Abstract
We calculate the radiative lifetime and energy bandstructure of excitons in semiconducting carbon nanotubes within a tight-binding approach including the electron-hole correlations via the Bethe-Salpeter equation. In the limit of rapid interband thermalization, the radiative decay rate is maximized at intermediate temperatures and decreases at low temperature because the lowest-energy excitons are optically forbidden. The intrinsic phonons cannot scatter excitons between optically active and forbidden bands, so sample-dependent extrinsic effects that break the symmetries can play a central role. We calculate the diameter-dependent energy splittings between singlet and triplet excitons of different symmetries and the resulting dependence of radiative lifetime on temperature and tube diameter.
| Original language | English |
|---|---|
| Pages (from-to) | 2495-2499 |
| Number of pages | 5 |
| Journal | Nano Letters |
| Volume | 5 |
| Issue number | 12 |
| DOIs | |
| State | Published - Dec 2005 |
Fingerprint
Dive into the research topics of 'Radiative lifetime of excitons in carbon nanotubes'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver