BackGeneral Chemistry Study Notes: Thermochemistry, Quantum Mechanics, Periodic Properties, Gases, Bonding, Intermolecular Forces, and Solutions
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Chapter 6 – Gases
Properties of Gases
Gases are one of the fundamental states of matter, characterized by their ability to expand and fill any container, compressibility, and low density. The behavior of gases can be described by several physical laws and properties.
Expand to fill container
Compressible
Low density
Negligible intermolecular forces (ideal gas assumption)
Pressure
Pressure (P): Force per unit area.
Atmospheric pressure at sea level: 1 atm = 101,325 Pa = 760 mmHg = 760 torr
Manometers and barometers are used to measure gas pressure.
Gas Laws
Boyle's Law: (at constant T, n)
Charles's Law: (at constant P, n)
Avogadro's Law: (at constant P, T)
Ideal Gas Law:
Dalton's Law of Partial Pressures
Total pressure of a mixture of gases equals the sum of the partial pressures of each gas:
Real Gases
Deviate from ideal behavior at high pressures and low temperatures.
Van der Waals Equation:
Graham's Law of Effusion
Rate of effusion is inversely proportional to the square root of molar mass:
Chapter 7 – Thermochemistry
Energy, Heat, and Work
Thermochemistry studies the energy changes that accompany chemical reactions and physical changes.
Temperature: Average kinetic energy of particles in a system.
Heat (q): Energy transferred due to temperature difference.
Work (w): Energy used to move an object against a force.
Kinetic Energy (KE):
Calorie (cal):
First Law of Thermodynamics
Energy is conserved:
Enthalpy (H)
At constant pressure:
Enthalpy change for a reaction:
Calorimetry
Measures heat flow in a reaction.
q = mC\Delta T (C = specific heat capacity)
Hess's Law
If a reaction is carried out in a series of steps, the enthalpy change for the overall reaction is the sum of the enthalpy changes for the individual steps.
Chapter 8 – The Quantum-Mechanical Model of the Atom
Wave Properties of Light
Wavelength (λ): Distance between peaks (measured in meters).
Frequency (ν): Number of waves per second (Hz).
Speed of light (c): m/s
Electromagnetic Spectrum
Visible light: 400–750 nm (Violet to Red)
Photoelectric Effect
Light can eject electrons from a metal surface if above a threshold frequency.
Energy of a photon:
Planck's constant: J·s
Atomic Orbitals and Quantum Numbers
Orbitals are regions of probability for finding electrons.
Heisenberg Uncertainty Principle:
Quantum numbers describe the size, shape, and orientation of orbitals.
Electron Configuration Rules
Aufbau Principle: Fill lowest energy orbitals first.
Pauli Exclusion Principle: No two electrons in an atom can have the same set of quantum numbers.
Hund's Rule: Fill degenerate orbitals singly before pairing.
Chapter 9 – Periodic Properties of the Elements
Effective Nuclear Charge (Zeff)
The net positive charge experienced by valence electrons.
Increases across a period, slightly increases down a group.
Electron Shielding
Core electrons shield valence electrons from the full nuclear charge.
Atomic Radius
Decreases across a period, increases down a group.
Ionization Energy
Energy required to remove an electron from an atom.
Increases across a period, decreases down a group.
Electron Affinity
Energy change when an atom gains an electron.
Electronegativity
Ability of an atom to attract electrons in a bond.
Highest in fluorine.
Chapters 10/11 – Chemical Bonding I & II: The Lewis Model, VSEPR, and MO Theory
Chemical Bonds
Ionic Bonds: Transfer of electrons from metal to nonmetal.
Covalent Bonds: Sharing of electrons between nonmetals.
Polar Covalent Bonds: Unequal sharing of electrons.
Lewis Structures
Show arrangement of valence electrons.
Octet rule: Atoms tend to have eight electrons in their valence shell.
VSEPR Theory
Predicts molecular shapes based on electron pair repulsion.
Bond Polarity and Electronegativity
Difference in electronegativity determines bond type:
Bond Type
Electronegativity Difference
Nonpolar Covalent
0 – 0.4
Polar Covalent
0.4 – 1.7
Ionic
1.7 – 3.3
Bond Energy and Length
Multiple bonds are shorter and stronger than single bonds.
Hybridization
Atomic orbitals mix to form hybrid orbitals (e.g., sp, sp2, sp3).
Chapter 12 – Liquids, Solids, and Intermolecular Forces
Intermolecular Forces
Forces between molecules, weaker than chemical bonds.
Types:
Dispersion (London) forces
Dipole-dipole interactions
Hydrogen bonding (special dipole-dipole, H with N, O, or F)
Ion-dipole forces
Properties of Liquids
Surface Tension: Energy required to increase the surface area of a liquid.
Viscosity: Resistance to flow.
Phase Changes
Melting, freezing, vaporization, condensation, sublimation, deposition.
Energy changes accompany phase transitions.
Heating Curves and Phase Diagrams
Show temperature changes and phase transitions as heat is added or removed.
Chapter 13 – Solutions and Solution Properties
Beer’s Law
Relates absorbance to concentration:
= absorbance, = molar absorptivity, = path length, = concentration
Solution Preparation and Measurement
Proper wavelength selection is crucial for accurate absorbance measurements.
Calibration curves are used to determine unknown concentrations.
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