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- W2792992005 endingPage "5364" @default.
- W2792992005 startingPage "5358" @default.
- W2792992005 abstract "It has been proposed, or confirmed, that diamond nanoparticles exist in various environments in space: close to active galactic nuclei, in the vicinity of supernovae and pulsars, in the interior of several planets in the Solar system, in carbon planets and other exoplanets, carbon-rich stars, meteorites, in X-ray active Herbig Ae/Be stars, and in the interstellar medium. Using density functional theory methods we calculate the carbon K-edge X-ray absorption spectrum of two large tetrahedral nanodiamonds: C26H32 and C51H52. We also study and test our methods on the astrophysical molecule CH4, the smallest C-H tetrahedral structure. A possible detection of nanodiamonds from X-ray spectra by future telescopes, such as the project Arcus, is proposed. Simulated spectra of the diffuse interstellar medium using Cyg X-2 as a source show that nanodiamonds studied in this work can be detected by Arcus, a high resolution X-ray spectrometer mission selected by NASA for a Phase A concept study." @default.
- W2792992005 created "2018-03-29" @default.
- W2792992005 creator A5035865269 @default.
- W2792992005 creator A5055724934 @default.
- W2792992005 creator A5059088217 @default.
- W2792992005 date "2018-03-07" @default.
- W2792992005 modified "2023-10-14" @default.
- W2792992005 title "Tetrahedral hydrocarbon nanoparticles in space: X-ray spectra" @default.
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