Intermolecular Forces: Van der Waals Radius and London Dispersion (Transcript Notes)

Van der Waals radius and atom size

  • The Van der Waals radius for an atom is one half the distance between atoms at the potential energy minimum. In equation form: R<em>extvdW=frac12d</em>extminR<em>{ ext{vdW}} = frac{1}{2} d</em>{ ext{min}}
  • In the figure discussed, the black arrows show the internuclear distance, and the red arrows show the Van der Waals radii.
  • Example comparison: helium vs xenon. Xenon has 54 electrons; helium has 2 electrons. More electrons mean a larger electron cloud, which contributes to a larger atomic size.

Electron cloud, polarizability, and size trends

  • Electrons are attracted to the nucleus; the farther the electrons are from the nucleus, the weaker the attractive force they feel.
  • When electrons are farther from the nucleus, the electron cloud is easier to distort, i.e., more polarizable.
  • Xenon has electrons farther from the nucleus than helium, making its electron cloud more polarizable and thus more easily distorted ("floppier").

London dispersion forces

  • London dispersion forces arise because instantaneous dipoles occur due to fluctuations in the electron distribution.
  • They are stronger for bigger atoms or molecules because bigger atoms have more electrons and are more polarizable.
  • A larger electron cloud leads to a larger separation of charge during fluctuations, enhancing dispersion forces.
  • London dispersion forces are also stronger for objects with more surface area, because there are more contact regions to interact.
  • Conceptual note: London dispersion forces are one type of intermolecular force (see next section).

Intermolecular vs intramolecular forces

  • Intermolecular forces: forces between molecules (you must have two or more particles to observe an intermolecular force).
  • Prefix inter- means between; related mnemonic: inter means between, as in intermolecular interactions.
  • Contrast with intra- in words like intramural sports, which occur within one campus or set of walls (within a single group).

Practice question 1

  • Question prompt: Compared to helium, the London dispersion forces between xenon atoms are expected to be stronger than those between helium atoms.
  • Answer: Yes — the London dispersion forces between xenon atoms are stronger.
  • Rationale: Xenon has a larger electron cloud (more electrons) than helium, making it more polarizable. Increased polarizability allows for larger instantaneous dipoles and greater fluctuations in charge distribution, which strengthens London dispersion forces.
  • General takeaway: London dispersion forces tend to be stronger for larger atoms or molecules due to more electrons and greater polarizability.

Practice question 2: Melting/boiling points and strength of interactions

  • Core concept: To melt (solid to liquid) or boil (liquid to gas), you must break intermolecular interactions.
  • The amount of energy (heat) required to break those interactions depends on their strength.
  • Prediction: Xenon should have a higher melting and/or boiling point than helium because xenon has stronger intermolecular interactions.
  • Given values: Helium melting point T<em>m(extHe)extaround1 extKT<em>m( ext{He}) ext{ around } 1~ ext{K}; Xenon melting point T</em>m(extXe)extaround161 extKT</em>m( ext{Xe}) ext{ around } 161~ ext{K}.
  • Conclusion: The prediction is correct; xenon’s stronger dispersion forces lead to a much higher melting point relative to helium.

Key numerical references and definitions

  • Electron counts used for illustration: Xenon has 5454 electrons; Helium has 22 electrons.
  • Van der Waals radius definition: R<em>extvdW=frac12d</em>extminR<em>{ ext{vdW}} = frac{1}{2} d</em>{ ext{min}} where dextmind_{ ext{min}} is the internuclear distance at the potential energy minimum.
  • Melting point comparison values cited: T<em>m(extHe)1 KT<em>m( ext{He}) \,\approx\, 1\ \text{K}; T</em>m(extXe)161 KT</em>m( ext{Xe}) \,\approx\, 161\ \text{K}.

Connections to broader concepts and implications

  • Larger electron clouds correlate with greater polarizability, which enhances dispersion forces and affects macroscopic properties like phase transitions (melting/boiling points).
  • Trends in van der Waals radii as atoms get larger will influence predictions of condensation, gas behavior, and interactions in condensed phases.
  • Practical relevance: understanding these forces helps in predicting liquefaction of gases, cryogenics, material design, and interpreting real-world phenomena such as vapor pressures and boiling behaviors.

Summary of core ideas

  • Van der Waals radius is a geometric quantity linked to the distance at the potential energy minimum: R<em>extvdW=frac12d</em>extminR<em>{ ext{vdW}} = frac{1}{2} d</em>{ ext{min}}.
  • Larger atoms (more electrons) have bigger, more polarizable electron clouds, leading to stronger London dispersion forces.
  • London dispersion forces strengthen with increased size and surface area, impacting melting/boiling points and overall intermolecular interactions.
  • Intermolecular forces require two or more particles; intra- refers to forces within a single particle or structure.
  • In the xenon-helium comparisons, xenon’s larger size yields stronger dispersion forces and a much higher melting point compared to helium (approximately 161 K vs 1 K in the given notes).