Hello! In our last lesson, we ventured into the complex world of many-body physics, examining the dramatic breakdown of excitons into an electron-hole plasma at high densities—the Mott transition. We saw that at its core, an exciton is a delicate bound state.
Today, we will return to the low-density limit, where excitons are well-defined entities, and investigate their most fundamental interaction: how they are created by light. This lesson directly addresses the learning outcome: to derive the optical absorption coefficient for excitons using Fermi's golden rule.
By the end of this lesson, you will understand why semiconductors exhibit sharp absorption peaks just below the bandgap energy and how to derive the mathematical expression that describes this spectrum. This is the crucial link between the quantum mechanical theory of excitons and the optical spectroscopy experiments you're conducting in the lab. Our derivation will proceed in three steps:
- Reviewing the quantum mechanical tools for light-matter interaction: Fermi's golden rule and the interaction Hamiltonian.
- Applying these tools to the specific case of creating an exciton from the semiconductor ground state.
- Connecting the calculated transition rate to the macroscopic, measurable quantity of the absorption coefficient.
1. The Quantum Framework for Optical Transitions
From your advanced quantum mechanics course, you'll recall that time-dependent perturbation theory provides the framework for describing how a quantum system responds to an external field, like light. The cornerstone of this framework is Fermi's Golden Rule.
Fermi's Golden Rule
Fermi's Golden Rule gives the transition rate from an initial state with energy to a final state with energy , induced by a weak, oscillating perturbation with frequency . For absorption, the rule is:
This powerful equation contains three key components:
- The Matrix Element : This term determines the "selection rules"—it quantifies how strongly the perturbation couples the initial and final states. If it's zero, the transition is forbidden.
- The Density of States: Implicitly, we sum over all possible final states, which brings in the density of states.
- The Delta Function : This enforces the conservation of energy. The energy of the absorbed photon must precisely match the energy difference between the final and initial states.
The Light-Matter Interaction Hamiltonian
To use Fermi's rule, we need to specify the perturbation . The following reading explains how to derive the interaction Hamiltonian for an electron in an electromagnetic field.
Chapter 3 Optical Transitions in Bulk Semiconductors
To understand how light interacts with electrons in a semiconductor, we start with the full Hamiltonian and identify the perturbation term. This handout from Cornell University provides a clear and concise derivation.
Please read Section 3.3, 'Light-Matter Interaction in Quantum Mechanics' (pages 3-5). Focus on sections 3.3.1 and 3.3.4. Starting from the minimal coupling substitution, you will see how the Hamiltonian is simplified to find the interaction term H'. The key result is that for an electron with charge -e, the perturbation due to a light wave described by vector potential A is H' ≈ (e/m₀)A⋅p.
As the text shows, by using the minimal coupling in the electron's kinetic energy term and taking the weak field limit, the primary interaction term is:
where is the free electron mass. For a monochromatic plane wave, the vector potential is . A crucial simplification is the electric dipole approximation. The wavelength of light ( nm) is vastly larger than the size of an exciton ( nm). Therefore, the spatial variation of the field across the exciton is negligible, and we can set . This simplifies the interaction to:
The matrix element in Fermi's rule becomes proportional to , where is the polarization vector of the light.
2. The Exciton Creation Matrix Element
Now we apply this formalism to our specific process: creating an exciton.
- Initial State : This is the semiconductor ground state, , where the valence band is full and the conduction band is empty. Its energy is .
- Final State : This is the semiconductor containing one exciton, . The exciton state is a coherent superposition of electron-hole pairs, described by a center-of-mass momentum and an envelope function for the relative motion (where represents the set of quantum numbers like ). Its energy is , where is the binding energy relative to the bandgap .
The following reading provides the key steps to evaluate the matrix element for exciton creation.
Physics, Modeling and Design of Nonlinear Electroabsorption ...
This appendix from a PhD thesis neatly outlines the calculation of the optical matrix element for exciton creation. It elegantly shows how the properties of the exciton envelope function determine the absorption strength.
