In-Depth Notes on Light-Matter Interaction
Basics of Light-Matter Interaction
Introduction to Light-Matter Interaction
- Focus on photons and their interaction with materials.
- Presentation based on a pre-print from "Optical Nanospectroscopy" by C. Höppener et al.
Planck's Contribution to Thermal Radiation
- Max Planck (1858-1947) proposed a model to explain the spectrum of thermal radiation.
- Key observations:
- A material emits a broad spectrum of electromagnetic radiation at temperature T.
- Intensity increases with temperature, shifting maximum spectral intensity towards shorter wavelengths (visible light).
- Planck regarded energy exchanges as discrete (photons) with energy ΔEi = ħωi, leading to the concept of Planck's constant, h ≈ 6.626 × 10^-34 J·s.
Standing Waves in a Cavity
- Consider a one-dimensional cavity with two mirrors separated by distance L:
- Standing waves are formed, characterized by intensity maxima in the cavity.
- The resonance condition states that wavelengths fit such that L = n(λ/2) where n is a positive integer.
- For three-dimensional cavities:
- Define wave numbers kn, leading to equations for three dimensions:
- k1 = (π/L)·n1
- k2 = (π/L)·n2
- k3 = (π/L)·n3
- Resulting wavelengths relationship: λn = 2L/n.
Spectral Mode Density and Energy Density
- Spectral mode density n(ω) determines the number of modes at a frequency ω:
- In a cubic resonator, N(ω < ωm) is computed based on k-space geometry.
- Use the equation:
- n(ω < ωm) = (1/3)(ωm^3) / (π^2c^3).
- Average energy per mode at thermal equilibrium:
- Following Planck’s law leading to the black-body radiation law, given by: ρ(ω, T) = n(ω)·W(T, ω).
Einstein Coefficients and Photon Interaction
- Transition types:
- Absorption: Photon excites electron, transferring energy matching the resonance condition (E2 - E1 = ħω).
- Stimulated Emission: Excited electron returns to lower energy state, emitting a photon.
- Spontaneous Emission: Photon emission without external trigger.
- Coefficients:
- Transition probabilities => P12, P21, spontaneous decay A21.
- Relate Einstein coefficients B12, B21 through these probabilities.
Rate Equations for Two-Level Systems
- For a two-level system interacting with a light field:
- Change in populations of excited/ground states modeled using N1 and N2.
- Deduces the population ratio: N1/N2 ties back to Boltzmann distribution.
- Steady-state leads to a definitive equation that equates probabilities, revealing dependence on photon density.
Semiclassical Approach to Light-Matter Interaction
- Combines classical electrodynamics and quantum mechanics for a two-level atom excited by light.
- Governs behavior when light interacts classically with atomic wave functions under specific conditions:
- Time evolution is dictated by Schrödinger’s equation modified for the interaction with a light wave.
- Introduction of Rabi oscillations reflects state transitions depending on interaction strength and frequency.
Interband Transitions in Solids
- In solids, interactions between valence and conduction bands:
- Absorption from lower states populates higher states, generating electron-hole pairs (related to the band gap energy).
- Reverse processes lead to emission (luminescence).
Excitons and Phonons
- Excitons: Bound states of electrons and holes (Frenkel excitons and Wannier-Mott excitons).
- Charge transfer excitons result from intermolecular interactions.
- Phonons: Lattice vibrations; energy carriers in solids and interact with electons.
Plasmons and Nanoparticle Optics
- Describe localized surface plasmon resonances (LSPRs) in nanoparticles:
- Relate to free carriers oscillating under electromagnetic fields, with properties influenced by particle size and surrounding medium.
- Applications extend to sensing and photothermal therapy.
Conclusion
- The principles outlined are foundational for understanding nanotechnology and quantum optics.
- Theoretical developments and experimental validations of these models continue to shape technological advances in science and engineering.