TY - JOUR
T1 - Dark excitons due to direct Coulomb interactions in silicon quantum dots
AU - Reboredo, F.
AU - Franceschetti, A.
AU - Zunger, A.
PY - 2000
Y1 - 2000
N2 - Electron-hole exchange interactions can lead to spin-forbidden “dark” excitons in direct-gap quantum dots. Here, we explore an alternative mechanism for creating optically forbidden excitons. In a large spherical quantum dot made of a diamond-structure semiconductor, the symmetry of the valence band maximum (VBM) is (Formula presented) The symmetry of the conduction band minimum (CBM) in direct-gap material is (Formula presented) but for indirect-gap systems the symmetry could be (depending on size) (Formula presented) e, or (Formula presented) In the latter cases, the resulting manifold of excitonic states contains several symmetries derived from the symmetries of the VBM and CBM (e.g., (Formula presented) or (Formula presented) Only the (Formula presented) exciton is optically active or “bright,” while the others (Formula presented) E, and (Formula presented) are “dark.” The question is which is lower in energy, the dark or bright. Using pseudopotential calculations of the single-particle states of Si quantum dots and a direct evaluation of the screened electron-hole Coulomb interaction, we find that, when the CBM symmetry is (Formula presented) the direct electron-hole Coulomb interaction lowers the energy of the dark excitons relative to the bright (Formula presented) exciton. Thus, the lowest energy exciton is forbidden, even without an electron-hole exchange interaction. We find that our dark-bright excitonic splitting agrees well with experimental data of Calcott et al., Kovalev et al., and Brongersma et al. Our excitonic transition energies agree well with the recent experiment of Wolkin et al. In addition, and contradicting simplified models, we find that Coulomb correlations are more important for small dots than for intermediate sized ones. We describe the full excitonic spectrum of Si quantum dots by using a many-body expansion that includes both Coulomb and exchange electron hole terms. We present the predicted excitonic spectra.
AB - Electron-hole exchange interactions can lead to spin-forbidden “dark” excitons in direct-gap quantum dots. Here, we explore an alternative mechanism for creating optically forbidden excitons. In a large spherical quantum dot made of a diamond-structure semiconductor, the symmetry of the valence band maximum (VBM) is (Formula presented) The symmetry of the conduction band minimum (CBM) in direct-gap material is (Formula presented) but for indirect-gap systems the symmetry could be (depending on size) (Formula presented) e, or (Formula presented) In the latter cases, the resulting manifold of excitonic states contains several symmetries derived from the symmetries of the VBM and CBM (e.g., (Formula presented) or (Formula presented) Only the (Formula presented) exciton is optically active or “bright,” while the others (Formula presented) E, and (Formula presented) are “dark.” The question is which is lower in energy, the dark or bright. Using pseudopotential calculations of the single-particle states of Si quantum dots and a direct evaluation of the screened electron-hole Coulomb interaction, we find that, when the CBM symmetry is (Formula presented) the direct electron-hole Coulomb interaction lowers the energy of the dark excitons relative to the bright (Formula presented) exciton. Thus, the lowest energy exciton is forbidden, even without an electron-hole exchange interaction. We find that our dark-bright excitonic splitting agrees well with experimental data of Calcott et al., Kovalev et al., and Brongersma et al. Our excitonic transition energies agree well with the recent experiment of Wolkin et al. In addition, and contradicting simplified models, we find that Coulomb correlations are more important for small dots than for intermediate sized ones. We describe the full excitonic spectrum of Si quantum dots by using a many-body expansion that includes both Coulomb and exchange electron hole terms. We present the predicted excitonic spectra.
UR - https://www.scopus.com/pages/publications/0000876587
U2 - 10.1103/PhysRevB.61.13073
DO - 10.1103/PhysRevB.61.13073
M3 - Article
AN - SCOPUS:0000876587
SN - 1098-0121
VL - 61
SP - 13073
EP - 13087
JO - Physical Review B - Condensed Matter and Materials Physics
JF - Physical Review B - Condensed Matter and Materials Physics
IS - 19
ER -