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Cross section measurements of the Big Bang nucleosynthesis reaction D($\alpha,gamma)^6Li$ by Coulomb dissociation of $^6Li$

Authors :
P. Koczon
Stefan Typel
A. Walus
F. Schümann
Naohito Iwasa
Kilian Eberhard Schwarz
Andreas Wagner
V. Tatischeff
E. Schwab
J. Kiener
D. Galaviz
F. Attallah
M. Caamaño
O. Sorlin
P. Senger
J. P. Thibaud
Margareta Hellström
A. Coc
Hans Geissel
K. Sümmerer
F. Uhlig
F. Hammache
B. Kohlmeyer
D. Cortina
Institut de Physique Nucléaire d'Orsay (IPNO)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Helmholtz zentrum für Schwerionenforschung GmbH (GSI)
Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM)
S.V. Harissopulos
P. Demetriou
R. Julin
Source :
International Conference on Frontiers in Nuclear Structures, Astrophysics and Reactions-FINUSTAR 2005, International Conference on Frontiers in Nuclear Structures, Astrophysics and Reactions-FINUSTAR 2005, Sep 2005, Isle of Kos, Greece. pp.21-25, ⟨10.1063/1.2200893⟩
Publication Year :
2005
Publisher :
HAL CCSD, 2005.

Abstract

International audience; The possibility that big-bang nucleosynthesis (BBN) may produce nontrivial amounts of 6Li is under study since the recent observations of this element in old halo stars. However, the interpretation of these observations needs a precise knowledge of the reaction rate of D(alpha, gamma)6Li which, at present, is extremely uncertain (a factor of 20) at the energies of astrophysical interest (Ecm

Details

Language :
English
Database :
OpenAIRE
Journal :
International Conference on Frontiers in Nuclear Structures, Astrophysics and Reactions-FINUSTAR 2005, International Conference on Frontiers in Nuclear Structures, Astrophysics and Reactions-FINUSTAR 2005, Sep 2005, Isle of Kos, Greece. pp.21-25, ⟨10.1063/1.2200893⟩
Accession number :
edsair.doi.dedup.....effae039dd560a0c9f418f09d5106f54
Full Text :
https://doi.org/10.1063/1.2200893⟩