Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Neutron capture cross section of unstable Ni63: Implications for stellar nucleosynthesis

Thumbnail Image

Date

2013

Authors

Lederer, C
Massimi, C
Altstadt, S
Andrzejewski, J.
Audouin, L
Barbagallo, M
Becares, V
Becvar, F
Billowes, J.
Schumann, D.

Journal Title

Journal ISSN

Volume Title

Publisher

American Physical Society

Abstract

The Ni63(n,γ) cross section has been measured for the first time at the neutron time-of-flight facility n-TOF at CERN from thermal neutron energies up to 200 keV. In total, capture kernels of 12 (new) resonances were determined. Maxwellian averaged cross

Description

Keywords

Keywords: Massive stars; Neutron capture cross section; S-process; Stellar models; Stellar nucleosynthesis; Thermal neutron energy; Time of flight; Chemical elements; Nucleosynthesis; Stars

Citation

URI

http://hdl.handle.net/1885/77437

Collections

ANU Research Publications

Source

Physical Review Letters

Type

Journal article

Book Title

Entity type

Access Statement

Open Access

License Rights

DOI

10.1103/PhysRevLett.110.022501

Restricted until

Downloads

File
Description
01_Lederer_Neutron_capture_cross_section_2013.pdf (507.39 KB)

DSpace software copyright © 2002-2026 LYRASIS