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Coherent effects in semiconductor optics

Photoexciation and similar effects

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Through Coherence (physics), Electromagnetic radiation and Electric field

This article focusses on coherent optical effects in semiconductors and semiconductor nanostructures. After an introduction into the basic principles, the semiconductor Bloch equations (abbreviated as SBEs) which are able to theoretically describe coherent semiconductor optics on the basis of a fully microscopic many-body quantum theory are introduced. Then, a few prominent examples for coherent effects in semiconductor optics are described all of which can be understood theoretically on the basis of the SBEs.

Starting point

Macroscopically, Maxwell's equations show that in the absence of free charges and currents an electromagnetic field interacts with matter via the optical polarization P. The wave equation for the electric field E reads (∇⋅∇−1c2∂2∂t2)E(r,t)=μ0∂2∂t2P(r,t) and shows that the second derivative with respect to time of P, i.e., ∂2∂t2P, appears as a source term in the wave equation for the electric field E. Thus, for optically thin samples and measurements performed in the far-field, i.e., at distances significantly exceeding the optical wavelength λ, the emitted electric field resulting from the polarization is proportional to its second time derivative, i.e., E∝∂2∂t2P. Therefore, measuring the dynamics of the emitted field E(t) provides direct information on the temporal evolution of the optical material polarization P(t).

Microscopically, the optical polarization arises from quantum mechanical transitions between different states of the material system. For the case of semiconductors, electromagnetic radiation with optical frequencies is able to move electrons from the valence (v) to the conduction (c) band. The macroscopic polarization P is computed by summing over all microscopic transition dipoles pcv via P=1V∑c,v(dcvpcv+c.c.), where dcv is the dipole matrix element which determines the strength of individual transitions between the states v and c, c.c. denotes the complex conjugate, and V is the appropriately chosen system's volume. If ϵc and ϵv are the energies of the conduction and valence band states, their dynamic quantum mechanical evolution is according to the Schrödinger equation given by phase factors e−iϵct/ℏ and e−iϵvt/ℏ, respectively. The superposition state described by pcv is evolving in time according to e−i(ϵc−ϵv)t/ℏ. Assuming that we start at t=0 with pcv(t=0)=pcv,0, we have for the optical polarization

P(t)=∑c,v(dcvpcv,0e−i(ϵc−ϵv)t/ℏ+c.c.).

Thus, P(t) is given by a summation over the microscopic transition dipoles which all oscillate with frequencies corresponding to the energy differences between the involved quantum states. Clearly, the optical polarization P(t) is a coherent quantity which is characterized by an amplitude and a phase. Depending on the phase relationships of the microscopic transition dipoles, one may obtain constructive or destructive interference, in which the microscopic dipoles are in or out of phase, respectively, and temporal interference phenomena like quantum beats, in which the modulus of P(t) varies as function of time.

Ignoring many-body effects and the coupling to other quasi particles and to reservoirs, the dynamics of photoexcited two-level systems can be described by a set of two equations, the so-called optical Bloch equations. These equations are named after Felix Bloch who formulated them in order to analyze the dynamics of spin systems in nuclear magnetic resonance. The two-level Bloch equations read

iℏ∂∂tpcv=Δϵpcv+E⋅dI

and

iℏ∂∂tI=2E⋅d(pcv−pcv⋆).

Here, Δϵ=(ϵc−ϵv) denotes the energy difference between the two states and I is the inversion, i.e., the difference in the occupations of the upper and the lower states. The electric field E couples the microscopic polarization p to the product of the Rabi energy E⋅d and the inversion I. In the absence of the driving electric field, i.e., for E=0, the Bloch equation for p describes an oscillation, i.e., pcv(t)∝e−iΔϵt/ℏ.

The optical Bloch equations enable a transparent analysis of several nonlinear optical experiments. They are, however, only well suited for systems with optical transitions between isolated levels in which many-body interactions are of minor importance as is sometimes the case in atoms or small molecules. In solid state systems, such as semiconductors and semiconductor nanostructures, an adequate description of the many-body Coulomb interaction and the coupling to additional degrees of freedom is essential and thus the optical Bloch equations are not applicable.

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