Direct Observation of Dark Excitons in Individual Carbon Nanotubes: Role of Local Environments
| dc.creator | Srivastava, A. | |
| dc.creator | Htoon, H. | |
| dc.creator | Klimov, V. I. | |
| dc.creator | Kono, J. | |
| dc.date | 2008-04-05 | |
| dc.date.accessioned | 2026-07-07T09:57:25Z | |
| dc.date.available | 2026-07-07T09:57:25Z | |
| dc.description | We report the direct observation of the spin-singlet dark excitonic state in individual single-walled carbon nanotubes through low-temperature micro-photoluminescence spectroscopy in magnetic fields. A magnetic field up to 5 T, applied along the nanotube axis, brightened the dark state, leading to the emergence of a new emission peak. The peak rapidly grew in intensity with increasing field at the expense of the originally-dominant bright exciton peak and finally became dominant at fields $>$3 T. This behavior, universally observed for more than 50 nanotubes of different chiralities, can be quantitatively explained through a model incorporating the Aharonov-Bohm effect and intervalley Coulomb mixing, unambiguously proving the existence of dark excitons. The directly measured dark-bright splitting values were 1-4 meV for tube diameters 1.0-1.3 nm. Scatter in the splitting value emphasizes the role of the local environment surrounding a nanotube in determining the excitonic fine structure of single-walled carbon nanotubes. | |
| dc.description | 4 pages, 4 figures | |
| dc.identifier | https://arxiv.org/abs/0804.0875 | |
| dc.identifier | http://arxiv.org/abs/0804.0875 | |
| dc.identifier | Physical Review Letters 101, 087402 (2008) | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/167335 | |
| dc.subject | Mesoscale and Nanoscale Physics | |
| dc.subject | Materials Science | |
| dc.title | Direct Observation of Dark Excitons in Individual Carbon Nanotubes: Role of Local Environments | |
| dc.type | text |