Please read Appendix A, 'Excitonic Absorption in Quantum Wells' (pages 176-179). Focus on the derivation from Eq. (A.7) to Eq. (A.9). This shows how the total matrix element for the two-particle exciton state elegantly simplifies.
Let's summarize the essential logic of the calculation:
- The interaction operator acts on the ground state, promoting an electron from a valence band Bloch state to a conduction band Bloch state .
- The matrix element for this single-particle transition is , where is the momentum matrix element between the Bloch periodic parts. The Kronecker delta enforces that optical transitions are vertical in k-space.
- The full matrix element involves an overlap between this created electron-hole pair and the final exciton state. The dipole approximation () implies that the center-of-mass momentum of the created exciton must be . Only excitons that are nearly stationary can be created by single-photon absorption.
- The final result for the matrix element connecting the ground state to an exciton state is: where is the crystal volume.
This is a beautiful and intuitive result. The strength of optical absorption into a particular exciton state is directly proportional to , the value of the relative motion envelope function at zero separation. In other words, the transition strength depends on the probability of finding the electron and the hole in the same unit cell. This makes perfect sense: to create an electron-hole pair with a single photon, the electron and hole must originate from the same point.
For hydrogen-like s-orbitals, is non-zero, while for states with non-zero angular momentum (), . This immediately gives us a powerful selection rule: in the dipole approximation, only s-like excitons can be created by single-photon absorption.
3. The Excitonic Absorption Coefficient
We are now ready to assemble the final piece: the absorption coefficient . This is defined as the energy absorbed per unit time, per unit volume, divided by the incident energy flux (intensity, ).
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Total Transition Rate (): We sum the rates for all possible final exciton states (with ) per unit volume.
where is the exciton energy.
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Intensity (): The intensity of the light wave is , where is the refractive index. Using , we have , so .
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Putting it all together:
Substitute the matrix element into :Now, we find :
After cancelling terms (, one ), we arrive at the absorption coefficient:
In a real system, scattering and finite lifetimes broaden the sharp delta functions into a lineshape function, typically a Lorentzian with a width . The final, more realistic expression is:
This equation is the central result of our lesson. It predicts that the optical absorption spectrum of a semiconductor will consist of a series of discrete peaks corresponding to the creation of different s-like exciton states () at energies just below the bandgap.

Test your understanding!
For a 3D hydrogenic exciton, the envelope function at the origin for an s-state is given by , where is the exciton Bohr radius and is the principal quantum number.
How does the intensity of the absorption peak for the exciton state compare to the state? Why is the peak always the most prominent in experimental spectra?
Show answer
The absorption coefficient is proportional to . Therefore, the ratio of the peak intensities (integrated absorption) for the and states is:
The intensity of the peak is only 1/8th that of the peak. In general, the peak intensity scales as . This is why the ground state exciton peak is by far the strongest and most easily observed feature in the absorption spectrum. The higher-energy states are progressively weaker and eventually merge into the continuum.
Conclusion
In this lesson, we have built a bridge from fundamental quantum mechanics to a key experimental observable in semiconductor physics.
Key Takeaways:
- The absorption of light to create an exciton is governed by Fermi's Golden Rule.
- The strength of the transition is determined by a matrix element , which simplifies under the dipole approximation.
- The transition strength is directly proportional to , the probability of finding the electron and hole at the same position. This leads to the selection rule that only s-like excitons are optically active in single-photon absorption.
- The final expression for the absorption coefficient, , predicts a Rydberg-like series of discrete peaks just below the bandgap, with intensities decreasing as for the states.
Preview of the Next Lesson
We have successfully derived the absorption coefficient. The expression we found contains a collection of fundamental constants and two key physical quantities: the interband momentum matrix element and the envelope function term . It is common practice to group these terms into a single, convenient parameter called the oscillator strength. In our next lesson, we will formally define and evaluate the oscillator strength for exciton transitions, providing a quantitative measure of how "strong" an optical transition is. This will be our next step in fully characterizing the optical properties of excitons.