123109-3
Hu et al.
Appl. Phys. Lett. 90, 123109 ͑2007͒
dence of the spontaneous peak intensity was sublinear with
Ist=I0p.83. The simultaneous superlinear dependence of the
emission intensity and the linewidth narrowing at high
pumping power ͓shown in Fig. 4͑b͔͒ suggests a transition
from spontaneous emission to stimulated emission in the
MOCVD-grown InN nanobelts.
Note here that for lasing in the InN nanobelts, a nanobelt
cavity with effective reflectance on both ends is required.
Though InN nanobelts were not vertically aligned with re-
spect to the substrate, they were grown from the substrate,
which enables good contact between the bottom end and the
substrate. The observation of the lasing behavior from the
InN nanobelts grown on the a-SiNx coated silicon confirmed
the fact that the waveguide structure based on the refractive
index difference at the interface of air ͑nair=1͒/InN ͑nInN
FIG. 4. ͑a͒ Power-dependent PL spectra of InN nanobelts grown on SiN
coated Si substrates recorded at 20 K with excitation intensities of 39, 50,
62, 73, and 75 kW/cm2 for PL spectra ͑I͒, II, III, IV, and ͑V͒, respectively.
The inset shows the integrated intensity under different excitation intensi-
ties. ͑b͒ Linewidth of the emission peak as a function of excitation intensity.
͑c͒ Lasing spectrum obtained at different sites of the same sample as ͑a͒ at
the excitation intensity of 77.5 kW/cm2.
ϳ2.9͒/SiNx ͑nSiN ϳ1.9͒ facilitates better confinement and
x
amplification of the light within the waveguide structure of
air/InN/SiNx for lasing action. This effect may be similar to
the UV lasing action of ZnO nanoneedles grown on SiO2
coated Si substrates, as reported by Lau et al.21
Assuming that the measured lasing modes were resulted
from a Fabry-Pérot cavity, the cavity length ͑L͒ can be de-
termined by L=2/2n⌬, where n is the refractive index and
⌬ is the mode spacing. Taking n=2.9 for InN and ⌬
=7 nm, a cavity length of ϳ60 m is required to sustain the
observed lasing modes. This calculated cavity length falls
well in the range of the length of nanowires measured by
SEM. Figure 4͑c͒ depicts another Fabry-Pérot cavity mode
taken at a different site of the same sample, wherein an av-
erage mode spacing of 11 nm was observed, corresponding
to a cavity length of 41 m. According to a first
thus leading to a lower lasing threshold for longer cavity
length. In the present case, more than one cavity length was
observed, suggesting that lasing takes place from InN nano-
belts of different lengths. This fact also reflects the nonuni-
formity of nanobelt length. Furthermore, as shown in Fig.
4͑a͒, a clear redshift of the gain profile was observed from
39 to 75 kW/cm−2. The redshift of the gain profile could be
induced by the band gap renormalization due to Coulomb
interactions among amplified free carriers at the band edge.
Similar redshift phenomena have been reported in 1D GaN
͑Ref. 23͒ or ZnO ͑Ref. 24͒ nanostructures. Another possibil-
ity of the redshift could be ascribed to the local heating of
the nanowires, as high power densities of continue wave ex-
citation were used in our study.
Nano Science and Technology is gratefully acknowledged.
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This research was financially supported by the Ministry
of Education, Asian Office of Aerospace Research and De-
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