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First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV...

First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_40dd0a47d06440e1b6fc0534611b525a

First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process

About this item

Full title

First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process

Publisher

Les Ulis: EDP Sciences

Journal title

EPJ Web of conferences, 2022-01, Vol.260, p.11026

Language

English

Formats

Publication information

Publisher

Les Ulis: EDP Sciences

More information

Scope and Contents

Contents

Most elements heavier than iron have been generated in the stellar media by means of neutron capture reactions, approximately half are produced by the slow neutron capture or s-process. Radiative neutron capture cross section measurements are of fundamental importance for the study of this mechanism. In this contribution we present a brief summary...

Alternative Titles

Full title

First 80Se(n,γ) cross section measurement with high resolution in the full stellar energy range 1 eV - 100 keV and its astrophysical implications for the s-process

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_40dd0a47d06440e1b6fc0534611b525a

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_40dd0a47d06440e1b6fc0534611b525a

Other Identifiers

ISSN

2101-6275

E-ISSN

2100-014X

DOI

10.1051/epjconf/202226011026

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