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London Dispersion Forces

Weakest IMF; present in all molecules

  • Caused by temporary electron cloud distortions (instantaneous dipoles)
  • Strength increases with molecular size/polarizability
  • Only IMF for nonpolar molecules (e.g., N2N_2, CH4CH_4)

Dipole-dipole Interactions

Attraction between positive end of one polar molecule and negative end of another

  • Stronger than LDF for similar-sized molecules
  • Only in polar molecules (permanent dipole)
  • Strength depends on magnitude of dipole moment

Ion-dipole Forces

Force between ion and dipole molecule

  • Strongest IMF
  • Important in solutions of ionic compounds (e.g., NaClNaCl in H2OH_2O)
  • Ions attract partial charges on polar molecules

Hydrogen Bonding

Special dipole-dipole interaction when H bonded to N, O, or F

  • Very strong for IMF (but weaker than covalent/ionic bonds)
  • Responsible for unique properties of water
  • Present in H2OH_2O, NH3NH_3, HF, DNA, proteins

Amorphous And Crystalline Solids

Crystalline solids: Highly ordered, repeating structure

  • Sharp melting points
  • Long-range order

Amorphous solids: Disordered, random structure

  • No sharp melting point (soften gradually)
  • Short-range order only

Types Of Crystals: Ionic, Covalent Network, Molecular, Metallic

Crystal TypeParticlesForcesPropertiesExamples
IonicIonsIonicHard, brittle, high MP, conductive when moltenNaCl
Covalent networkAtomsCovalentVery hard, very high MP, poor conductorDiamond, SiO2
MolecularMoleculesIMFVariable MP (generally lower), poor conductorIce, I2
MetallicCations in e- seaMetallicShiny, malleable, conductive, variable MPFe, Cu

States Of Matter And Particle Arrangement

Solid: Fixed shape and volume; particles vibrate in fixed positions Liquid: Fixed volume, variable shape; particles flow past each other Gas: Variable shape and volume; particles move freely, far apart

PV=nRTPV=nRT Application

Ideal gas law: PV=nRTPV = nRT

  • P = pressure (atm)
  • V = volume (L)
  • n = moles
  • R = 0.08206 L - atm/mol - K (ideal gas constant)
  • T = temperature (K)

Applications:

  • Calculate unknown variable when others known
  • Compare two sets of conditions (combined gas law)

Partial Pressure And Dalton's Law

Dalton's Law of Partial Pressures: Ptotal=P1+P2+P3+P_{total} = P_1 + P_2 + P_3 + \cdots

Mole fraction and partial pressure: PA=χA×PtotalP_A = \chi_A \times P_{total}

Maxwell-boltzmann Distributions

Distribution of molecular speeds at a given temperature

  • Peak: most probable speed
  • Average speed: moves right as T increases
  • Curve spreads: wider distribution at higher T

vrms=3RTMv_{rms} = \sqrt{\frac{3RT}{M}}

Real Gases Vs. Ideal Gases

Ideal gas assumptions:

  • No volume occupied by gas particles
  • No intermolecular forces between particles

Real gases deviate at:

  • High pressure (particle volume significant)
  • Low temperature (IMF significant)

van der Waals equation: (P+an2V2)(Vnb)=nRT\left(P + \frac{an^2}{V^2}\right)(V - nb) = nRT

Molarity And Concentration

Molarity (M): M=moles of soluteliters of solutionM = \frac{\text{moles of solute}}{\text{liters of solution}}

Other concentration units:

  • Molality (m) = moles solute / kg solvent
  • Mole fraction (χ\chi) = nA/ntotaln_A / n_{total}
  • ppm = (mass solute / mass solution) × 106

Chromatography And Distillation

Chromatography: Separates based on differential affinity to stationary/mobile phase

  • Paper chromatography
  • Column chromatography
  • Gas chromatography

Distillation: Separates based on boiling point differences

  • Simple distillation (large BP difference)
  • Fractional distillation (small BP difference)

Solubility Rules

Common soluble compounds (exceptions noted):

  • Group 1 ions: all soluble
  • NH4+NH_4^+: all soluble
  • Nitrates (NO3NO_3^-): all soluble
  • Acetates (CH3COOCH_3COO^-): all soluble
  • Cl-, Br-, I-: soluble (except with Ag+, Pb2+, Hg22+)
  • SO42-: soluble (except with Pb2+, Ba2+, Ca2+, Sr2+, Ra2+)

Common insoluble compounds:

  • Carbonates (CO32CO_3^{2-}), phosphates (PO43PO_4^{3-}), sulfides (S2S^{2-}), hydroxides (OHOH^-)

Photons And Electron Emission

Photoelectric effect: Emission of electrons when light shines on metal surface

  • Each photon has energy E=hf=hc/λE = hf = hc/\lambda
  • Electrons emitted only if photon energy > binding energy
  • Kinetic energy of ejected electron: KE=hfΦKE = hf - \Phi (work function)

Absorbance And Concentration

A=εlcA = \varepsilon \cdot l \cdot c

  • A = absorbance (dimensionless)
  • epsilon = molar absorptivity (L/mol - cm)
  • l = path length (cm)
  • c = concentration (mol/L)

Relationship: Absorbance directly proportional to concentration