Another important contributor to losses is that any energy above and beyond the bandgap energy is lost.
2.
Due to the small dephasing constant used, several excitonic resonances appear well below the bandgap energy.
3.
The bandgap energy at room temperature is 0.75 eV and lies between that of Ge and Si.
4.
As an example, a typical GNR of width of 10 nm has a desirable bandgap energy of 0.4eV.
5.
Any photon with more energy than the bandgap can cause photoexcitation, but any energy above the bandgap energy is lost.
6.
Due to the small dephasing constant used, several excitonic resonances appear ( vertical lines ) well below the bandgap energy.
7.
In this form, one can verify that an unexcited semiconductor shows several excitonic absorption resonances well below the fundamental bandgap energy.
8.
This emission peak often remains well below the fundamental bandgap energy even at the high excitations where all states are continuum states.
9.
Lead-sulfur ( PbS ) dots demonstrated two-electron ejection when the incoming photons had about three times the bandgap energy.
10.
The bandgap energy that determines the energy ( and hence color ) of the fluorescent light is inversely proportional to the square of the size of quantum dot.
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