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CHM 311: Physical Chemistry I

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CHM 311: Physical Chemistry I

Tác giả
Anderson Marsh
Nhà xuất bản
Lebanon Valley College
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LibreTexts
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EN
Danh mục
Khoa học cơ bản
Mục lục· 150 mục
  1. 01: The Path to Quantum Mechanics
  2. 1.01: Prelude to the Foundations of Quantum Mechanics
  3. 1.02: Blackbody Radiation Cannot Be Explained Classically
  4. 1.03: Quantum Hypothesis Used for Blackbody Radiation Law
  5. 1.04: Photoelectric Effect Explained with Quantum Hypothesis
  6. 1.05: Matter Has Wavelike Properties
  7. 1.06: de Broglie Waves can be Experimentally Observed
  8. 02: Foundations of Quantum Mechanics
  9. 2.01: The Schrodinger Equation
  10. 2.02: The Postulates of Quantum Mechanics
  11. 2.03: The Wavefunction Specifies the State of a System
  12. 2.04: Wavefunctions Have a Probabilistic Interpretation
  13. 2.05: Wavefunctions Must Be Normalized
  14. 2.06: Linear Operators in Quantum Mechanics
  15. 2.07: Quantum Operators Represent Classical Variables
  16. 2.08: The Schrodinger Equation is an Eigenvalue Problem
  17. 2.09: Observable Quantities Must Be Eigenvalues of Quantum Mechanical Operators
  18. 2.10: Eigenfunctions of Operators are Orthogonal
  19. 2.11: The Heisenberg Uncertainty Principle
  20. 2.12: Commuting Operators Allow Infinite Precision
  21. 03: Model Systems in Quantum Mechanics
  22. 3.01: The Energy of a Particle in a Box is Quantized
  23. 3.02: The Free Electron Model
  24. 3.03: The Average Momentum of a Particle in a Box is Zero
  25. 3.04: A Particle in a Three-Dimensional Box
  26. 3.05: Tunneling
  27. 3.06: A Harmonic Oscillator Obeys Hooke's Law
  28. 3.07: The Equation for a Harmonic-Oscillator Model of a Diatomic Molecule Contains the Reduced Mass of the Molecule
  29. 3.08: The Harmonic Oscillator Approximates Molecular Vibrations
  30. 3.09: The Harmonic Oscillator Energy Levels
  31. 3.10: The Harmonic Oscillator Wavefunctions involve Hermite Polynomials
  32. 3.11: Hermite Polynomials are either Even or Odd Functions
  33. 3.12: Spherical Polar Coordinates
  34. 3.13: Potential Energy and the Hamiltonian
  35. 3.14: Solution to the Schrodinger Equation
  36. 3.15: Spherical Harmonics
  37. 3.16: Angular Momentum
  38. 3.17: The Three Components of Angular Momentum Cannot be Measured Simultaneously with Arbitrary Precision
  39. 3.18: Application to the Rotation of Real Molecules
  40. 04: The Hydrogen Atom
  41. 4.01: The Hydrogen Atomic Spectrum
  42. 4.02: The Rydberg Formula and the Hydrogen Atomic Spectrum
  43. 4.03: Bohr's Hydrogen Atom
  44. 4.04: The Schrodinger Equation
  45. 4.05: Other One-Electron Systems
  46. 4.06: The Wavefunctions
  47. 4.07: s-orbitals are Spherically Symmetric
  48. 4.08: Orbital Angular Momentum and the p-Orbitals
  49. 05: Many Electron Atoms
  50. 5.01: The Helium Atom Cannot Be Solved Exactly
  51. 5.02: Atomic and Molecular Calculations are Expressed in Atomic Units
  52. 5.03: The Variational Method Approximation
  53. 5.04: Single-electron Wavefunctions and Basis Functions
  54. 5.05: An Electron has an Intrinsic Spin Angular Momentum
  55. 5.06: Wavefunctions must be Antisymmetric to Interchange of any Two Electrons
  56. 5.07: Antisymmetric Wavefunctions can be Represented by Slater Determinants
  57. 5.08: Electron Configurations The Pauli Exclusion Principle The Aufbau Principle and Slater Determinants
  58. 5.09: The Self-Consistent Field Approximation (Hartree-Fock Method)
  59. 5.10: Hartree-Fock Calculations Give Good Agreement with Experimental Data
  60. 5.11: Term Symbols Gives a Detailed Description of an Electron Configuration
  61. 5.12: The Allowed Values of J - the Total Angular Momentum Quantum Number
  62. 5.13: Hund's Rules Determine the Term Symbols of the Ground Electronic States
  63. 06: Molecular Structure and Bonding
  64. 6.01: The Born-Oppenheimer Approximation
  65. 6.02: The Orbital Approximation and Orbital Configurations
  66. 6.03: Linear Variational Method and the Secular Determinant
  67. 6.04: Trial Functions Can Be Linear Combinations of Functions That Also Contain Variational Parameters
  68. 6.05: The H Prototypical Species
  69. 6.06: The Overlap Integral
  70. 6.07: Chemical Bond Stability
  71. 6.08: Bonding and Antibonding Orbitals
  72. 6.09: A Simple Molecular-Orbital Treatment of H Places Both Electrons in a Bonding Orbital
  73. 6.10: Molecular Orbitals Can Be Ordered According to Their Energies
  74. 6.11: Molecular-Orbital Theory Does not Predict a Stable Diatomic Helium Molecule
  75. 6.12: Electrons Populate Molecular Orbitals According to the Pauli Exclusion Principle
