S-factor measurement of the 2H(α,γ)6Li reaction at energies relevant for Big-Bang nucleosynthesis

S-factor measurement of the 2H(α,γ)6Li reaction at energies relevant for Big-Bang nucleosynthesis

For about 20 years now, observations of 6Li in several old metal-poor stars inside the halo of our galaxy have been reported, which are largely independent of the stars’ metallicity, and which point to a possible primordial origin. The observations exceed the predictions of the Standard Big-Bang Nuc...

Full description

Bibliographic Details
Main Author: Anders, Michael
Other Authors: Technische Universität Dresden, Institut für kern- und Teilchenphysik
Format: Others
Language:English
Published: Forschungszentrum Dresden 2014
Subjects:
Urknall-Nukleosynthese LUNA Beschleuniger
Laboratory for Underground Nuclear Astrophysics
Experimental nuclear astrophysics Big-Bang nucleosynthesis Underground accelerator LUNA in-beam gamma-ray spectrometry neutron background
ddc:339
Online Access:http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-141091
http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-141091
http://www.qucosa.de/fileadmin/data/qucosa/documents/14109/20316.pdf

Internet

http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-141091
http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-141091
http://www.qucosa.de/fileadmin/data/qucosa/documents/14109/20316.pdf

Similar Items