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Quantum Chemistry ||  Lect # 9 || Radial Distribution Function || Dr Rizwana thumbnail

Quantum Chemistry || Lect # 9 || Radial Distribution Function || Dr Rizwana

Dr Rizwana Mustafa·
5 min read

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TL;DR

Radial distribution function describes electron probability density as a function of distance r from the nucleus.

Briefing

Radial distribution function (RDF) is framed as a probability map for where an electron is likely to be found around a nucleus: it describes the electron density in a spherical region centered on the proton, plotted against the distance r from the nucleus. In this picture, electrons occupy quantized shells and orbitals, and the RDF peaks in the regions where the electron’s wavefunction has the highest probability density. The lecture emphasizes that at r = 0 (zero distance from the nucleus), the probability of finding the electron is zero, so the RDF curves start from the origin rather than showing any electron density at the center.

As the distance from the nucleus increases, the RDF behavior changes systematically with the principal quantum number n. For a given shell, the electron is most likely to be found at the radius where the RDF reaches its maximum peak—interpreted as the most probable region for that electron’s presence. The lecture links this to energy: low-energy electrons remain in lower-energy orbitals rather than “jumping” into higher-energy states, so the RDF peak for a shell corresponds to the dominant location of that electron’s probability density. When moving from n1 to n2 to n3, the most probable radius shifts outward, and the lecture gives a scaling idea consistent with the Bohr-model trend: the characteristic distance for n2 is about four times that for n1, and for n3 about nine times that for n1.

A key comparative point is that the RDF peak height and the spatial spread both evolve with n and orbital type. For higher n values, the electron’s “sphere” expands outward, meaning the probability distribution spreads over a larger region of space. The lecture also compares orbital angular momentum types (s, p, d, f) in terms of where the maximum probability density tends to appear: the highest probability density is associated with s orbitals, followed by p, then d, then f, in the order described. Even when probability density becomes very small between shells or between energy regions, it does not drop to zero everywhere; instead, the distribution shows structured minima and regions of suppressed likelihood.

That structure is attributed to the wave nature of electrons. The RDF is tied to the electron’s wavefunction: by taking the square of the wavefunction (the lecture describes using the “square of that specific electron” and plotting it versus r), one obtains the probability density that produces peaks, troughs, and nodes. The lecture describes “trough” regions as representing the probability suppression between two energy levels, where the probability of finding the electron is almost zero; these correspond to nodes and anti-nodes in the wave picture. Overall, RDF is presented as a direct, visual way to connect quantum wave behavior—peaks, gaps, and nodes—to the spatial likelihood of electron positions around the nucleus, setting up the next discussion on penetration and screening effects.

Cornell Notes

Radial distribution function (RDF) gives the probability of finding an electron at a distance r from the nucleus, treating the nucleus as the center of a sphere. The RDF is derived from the electron’s wavefunction by using its squared value versus r, producing peaks where probability density is highest and nodes where it is (nearly) zero. At r = 0, the probability is zero, so RDF curves start at the origin. As the principal quantum number n increases (n1 → n2 → n3), the most probable radius moves farther from the nucleus and the electron’s distribution spreads outward, following a Bohr-like scaling trend (about 4× for n2 and 9× for n3 relative to n1). The wave nature also creates troughs between energy regions, interpreted as nodes/anti-nodes where electron presence is strongly suppressed.

What does the radial distribution function measure, and why is it plotted against distance r?

RDF measures the probability density (electron density) of finding an electron at a particular distance r from the nucleus. Because the nucleus sits at the center of a spherical coordinate system, plotting against r shows how likely the electron is to be located in different spherical shells around the proton.

Why does the probability of finding an electron become zero at r = 0?

The lecture highlights a common feature of the RDF curves: at zero distance from the nucleus, the probability is zero. In the wavefunction-based picture, the electron’s probability density does not have support at the exact center, so the RDF starts from the origin.

How do the RDF peaks change when moving from n1 to n2 to n3?

For each shell, the RDF has a maximum peak at the radius where the electron is most likely to be found. As n increases, that peak shifts outward: the characteristic distance for n2 is described as about four times that for n1, and for n3 about nine times that for n1, consistent with the Bohr-model scaling trend.

What does the lecture say about electron probability between shells or energy regions?

Between certain energy regions (for example, between two levels such as k1 and l1), there are areas where the probability of finding the electron is almost zero. These trough regions are tied to the wave nature of the electron and correspond to nodes (and anti-nodes) where the wavefunction’s squared value is strongly suppressed.

How does orbital type (s, p, d, f) relate to where the maximum probability density appears?

The lecture orders the maxima by orbital type: the highest maximum probability density is associated with s, then p, then d, then f. It also notes that while probability can be very small in some regions, it is not everywhere zero because the electron is described as moving in a wave-associated form.

Review Questions

  1. How is RDF constructed from the electron wavefunction, and what does squaring the wavefunction accomplish?
  2. What physical meaning do peaks, troughs, and nodes have in the radial distribution picture?
  3. How does increasing the principal quantum number n affect both the location of the RDF maximum and the spatial spread of electron probability?

Key Points

  1. 1

    Radial distribution function describes electron probability density as a function of distance r from the nucleus.

  2. 2

    RDF curves start at r = 0 because the probability of finding the electron at the nucleus center is zero.

  3. 3

    Each shell (n1, n2, n3, etc.) has a most-probable radius where the RDF reaches a maximum peak.

  4. 4

    Increasing n shifts the RDF maximum outward and expands the spatial spread of the electron distribution, following a Bohr-like scaling trend (about 4× for n2 and 9× for n3 relative to n1).

  5. 5

    Orbital type influences where the maximum probability density occurs, with s highest, then p, then d, then f (as described).

  6. 6

    Wave behavior explains structured minima: troughs between energy regions correspond to nodes/anti-nodes where probability is almost zero.

  7. 7

    Even where probability is strongly suppressed, RDF is not universally zero across all r; it reflects quantized wave patterns rather than a single fixed radius.

Highlights

RDF is presented as a direct probability map: it tells how likely an electron is to be found at each distance from the nucleus.
At r = 0, the probability is zero, so RDF curves begin at the origin.
As n increases, the most probable electron radius moves outward—n2 is described as ~4× and n3 as ~9× the characteristic distance of n1.
Troughs between energy regions are interpreted as nodes where the electron’s probability is almost zero, reflecting the wave nature of electrons.

Topics

  • Radial Distribution Function
  • Electron Probability Density
  • Quantum Shells
  • Wavefunction Nodes
  • Bohr Radius Scaling

Mentioned