3. Leptons

Learning Outcomes
  • I can identify the members of the lepton family.
  • I can describe the properties of electrons and neutrinos.
  • I can explain the role of leptons in particle interactions.
  • I can compare leptons and quarks.
  • I can explain lepton conservation in simple interactions.

Key Topics:
  • Solutions to the Schrödinger equation for the hydrogen atom
  • Quantization of energy levels and orbitals

Quantum Mechanics and Energy Quantization: Schrödinger’s Equation for the Hydrogen Atom 

Quantum mechanics fundamentally changed our understanding of atomic structure, showing that electrons do not move in fixed orbits but exist in quantized energy levels. Let’s explore how the Schrödinger equation leads to energy quantization in the hydrogen atom and how it defines orbitals! 


1. Schrödinger’s Equation for the Hydrogen Atom

(A) Why Classical Physics Failed

In Bohr’s model, electrons were assumed to orbit the nucleus in circular paths, but:

  • It could not explain multi-electron atoms.
  • It violated classical electromagnetism (orbiting electrons should radiate energy and collapse into the nucleus).

Quantum Mechanics Solution: Electrons exist as probability waves, described by Schrödinger’s equation.


(B) The Time-Independent Schrödinger Equation for Hydrogen

For a single electron in a Coulomb potential (V) due to a proton:

\( - \frac{ \vec{h} }{2m} \)∇2ψ + V(r) = Eψ

where:

  • ψ(r, θ, φ) = wave function (describes electron position)
  • \( V(r) = - \frac{ke^2}{r} \) = Coulomb potential (attraction between electron and proton)
  • ∇2 = Laplacian operator (in spherical coordinates)
  • E = quantized energy levels

Solving this equation gives the allowed energy levels and orbitals!


2. Quantization of Energy Levels 

The allowed energy levels in hydrogen are:

\( E_n = - \frac{13.6eV}{n^2}, n = 1, 2, 3, ... \)

where:

  • n = principal quantum number (labels the energy level)
  • 13.6 eV = ground-state energy of hydrogen

Key Facts:
Energy is quantized → Electrons can only have specific values of En.
Higher n → Larger orbital, lower binding energy (less tightly bound to nucleus).
At n = ∞, E = 0 → The electron is free (ionization).


3. Hydrogen Orbitals: Solutions to Schrödinger’s Equation 

(A) Quantum Numbers and Electron Orbitals

Each solution ψn, l, m is labeled by three quantum numbers:

Principal Quantum Number Ні

  • Determines energy level.
  • n = 1, 2, 3, ...

Azimuthal (Orbital) Quantum Number (l)

  • Determines orbital shape.
  • l = 0, 1, 2, ..., (n - 1)
  • Corresponds to s, p, d, f orbitals.

Magnetic Quantum Number (ml)

  • Determines orbital orientation.
  • ml = -l. ..., 0, ..., +l

Example:
For n = 2: l = 0 (2s) or l = 1 (2p).
For l = 1: ml = -1, 0, +1 (three p-orbitals).


(B) Shapes of Atomic Orbitals

s-Orbitals (l = 0): Spherical, no angular dependence.

p-Orbitals (l = 1): Dumbbell-shaped, oriented along axes.

d-Orbitals (l = 2): More complex shapes, important in transition metals.

Key Idea: Quantum mechanics replaces "orbits" with "orbitals" – regions where electrons are most likely to be found.


4. Worked Example: Hydrogen Energy Levels

Example: Energy of an Electron in the n = 3

 Level

Find the energy of an electron in the third energy level (n = 3) of hydrogen.

Solution:

Using:

\( E_n = - \frac{13.6eV}{n^2} \)

\( E_3 = - \frac{13.6eV}{3^2} \)

E3=−1.51 eVE_3 = -1.51 \text{ eV}

Answer: The energy is -1.51eV, meaning the electron is less tightly bound than in lower levels.

Key Concept: Excited electrons have higher energy and can transition by absorbing/emitting photons.


5. Applications of Quantum Energy Quantization 

  • Spectroscopy  – Atomic emission/absorption lines (e.g., hydrogen’s Balmer series).
  • Lasers & LEDs  – Operate using electron transitions between quantized levels.
  • Quantum Computing  – Uses quantum states in atoms and semiconductors.
  • Astrophysics  – Identifies chemical composition of stars via spectral lines.

Key Fact: All chemical properties depend on quantum energy levels of electrons!


6. Key Takeaways! 

  • Solving Schrödinger’s equation for hydrogen gives quantized energy levels.
  • Electrons exist in orbitals defined by quantum numbers ().
  • Energy levels follow the formula \( E_n = - \frac{13.6eV}{n^2} \).

Quantum mechanics explains atomic spectra, bonding, and chemistry.


7. Want to Try a Challenge? 

Find the energy of an electron in the n = 4 level of hydrogen.
Determine the number of orbitals in the n = 3

 level.

Hint: Use \( E_n = - \frac{13.6eV}{n^2} \) and count allowed (l, ml) values!

Activities:

  • Problem-solving exercises on quantized energy
  • Visualization of atomic orbitals using software

Assessment:

  • Numerical problem set on atomic energy levels