Unit 1: Atomic Structure

Bohr's Theory and its Limitations

Bohr's model of the atom (1913) was a major step forward, primarily for hydrogen and hydrogen-like ions (e.g., He⁺, Li²⁺).

Key Postulates:

  1. Electrons revolve around the nucleus in fixed, circular paths called orbits or stationary states.
  2. Each orbit has a definite energy. As long as an electron is in an orbit, it does not radiate energy.
  3. The angular momentum of an electron in an orbit is quantized (can only have specific values).
    mvr = n(h / 2π)
    Where 'n' is the principal quantum number (n = 1, 2, 3...), h is Planck's constant.
  4. An electron can jump from a lower energy orbit (n_initial) to a higher energy orbit (n_final) by absorbing energy. It can jump from a higher to a lower orbit by emitting energy. This energy difference is emitted as a photon of light.
    ΔE = E_final - E_initial = hν = hc / λ

Limitations of Bohr's Theory:


Dual Behaviour of Matter and Radiation

de Broglie's Relation

Louis de Broglie (1924) proposed that just as light (radiation) has both wave and particle properties, all moving matter (like electrons) also has wave properties.

He combined Einstein's mass-energy equation (E = mc²) and Planck's quantum equation (E = hν) to derive a relationship for the wavelength (λ) of a particle.

Where: λ is the de Broglie wavelength, h is Planck's constant, p is the momentum, m is the mass, and v is the velocity of the particle.

Significance: This is highly significant for microscopic particles (like electrons), where the wavelength is measurable. For macroscopic objects (like a baseball), the mass (m) is so large that the wavelength (λ) is insignificantly small, making its wave nature undetectable.


Heisenberg Uncertainty Principle

Werner Heisenberg (1927) stated that it is impossible to measure simultaneously and accurately both the position and the momentum (or velocity) of a microscopic particle like an electron.

The act of measuring one quantity (e.g., position) inevitably disturbs the other (e.g., momentum) in an unpredictable way.

Mathematical Form:
(Δx) · (Δp) ≥ h / 4π

Where:

Significance: This principle rules out the possibility of fixed orbits (like in Bohr's model) and introduces the concept of probability and orbitals. We can only talk about the *probability* of finding an electron in a certain region of space, not its exact path.


Hydrogen Atom Spectra

When hydrogen gas is excited in a discharge tube, it emits light. When passed through a prism, this light splits into specific lines (a line emission spectrum). Each line corresponds to an electron falling from a higher energy level (n_final) to a lower one (n_initial).

The wavelength (or wavenumber, ν̄ = 1/λ) of these lines is given by the Rydberg formula:

ν̄ = 1/λ = R_H · [ (1 / n_initial²) - (1 / n_final²) ]

Where R_H is the Rydberg constant (109,677 cm⁻¹).

Spectral Series:

Series Name n_initial n_final Spectral Region
Lyman 1 2, 3, 4, ... Ultraviolet (UV)
Balmer 2 3, 4, 5, ... Visible
Paschen 3 4, 5, 6, ... Infrared (IR)
Brackett 4 5, 6, 7, ... Infrared (IR)
Pfund 5 6, 7, 8, ... Far-Infrared (Far-IR)

Quantum Numbers and Significance

To describe the state of an electron in an atom, we use four quantum numbers, which are solutions to the Schrödinger wave equation.

  1. Principal Quantum Number (n)
    • Allowed values: n = 1, 2, 3, ... (positive integers)
    • Significance: Determines the main energy level (shell) and the average distance of the electron from the nucleus. Higher 'n' = higher energy and larger size. (K shell n=1, L shell n=2, etc.)
  2. Azimuthal Quantum Number (l)
    • Allowed values: l = 0, 1, 2, ... up to (n-1)
    • Significance: Determines the shape of the subshell (orbital). It is also known as the orbital angular momentum quantum number.
      • l = 0 → s subshell (spherical)
      • l = 1 → p subshell (dumbbell)
      • l = 2 → d subshell (double dumbbell)
      • l = 3 → f subshell (complex)
  3. Magnetic Quantum Number (m_l)
    • Allowed values: m_l = -l, ... 0, ... +l (all integers from -l to +l)
    • Significance: Determines the spatial orientation of the orbital. For a given 'l', there are (2l + 1) possible values, meaning (2l + 1) orbitals in that subshell.
      • l=0 (s): m_l=0 (1 s-orbital)
      • l=1 (p): m_l=-1, 0, +1 (3 p-orbitals: p_x, p_y, p_z)
      • l=2 (d): m_l=-2, -1, 0, +1, +2 (5 d-orbitals)
  4. Spin Quantum Number (m_s)
    • Allowed values: +1/2 or -1/2
    • Significance: Describes the intrinsic angular momentum or "spin" of the electron. An electron can spin in one of two directions ("spin up" or "spin down").

Atomic Orbitals

An atomic orbital is a 3D region of space around the nucleus where the probability of finding an electron is maximum (e.g., >90%). The shape of these orbitals is determined by the azimuthal quantum number (l).

Shapes of s, p, and d orbitals


Electronic Configuration of Atoms

This is the distribution of electrons of an atom in its atomic orbitals, governed by three main rules.

1. Aufbau Principle (Building-up Principle)

Electrons fill orbitals starting at the lowest available energy levels before filling higher levels.

Order of filling (Madelung Rule): Electrons fill orbitals in order of increasing (n+l) value. If two orbitals have the same (n+l) value, the one with the lower 'n' value is filled first.

Filling Order: 1s < 2s < 2p < 3s < 3p < 4s < 3d < 4p < 5s < 4d ...

Example: 4s (n+l = 4+0 = 4) is filled before 3d (n+l = 3+2 = 5).

2. Pauli Exclusion Principle

"No two electrons in an atom can have the same set of all four quantum numbers."

This implies that if two electrons are in the same orbital (same n, l, m_l), they must have opposite spins (one +1/2, one -1/2). Therefore, an orbital can hold a maximum of two electrons, and they must be spin-paired.

3. Hund's Rule of Maximum Multiplicity

"For a set of degenerate orbitals (orbitals of the same energy, like the three p-orbitals), pairing of electrons will not occur until each orbital is first singly occupied (half-filled)."

Furthermore, all singly occupied orbitals will have the same spin (parallel spins).

Example: Nitrogen (Z=7)
Configuration: 1s² 2s² 2p³
The 2p orbitals are filled as: [↑] [↑] [↑] (on 2p_x, 2p_y, 2p_z)
NOT as: [↑↓] [↑] [ ]


Stability of Half-filled and Completely-filled Orbitals

Subshells that are exactly half-filled (e.g., p³, d⁵, f⁷) or completely-filled (e.g., p⁶, d¹⁰, f¹⁴) are exceptionally stable.

Reasons for Stability:

  1. Symmetry: A half-filled or completely-filled set of degenerate orbitals has a perfectly symmetrical distribution of electron density, which leads to greater stability.
  2. Exchange Energy: Electrons with the same spin (parallel spins) in degenerate orbitals can exchange their positions. Each such exchange releases energy, called exchange energy. The more parallel spins there are, the greater the exchange energy, and the greater the stability. A half-filled d⁵ subshell (5 parallel spins) has the maximum possible exchange energy.

Anomalous Electronic Configurations:

This stability explains the anomalous configurations of Chromium (Cr) and Copper (Cu).