Investigation of the reaction 90Zr(p,γ) with in-beam γ-ray spectroscopy
Investigation of the reaction 90Zr(p,γ) with in-beam γ-ray spectroscopy
About this item
Full title
Author / Creator
Erbacher, Philipp , Endres, A , Glorius, J , Netterdon, L , Sonnabend, K , Thomas, B and Zilges, A
Publisher
Les Ulis: EDP Sciences
Journal title
Language
English
Formats
Publication information
Publisher
Les Ulis: EDP Sciences
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Scope and Contents
Contents
The p nucleus 92Mo is believed to be mainly produced through photodisintegration reactions in type II supernovae. However, this production scenario cannot solely account for the observed solar relative isotopic abundance of 92Mo. Additional production scenarios have been suggested to explain this discrepancy. One of these scenarios could be the pro...
Alternative Titles
Full title
Investigation of the reaction 90Zr(p,γ) with in-beam γ-ray spectroscopy
Authors, Artists and Contributors
Author / Creator
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Primary Identifiers
Record Identifier
TN_cdi_doaj_primary_oai_doaj_org_article_684c0acc8006436eb4cfb44e4ca797aa
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_684c0acc8006436eb4cfb44e4ca797aa
Other Identifiers
ISSN
2101-6275
E-ISSN
2100-014X
DOI
10.1051/epjconf/20159302021
