Analysis of previous microscopic calculations for the second 0 + state in 12 C in terms of 3-α particle Bose-condensed state

By Y. Funaki, A. Tohsaki, H. Horiuchi, P. Schuck, G. Röpke. 2003

179 citations recorded by the source corpus.

The wave function of the second ${0}^{+}$ state of ${}^{12}\mathrm{C},$ which was obtained a long time ago by solving the microscopic $3\ensuremath{\alpha}$ problem, is shown to be almost completely equivalent to the wave function of the $3\ensuremath{\alpha}$ condensed state, which has been proposed recently by the present authors. This equivalence of the wave functions is shown to hold in two cases where different effective two-nucleon forces are adopted. This finding gives strong support for interpreting the second ${0}^{+}$ state of ${}^{12}\mathrm{C},$ which is the key state for the synthesis of ${}^{12}\mathrm{C}$ in stars (``Hoyle'' state), and which is one of the typical mysterious ${0}^{+}$ states in light nuclei, as a gaslike structure of three $\ensuremath{\alpha}$ particles, Bose condensed into an identical s-wave function.

Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/0ea1a8c0300524846fb24b64751259bd89147515

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In Atomic and Molecular Physics, and Optics

  1. Martin Freer
  2. U. Meissner
  3. Dean Lee

In Nuclear and High Energy Physics

  1. Martin Freer
  2. Dean Lee
  3. H. Horiuchi
  4. Y. Kanada-En’yo
  5. U. Meissner
  6. Evgeny Epelbaum
  7. H. Hammer
  8. Hermann Krebs

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