  76. 6.13: Diatomic Molecules of the First and Second Periods
  77. 6.14: Molecular Orbital Theory Predicts that Molecular Oxygen is Paramagnetic
  78. 6.15: Molecular-Orbital Theory Also Applies to Heteronuclear Diatomic Molecules
  79. 6.16: Orbital ionization energies
  80. 6.17: Polar bonds
  81. 6.18: Molecular Term Symbols Describe Electronic States of Molecules
  82. 6.19: Molecular Term Symbols Designate Symmetry
  83. 6.20: The pi-Electron Approximation of Conjugation
  84. 6.21: Butadiene is Stabilized by a Delocalization Energy
  85. 6.22: Benzene and Aromaticity
  86. 07: Group Theory and Symmetry
  87. 7.01: Symmetry Elements and Operations Define the Point Groups
  88. 7.02: Symmetry Operations Define Groups
  89. 7.03: Symmetry Operations as Matrices
  90. 7.04: Molecules can be Represented by Reducible Representations
  91. 7.05: Character Tables Summarize the Properties of a Point Group
  92. 7.06: Characters of Irreducible Representations
  93. 7.07: Molecular Orbitals can be Constructed on the Basis of Symmetry
  94. 7.08: HO
  95. 7.09: The Exploitation of Symmetry Can Help Simplify Numerical Calculations
  96. 08: Statistical Mechanics
  97. 8.01: The Boltzmann Factor is used to Approximate the Fraction of Particles in a Large System
  98. 8.02: The Boltzmann Distribution represents a Thermally Equilibrated Distribution
  99. 8.03: Translational Partition Functions of Monotonic Gases
  100. 8.04: Most Atoms are in the Ground Electronic State
  101. 8.05: Pressure can be Expressed in Terms of the Canonical Partition Function
  102. 8.06: Most Molecules are Rotationally Excited at Ordinary Temperatures
  103. 8.07: Rotational Partition Functions of Diatomic Gases Contain a Symmetry Number
  104. 8.08: Rotational Partition Functions of Polyatomic Molecules Depend on the Sphar of the Molecule
  105. 8.09: Most Molecules are in the Ground Vibrational State
  106. 8.10: Vibrational Partition Functions of Polyatomic Molecules Include the Partition Function for Each Normal Coordinate
  107. 8.11: The Partition Function of Distinguishable Independent Molecules is the Product of the Molecular Partition Functions
  108. 8.12: Partition Functions can be Decomposed into Partition Functions of Each Degree of Freedom
  109. 8.13: The Average Ensemble Energy is Equal to the Observed Energy of a System
  110. 8.14: The Energy of a Diatomic Polyatomic Molecule Can Be Approximated as a Sum of Separate Terms
  111. 8.15: Heat Capacity at Constant Volume is the Change in Internal Energy with Temperature
  112. 8.16: Molar Heat Capacities
  113. 8.17: The Equipartition Principle
  114. 8.18: The Famous Equation of Statistical Thermodynamics is Sk ln W
  115. 8.19: Entropy Can Be Expressed in Terms of a Partition Function
  116. 8.20: The Statistical Definition of Entropy is Analogous to the Thermodynamic Definition
  117. 8.21: Practical Absolute Entropies of Gases Can Be Calculated from Partition Functions
  118. 8.22: Standard Entropies Depend Upon Molecular Mass and Structure
  119. 8.23: Spectroscopic Entropies sometimes disgree with Calorimetric Entropies
  120. 09: Molecular Spectroscopy
  121. 9.01: The Electromagnetic Spectrum
  122. 9.02: Introduction to Spectroscopy
  123. 9.03: Rotation of Linear Molecules
  124. 9.04: Microwave Rotational Spectroscopy
  125. 9.05: The Selection Rule for the Rigid Rotor
  126. 9.06: Rotational Spectra of Polyatomic Molecules
  127. 9.07: The Harmonic Oscillator and Infrared Spectra
  128. 9.08: The Harmonic Oscillator Selection Rule
  129. 9.09: Vibrational Overtones
  130. 9.10: Vibrational Spectroscopy Techniques
  131. 9.11: Rotations Accompany Vibrational Transitions
  132. 9.12: Unequal Spacings in Vibration-Rotation Spectra
  133. 9.13: Unequal Spacings in Pure Rotational Spectra
  134. 9.14: Normal Modes in Polyatomic Molecules
  135. 9.15: Irreducible Representation of Point Groups
  136. 9.16: Group Theory Determines Infrared Activity
  137. 9.17: Raman- Application
  138. 9.18: Raman- Theory
  139. 10: Electronic Spectroscopy
  140. 10.01: Using Atomic Term Symbols to Interpret Atomic Spectra
  141. 10.02: The Dynamics of Transitions can be Modeled by Rate Equations
  142. 10.03: A Two-Level System Cannot Achieve a Population Inversion
  143. 10.04: Population Inversion can be Achieved in a Three-Level System
  144. 10.05: What is Inside a Laser
  145. 10.06: The Helium-Neon Laser
  146. 10.07: Modern Applications of Laser Spectroscopy
  147. 10.08: The Beer-Lambert Law
  148. 10.09: Electronic Spectra Contain Electronic Vibrational and Rotational Information
  149. 10.10: The Franck-Condon Principle
  150. 10.11: Electronically Excited Molecules can Relax by a Number of Processes