Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..545t&link_type=abstract
ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,
Astronomy and Astrophysics
Astronomy
Scientific paper
The ground state properties of the carbon isotopes are investigated using the extended version of the Antisymmetrized Molecular Dynamics (AMD) Multi Slater Determinant method. We can reproduce reasonably well many experimental data for 12C-22C. In this contribution we present a systematic calculation of binding energies, energies of the 21+ states and B(E2) transition strengths.
Ikeda Kiyomi
Itagaki Naoyuki
Otsuka Tomohiro
Thiamova G.
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