Title: Study of Fe-60(n,gamma)Fe-61 reaction of astrophysical interest via d(Fe-60,p gamma) indirect reaction
Authors: Giron, S
Hammache, F
de Sereville, N
Beaumel, D
Burgunder, J
Caceres, L
Clement, E
Duchene, G
Flavigny, F
De France, G
Franchoo, S
Fernandez, B
Galaviz-Redondo, D
Gasques, L
Gibelin, J
Gillibert, A
Grevy, S
Guillot, J
Heil, M
Kiener, J
Lapoux, V
Marechal, F
Matta, A
Matea, Y
Moukaddam, M
Nalpas, L
Obertelli, A
Perrot, L
Raabe, Riccardo
Scarpaci, J. A
Sorlin, O
Stefan, I
Stoedel, C
Takechi, M
Thomas, J. C
Togano, Y #
Issue Date: 2010
Publisher: Amer inst physics
Host Document: Fifth european summer school on experimental nuclear astrophysics vol:1213 pages:201-204
Series Title: AIP Conference Proceedings
Conference: 5th European Summer School on Experimental Nuclear Astrophysics Sicily, ITALY, SEP 20-27, 2009
Abstract: INTEGRAL and RHESSI spacecrafts recently detected the 1.173 and 1.333 MeV gamma-ray lines coming from the Fe-60 - Co-60 - Ni-60 radioactive decay chain. The long lived isotope Fe-60 (T-1/2 = 1.5 10(6)y) is believed to be primarily produced in core-collapse supernovae. However the interpretation of the observations is difficult because of the large uncertainties concerning Fe-59(n,gamma)Fe-60 and Fe-60(n,gamma)Fe-61 cross sections, involved in Fe-60 nucleosynthesis.
ISBN: 978-0-7354-0756-5
ISSN: 0094-243X
Publication status: published
KU Leuven publication type: IC
Appears in Collections:Non-KU Leuven Association publications
# (joint) last author

Files in This Item:

There are no files associated with this item.

Request a copy


All items in Lirias are protected by copyright, with all rights reserved.

© Web of science