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Nuclear reactions in shock wave front during supernova eventsThe new unique isotopic anomalous coponent of Xe(XeX) was found in the carbonaceous chondrites. It is enriched in light shielded isotopes (124Xe and 126Xe) and in heavy nonshielded isotopes (134Xe and 136Xe. All characteristics of Xe-X can be explained by a model of nucleosynthesis of the Xe isotopes in shock wave front passed through the He envelope during supernova events. The light isotopes are created by p process and the heavy isotopes are created by n process (slow r process). They were captured with high temperature carbon grains condensing by supernova shock waves.
Document ID
19850026602
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lavrukhina, A. K.
(Academy of Sciences (USSR) Moscow, Ussr)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 3
Subject Category
Space Radiation
Report/Patent Number
OG-8.2-19
Accession Number
85N34915
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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