E0 transition strength and cluster structure in 13C

Details E0 transition strength and cluster structure in 13C E0 transition strength and cluster structure in 13C

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1016..451y&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From

Mathematics

Probability

Acoustic Cavitation In Liquids, 3H-, 3He-, And 4He-Induced Reactions, Cluster Models

Scientific paper

We study the structure of low-lying states of 13C with a microscopic cluster model. The second 0+ state of 12C, which is known as the Hoyle state and is important for astrophysical reactions, has been clarified to have dilute α-cluster structure. On the basis of the α-cluster model, we discuss the effect of one valence neutron in 13C on the α-cluster configuration of the Hoyle state. For these purpose, we investigate the iso-scalar E0 transition probability from the ground 1/2- state to this excited states.

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