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SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE 32 Si IN SUPERNOVAE

Pignatari, M.; Zinner, E.; Bertolli, M. G.; Trappitsch, R.; Hoppe, P.; Rauscher, T.; Fryer, C.; Herwig, F.; Hirschi, R.; Timmes, F. X.; Thielemann, F.-K.

Authors

M. Pignatari

E. Zinner

M. G. Bertolli

R. Trappitsch

P. Hoppe

T. Rauscher

C. Fryer

F. Herwig

F. X. Timmes

F.-K. Thielemann



Abstract

Carbon-rich grains are observed to condense in the ejecta of recent core-collapse supernovae (SNe) within a year after the explosion. Silicon carbide grains of type X are C-rich grains with isotopic signatures of explosive SN nucleosynthesis have been found in primitive meteorites. Much rarer silicon carbide grains of type C are a special sub-group of SiC grains from SNe. They show peculiar abundance signatures for Si and S, isotopically heavy Si, and isotopically light S, which appear to be in disagreement with model predictions. We propose that C grains are formed mostly from C-rich stellar material exposed to lower SN shock temperatures than the more common type X grains. In this scenario, extreme 32S enrichments observed in C grains may be explained by the presence of short-lived 32Si (τ1/2 = 153 yr) in the ejecta, produced by neutron capture processes starting from the stable Si isotopes. No mixing from deeper Si-rich material and/or fractionation of Si from S due to molecular chemistry is needed to explain the 32S enrichments. The abundance of 32Si in the grains can provide constraints on the neutron density reached during the SN explosion in the C-rich He shell material. The impact of the large uncertainty of the neutron capture cross sections in the 32Si region is discussed.

Citation

Pignatari, M., Zinner, E., Bertolli, M. G., Trappitsch, R., Hoppe, P., Rauscher, T., …Thielemann, F. (in press). SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE 32 Si IN SUPERNOVAE. Astrophysical Journal Letters, 771(1), L7. https://doi.org/10.1088/2041-8205/771/1/l7

Journal Article Type Letter
Acceptance Date May 23, 2013
Online Publication Date Jun 13, 2013
Deposit Date Jun 16, 2023
Journal The Astrophysical Journal
Print ISSN 2041-8205
Electronic ISSN 2041-8213
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 771
Issue 1
Pages L7
DOI https://doi.org/10.1088/2041-8205/771/1/l7
Keywords Space and Planetary Science; Astronomy and Astrophysics