Despite recent advances,
the synthesis of colloidal InSb quantum
dots (QDs) remains underdeveloped, mostly due to the lack of suitable
precursors. In this work, we use Lewis acid–base interactions
between Sb(III) and In(III) species formed at room temperature
in situ
from commercially available compounds (
viz.
, InCl
3
, Sb[NMe
2
]
3
and a primary
alkylamine) to obtain InSb adduct complexes. These complexes are successfully
used as precursors for the synthesis of colloidal InSb QDs ranging
from 2.8 to 18.2 nm in diameter by fast coreduction at sufficiently
high temperatures (≥230 °C). Our findings allow us to
propose a formation mechanism for the QDs synthesized in our work,
which is based on a nonclassical nucleation event, followed by aggregative
growth. This yields ensembles with multimodal size distributions,
which can be fractionated in subensembles with relatively narrow polydispersity
by postsynthetic size fractionation. InSb QDs with diameters below
7.0 nm have the zinc blende crystal structure, while ensembles of
larger QDs (≥10 nm) consist of a mixture of wurtzite and zinc
blende QDs. The QDs exhibit photoluminescence with small Stokes shifts
and short radiative lifetimes, implying that the emission is due to
band-edge recombination and that the direct nature of the bandgap
of bulk InSb is preserved in InSb QDs. Finally, we constructed a sizing
curve correlating the peak position of the lowest energy absorption
transition with the QD diameters, which shows that the band gap of
colloidal InSb QDs increases with size reduction following a 1/
d
dependence.