Properties of Substances and Mixtures

Intermolecular Forces (IMFs)

  • London Dispersion Forces (LDF):
    • Present in all substances; sole force in nonpolar substances.
    • Temporary dipoles due to random electron motion induce dipoles in neighboring molecules, leading to Coulombic attraction.
    • Increase with greater contact area, more electrons/larger electron cloud, and pi bonding (polarizability).
  • Dipole-Induced Dipole:
    • Occurs between polar and nonpolar molecules.
    • Increases with polarity of the polar molecule and polarizability of the nonpolar molecule.
  • Dipole-Dipole:
    • Occurs between two polar molecules.
    • Strength increases with greater polarity and favorable orientations.
    • Typically stronger than LDF, but data should be checked.
  • Hydrogen Bonding:
    • Strong form of dipole-dipole interaction.
    • Requires a partially positive hydrogen atom attached to N, O, or F on one molecule, attracted to a partially negative N, O, or F on another molecule.
  • Ion-Dipole:
    • Occurs between an ion and a polar molecule.
    • Usually stronger than dipole-dipole interactions.

Properties of Solids

  • Properties depend on the strength and type of IMFs (boiling point (BP), vapor pressure (VP), melting point (MP)).
    • When boiling, all IMFs must be overcome to vaporize a substance.
  • Ionic Solids:
    • Strong interactions between ions result in low VP and high MP/BP.
    • Brittle due to repulsions between like charges.
    • Conduct electricity when ions are mobile (solutions or molten state).
  • Covalent Network Solids:
    • 3D (or 2D for graphite) covalent bonds throughout the structure.
    • Very strong, leading to very high MP/BP.
    • Hard/rigid due to fixed bond angles.
    • Examples: diamond, Buckyball (C60), graphite, SiC, SiO2.
  • Molecular Solids:
    • Individual molecules held together by relatively weak IMFs.
    • High VP and low MP/BP.
    • Do not conduct electricity.
  • Metallic Solids:
    • Metal atoms in a sea of valence electrons.
    • Can form alloys (interstitial and substitutional).
    • Conduct heat and electricity.
  • Biomolecules/Polymers:
    • Large molecules with intramolecular forces affecting shape/properties.

Solids, Liquids, and Gases

  • Solids:
    • Particles in regular, crystalline arrangements or amorphous structures.
    • Limited particle motion; no translational kinetic energy.
    • Structure determined by interparticle attractions.
  • Liquids:
    • Particles close together but able to move and collide.
    • Arrangement and movement depend on polarity, hydrogen bonding, and temperature.
    • Molar volume similar to corresponding solid.
  • Gases:
    • Constant random motion in straight lines until collision.
    • Frequency of collisions depends on volume, pressure, and temperature.
    • Limited IMFs; no definite shape or volume.

Ideal Gas Law

  • Relates pressure (P), volume (V), moles (n), and absolute temperature (T) of a gas: PV = nRT
    • R is the Universal Gas Constant (0.08206 Latm/molK).
  • Combined Gas Law derivation: \frac{PV}{nT} = R = \frac{PV}{nT}
  • Dalton's Law of Partial Pressures: Total pressure is the sum of individual pressures (P = P1 + P2 + P_3…).
    • Application: Gases collected by bubbling through water require accounting for water vapor pressure.
  • Mole Fraction (X):
    • Represents the fraction of the sample (in moles) for one of the gases.
    • Mole fraction * total pressure = pressure of the gas in question.

Kinetic Molecular Theory (KMT)

  • Based on postulates for an IDEAL gas:
    • Gas particle size is negligible compared to the space between particles.
    • Constant random motion with perfectly elastic collisions (energy transferred, not lost).
    • No attractive or repulsive forces between gas particles.
    • Temperature is a measure of average kinetic energy (KE = \frac{1}{2} mv^2).
    • Graham's law: smaller molecules move faster than larger molecules at the same temperature.

Deviation from Ideal Gas Law

  • Real gases deviate from ideal behavior at high pressure or low temperature.
  • Factors causing deviation:
    • Volume of particles: Significant for larger particles, increases the P*V term.
    • Intermolecular Forces: Increase with stronger IMFs, decreases the P*V term.
    • Maxwell-Boltzmann distribution: Describes particle energies at different temperatures.

Solutions and Mixtures

  • Solutions: Homogeneous mixtures where a solute is dissolved in a solvent.
  • Heterogeneous mixtures: Non-uniform composition.
  • Molarity:
    • Common unit for solution concentration: Molarity = \frac{moles \, of \, solute}{Liter \, of \, solution}
    • Ion concentration depends on the ratio of atoms in the formula.

Representations of Solutions

  • Considerations:
    • Whether the solute forms ions or not.
    • Relative sizes, amounts, and orientation of water to ions.
    • Solution concentration and number of particles represented.
    • Changes in volume or states of matter (precipitate or gas formation).
    • Types of IMFs between solute and solvent.

Separation of Solutions and Mixtures

  • Chromatography:
    • Separates components based on differences in IMFs.
    • Types: Paper, Column, and Thin-Layer Chromatography (TLC).
    • Mobile phase (solvent) and stationary phase.
    • Column chromatography: Use for material recovery.
    • R_f \, value = \frac{distance \, traveled \, by \, dye}{distance \, traveled \, by \, solvent}
  • Distillation:
    • Separates mixtures based on differences in boiling points.
    • Repeated boiling and condensation of vapors.

Solubility

  • Miscible: Solute and solvent will mix.
  • Immiscible: Solute and solvent do not mix.
  • Substances with similar IMFs tend to be miscible.
  • Solution formation steps:
    • Solute separation (requires energy).
    • Solvent separation (requires energy).
    • Solvent-solute attraction (releases energy).

Spectroscopy and the Electromagnetic Spectrum

  • Spectroscopy: Study of matter's interaction with electromagnetic radiation.
  • Microwave Rotational Spectroscopy:
    • Microwaves cause molecules to rotate due to interaction with molecular dipole.
  • Infrared (IR) Vibrational Spectroscopy:
    • Measures atomic vibrations, determines functional groups.
  • Ultraviolet-Visible (UV-Vis) Light Spectroscopy:
    • Photons excite electrons to higher energy levels.
    • Energy released as EM radiation during transitions in electronic energy levels.

Properties of Photons

  • Photoelectric Effect:
    • Light shone on a material's surface ejects electrons if energy exceeds binding energy (or shorter wavelength/higher frequency than threshold).
    • Photon absorption/emission changes atom/molecule energy.
  • Photon energy:
    • E = hv
    • h (Planck's constant) = 6.626 \times 10^{-34} m/second
    • v (frequency) in Hertz (1/sec).
    • Electron energy: E = \frac{1}{2} mv^2
  • Combined equations:
    • E = \frac{hc}{\lambda}
    • c (speed of light) = 3.00 \times 10^8 m/sec
    • λ = wavelength (m).

Beer-Lambert Law

  • Relates UV-Vis light absorbance to solution concentration.
  • Increased concentration increases absorbance and decreases % transmittance.
    • A = \epsilon bc
    • A = Absorbance.
    • ε = Molar absorptivity constant.
    • b = path length (usually 1 cm).
    • c = concentration (molarity).
  • Wavelength selection: Choose complementary color for absorbance around 1.