Base Association Constant
- Base Hydrolysis Constant
\[ K_\mathrm{b} := \frac{a_{\mathrm{BH}^+}a_{ \mathrm{OH}^-}}{a_{ \mathrm{B}}}. \]
9.3. Solubility Product
\[ K_{\rm sp} := a_{\mathrm{A}^-}a_{\mathrm{B}^+}. \]
Solid is in its standard state, and the activity is by definition one.
9.4. Autoprotolysis Constant
\[ K_{\mathrm{w}} := [\mathrm{H}^+][\mathrm{OH}^-]. \]
\( K_{\mathrm{w}} = 1.01\times 10^{-14}\) at 25.0 ℃.
10. Ionic Strength
\[ \mu := \frac{1}{2}\sum_{\text{species } i} c_iz_i^2 \] where \( c_i \) is the concentration, and \( z_i \) is the charge number.
11. Exchange Energy
For each pair of indistinguishable electrons, the system is stabilized by the amount of exchange energy \( \Pi_e \).
12. Hard and Soft Acid and Base
The absolute hardness \( \eta \) is defined by: \[ \eta := \frac{I - A}{2} \] where \( I \) is the ionization energy, and \( A \) is the electron affinity.
Notice that it is half the gap between HOMO and LUMO, with the center being the absolute electronegativity \( \chi \): \[ \chi := \frac{I + A}{2}. \]
If \( \eta \) is high, it is hard for the electron in the HOMO to "squish", that is, to be in a superposition of excited states and ground state.
13. Symmetry-Adapted Linear Combination
- SALC