Chekulaev M. S.1, Yastrebov S. G.
1
1Ioffe Institute, St. Petersburg, Russia
Email: mchs89@gmail.com
The spectral characteristics of hybtid cluster C73H90 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.
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Дата начала обработки статистических данных - 27 января 2016 г.