If you consider a quantum well (QW), what is the minimum energy barrier (difference between quantum well level and embedding layer bands) to effectively have the carriers two-dimensionally confined inside the QW, thus making it possible to detect 2D levels by optical techniques? Is the thermal energy KbT the only energy value to compare this energy barrier with (so at 10 K any barrier above 1 meV is enough)? Should I consider energy barriers only for separated carriers (e.g. only for electrons or holes) or should I consider the two carriers correlated?
To make things more clear: I have done calculation for confined levels into a QW solving the Schrodinger equation and I have found that QW levels are very close to band edges of embedding layers. Now I need to know if I should expect to see these levels by optical investigation (PL, PLE, PR) or if their energy difference is too low to have carriers recombine from 2D levels. From the model I can also get the wavefunction for confined carriers, but I still have not a clear picture what fraction of the carrier wavefunction should be in the QW for to detect it optically.