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• W2333826353 abstract "Nanometer-sized diamond grains are commonly found in primitive chondritic meteorites, but their origin is puzzling. Using evidence from atomistic simulation, we establish a mechanism by which nanodiamonds form abundantly in space in a two-stage process involving condensation of vapor to form carbon onions followed by transformation to nanodiamond in an energetic impact. This nonequilibrium process is consistent with common environments in space and invokes the fewest assumptions of any proposed model. Accordingly, our model can explain nanodiamond formation in both presolar and solar environments. The model provides an attractive framework for understanding noble gas incorporation and explains all key features of meteoritic nanodiamond, including size, shape, and polytype. By understanding the creation of nanodiamonds, new opportunities arise for their exploitation as a powerful astrophysical probe." @default.
• W2333826353 created "2016-06-24" @default.
• W2333826353 creator A5025479661 @default.
• W2333826353 creator A5041750270 @default.
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• W2333826353 date "2012-02-17" @default.
• W2333826353 modified "2023-09-26" @default.
• W2333826353 title "Nonequilibrium Route to Nanodiamond with Astrophysical Implications" @default.
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• W2333826353 doi "https://doi.org/10.1103/physrevlett.108.075503" @default.
• W2333826353 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/22401225" @default.
• W2333826353 hasPublicationYear "2012" @default.
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