Abstract:The Faddeev equations in configuration space are used to study the 12C nucleus considered as the 3α cluster system. The model includes a phenomenological (Ali–Bodmer) pair potential having s, d and g partial wave components, a three-body potential and takes into account the Coulomb interaction. The range parameter of the three-body potential is fixed by adjusting the position of the diffraction minimum of the 12C elastic form factor. To choose this parameter, we apply an s-wave model that allows us to reproduc… Show more
“…Next, the assumption on the "frozen" nucleon distribution in the α-particles is used to calculate the experimentally observable nucleonic structural characteristics, e. g., the root-mean-square (r. m. s.) radii and the transition radius R 12 . This extended α-cluster model leads generally to a satisfactory description of the 12 C nucleus [10,[13][14][15]20]. In particular, the calculated Γ and M 12 [13,14] are in reasonable agreement with experimental data (up to a factor two) even for the simplified local α -α interactions.…”
The near-threshold 12 C(0 2 -state structure is described as a system of three α-particles oscillating between the ground-state-like configuration and the elongated chain configuration whose probability exceeds 0.9.
“…Next, the assumption on the "frozen" nucleon distribution in the α-particles is used to calculate the experimentally observable nucleonic structural characteristics, e. g., the root-mean-square (r. m. s.) radii and the transition radius R 12 . This extended α-cluster model leads generally to a satisfactory description of the 12 C nucleus [10,[13][14][15]20]. In particular, the calculated Γ and M 12 [13,14] are in reasonable agreement with experimental data (up to a factor two) even for the simplified local α -α interactions.…”
The near-threshold 12 C(0 2 -state structure is described as a system of three α-particles oscillating between the ground-state-like configuration and the elongated chain configuration whose probability exceeds 0.9.
“…This was e.g. done within so-called semimicroscopic models (considering structureless α-particles) [2,3,4,5,6,7,8] and within fully microscopic models [9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24].…”
We investigate both bound and resonance states in 12 C embedded in a three-α-cluster continuum using a three-cluster microscopic model. The model relies on the Hyperspherical Harmonics basis to enumerate the channels describing the three-cluster discrete and continuous spectrum states. It yields the most probable distribution of the three α-clusters in space, and the dominant decay modes of the three-cluster resonances.
“…Obviously, a more detailed calculation should still be made in order to verify the extension of our results, as the two-body potential used in this toy model is not including higher partial waves, which are crucial to describe correctly the properties of 12 C [15][16][17]. A detailed analysis of the structure of the Hoyle state in 12 C, based on precise electron scattering data, can be found in [27].…”
Section: Discussionmentioning
confidence: 82%
“…We should mention here that the two-body potential used in this toy model does not consider higher partial waves, in particular d and g waves, which give a significant contribution to the properties of 12 C [15]. Much more realistic calculations can be found in [16,17].…”
Abstract-Motivated by the possibility of the second energy level (0 + 2 ) of 12 C (in a three-alpha model) to turn into an Efimov state, we study a simple non-realistic toy model formed by three bosons interacting by the phenomenological s-wave Ali-Bodmer potential plus a Coulomb interaction. An artificial three-body potential was used to create a resonance with energy close to the energy of the 0 + 2 of 12 C, 0.38 MeV. The strength of the Coulomb potential is decreased until the energies of the two alpha pairs are zero. The system was placed inside a harmonic trap and a stabilization method has been used to calculate the energies of the resonances. We found that the shielded-Coulomb potential, which keeps the long tail, is not able to produce the Efimov effect. The energy of the three alphas decreases only to 0.19 MeV when the two-body energy crosses the threshold to become bound.
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