The
photophysics of single-wall carbon nanotubes (SWCNTs) is intensively
studied due to their potential application in light harvesting and
optoelectronics. Excited states of SWCNTs form strongly bound electron–hole
pairs, excitons, of which only singlet excitons participate in application
relevant optical transitions. Long-living spin-triplet states hinder
applications, but they emerge as candidates for quantum information
storage. Therefore, knowledge of the triplet exciton energy structure,
in particular in a SWCNT chirality dependent manner, is greatly desired.
We report the observation of light emission from triplet state recombination,
i.e., phosphorescence, for several SWCNT chiralities using a purpose-built
spectrometer. This yields the singlet–triplet gap as a function
of the SWCNT diameter, and it follows predictions based on quantum
confinement effects. Saturation under high microwave power (up to
10 W) irradiation allows the spin-relaxation time for triplet states
to be determined. Our study sensitively discriminates whether the
lowest optically active state is populated from an excited state on
the same nanotube or through Förster exciton energy transfer
from a neighboring nanotube.