Condensation of carbon in radioactive supernova gas.
Chemistry resulting in the formation of large carbon-bearing molecules and dust in the interior of an expanding supernova was explored, and the equations governing their abundances were solved numerically. Carbon dust condenses from initially gaseous carbon and oxygen atoms because energetic electrons produced by radioactivity in the supernova cause dissociation of the carbon monoxide molecules, which would otherwise form and limit the supply of carbon atoms. The resulting free carbon atoms enable carbon dust to grow faster by carbon association than the rate at which the dust can be destroyed by oxidation. The origin of presolar micrometer-sized carbon solids that are found in meteorites is thereby altered.
Department of Physics and Astronomy, Clemson University, Clemson, SC 29634-1911, USA.
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Clayton
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Liu
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Dalgarno
D055580:Astronomical Phenomena; D001256:Astronomy; D002244:Carbon / Q000737:chemistry*; D002248:Carbon Monoxide / Q000737:chemistry; D019443:Cosmic Dust; D008433:Mathematics; D019110:Meteoroids; D008956:Models, Chemical; D010100:Oxygen / Q000737:chemistry
D019443:Cosmic Dust; D002244:Carbon; D002248:Carbon Monoxide; D010100:Oxygen