An excited molecule is, to classical electrodynamics, an oscillating point dipole. In free space it radiates the power and decays at the rate . Put the same dipole a few hundred nanometres from a glass surface, inside an organic layer on a mirror, or on top of a metal film, and both change: the field it radiates comes back to it, reflected by every interface, and does work on it. This is Purcell's observation applied to a planar structure, and it is the physics of OLED outcoupling, of surface-enhanced fluorescence and of the quenching that kills emission next to a metal. It is computed with the same transfer matrix as a plane-wave spectrum, applied to a different source.
A dipole as a sum of plane waves
The field of a dipole at height above a stack, in a medium of index and wavenumber , can be written as a superposition of plane waves with every in-plane wavenumber , including , for which is imaginary and the wave is evanescent. Each plane wave meets the stack below and returns multiplied by the stack's reflection coefficient or , the quantities the transfer matrix already computes, now evaluated at complex angles. Summing the reflected waves at the dipole's own position gives the reflected field there, and the work it does on the dipole is the change in radiated power. With and , the result for a dipole perpendicular and parallel to the interface is (Chance, Prock and Silbey; Lukosz and Kunz)
An emitter with intrinsic quantum yield also decays non-radiatively inside itself, so its total rate is ; a randomly oriented ensemble averages one perpendicular and two parallel dipoles. The same integrals, with the transmission coefficients in place of , give the power that crosses the stack into the substrate. Everything about the structure enters through and as functions of , which is why a dipole calculation costs little more than an angle-resolved reflectance.
Reading the integrand: where the power goes
The integration variable sorts the dipole's power into channels, and the calculator reports them separately:
- : plane waves that propagate in the dipole's own medium. Part escapes (into air above an OLED, into the objective of a microscope); the rest is reflected and interferes with the direct wave, which makes the rate oscillate with with a period of half a wavelength in the medium. That oscillation is Lukosz and Kunz's curve, and Drexhage's 1970 experiment with europium layers above a silver mirror.
- : evanescent in the emitter's medium but propagating in a denser substrate: light that enters the glass beyond its critical angle and is trapped in the substrate by total internal reflection unless the substrate is thin or textured.
- Discrete values of at which or has a pole: the guided modes of the stack (and the surface plasmon of a metal film), which take power without radiating it. In a lossless structure these are sharp poles on the real axis and PyStratify integrates around them analytically, which is why its guided fraction is exact and not a matter of grid resolution.
- : deeply evanescent waves that reach only a few nanometres. Against an absorbing medium they deposit the dipole's energy directly in it. For a dipole at distance from a metal this term grows like , the quasi-static image-dipole law, with the perpendicular dipole quenched twice as strongly as the parallel one: this is quenching, and it dominates below about 10 nm.
The sum of the four channels is the total rate; the escaping part divided by the total is the outcoupling efficiency of an OLED or the collection efficiency of a single-molecule experiment.
The microcavity effect and OLED design
In a thin-film light-emitting diode the emitter sits in an organic layer a fraction of a wavelength thick, between a metal cathode and a transparent anode on glass. The cathode's reflection coefficient is close to , so the reflected wave returns with a phase set almost entirely by the round-trip distance . At the distance where it returns in phase the dipole radiates more, mostly towards the surface normal; a quarter wave away it radiates less, and what it radiates goes sideways into guided modes. Neyts computed the two numbers an OLED engineer needs as the emitter moves through the layer: the fraction of power that reaches air, and the total rate (the Purcell factor), whose product with the intrinsic quantum yield is the effective yield. Furno and co-workers turned the same integrals into the loss budget of a complete device, with each loss channel (substrate, waveguide, surface plasmon, absorption) against the thickness of every layer, the analysis PyStratify's film emission reproduces.
Two practical rules follow from the integrals. First, the optimum emitter position is not at the antinode of the plane-wave standing wave but slightly closer to the mirror, because the evanescent channels grow monotonically as the emitter approaches it. Second, a thick transparent substrate is a trap: without outcoupling structures roughly half of what leaves the organic layers is lost in it, which is why the coherence and thick substrate section's incoherent treatment matters for devices and why textured surfaces appear in the graded and textured surfaces chapter.
Limits of the model
The emitter is a classical point dipole with a fixed frequency: linewidths, saturation and the modification of the emission spectrum by a strongly dispersive cavity are outside it, though the rates it gives are exactly what a quantum treatment yields for a two-level system at weak coupling. The media are local and the interfaces sharp: at distances below one or two nanometres from a metal, the electron gas's nonlocal response and the atomic structure of the surface change the quenching law, which is why computed rates at contact are a limit rather than a prediction. The calculator refuses an absorbing medium around the emitter (its power would not be defined without a cavity around the point source); a metal electrode is therefore an opaque layer rather than a half-space, which changes nothing in the physics once the layer is thicker than its skin depth.
References
- W. Lukosz and R. E. Kunz, J. Opt. Soc. Am. 67, 1607 (1977), doi:10.1364/JOSA.67.001607
- R. R. Chance, A. Prock and R. Silbey, Adv. Chem. Phys. 37, 1 (1978), doi:10.1002/9780470142561.ch1
- G. W. Ford and W. H. Weber, Phys. Rep. 113, 195 (1984), doi:10.1016/0370-1573(84)90098-X
- W. L. Barnes, J. Mod. Opt. 45, 661 (1998), doi:10.1080/09500349808230614
- K. A. Neyts, J. Opt. Soc. Am. A 15, 962 (1998), doi:10.1364/JOSAA.15.000962
- L. Novotny and B. Hecht, Principles of Nano-Optics, 2nd ed. (Cambridge University Press, 2012), ch. 10, doi:10.1017/CBO9780511794193
- M. Furno, R. Meerheim, S. Hofmann, B. Lüssem and K. Leo, Phys. Rev. B 85, 115205 (2012), doi:10.1103/PhysRevB.85.115205