Abstract:
The spectral characteristics of hybtid cluster Ñ$_{73}$Í$_{90}$ were calculated using the time-dependent Density Functional Theory method. The calculated spectrum demonstrates two maxima: at 5.7 and 3.8 eV, which are close to those in interstellar medium and laboretory experiments.
Keywords:interaction of light with matter, new forms of carbon, interstellar medium, Stone–Wales defect.