Spatial Structure of the 12C Nucleus in a 3α Model with Deep Potentials Containing Forbidden States

Abstract

The spatial structure of the lowest 01+, 02+, 21+ and 22+ states of the 12C nucleus is studied within the 3α model with the Buck, Friedrich, and Wheatley α α potential with Pauli forbidden states in the S and D waves. The Pauli forbidden states in the three-body system are treated by the exact orthogonalization method. The largest contributions to the ground and excited 21+ bound states energies come from the partial waves (λ, )=(2,2) and (λ, )=(4,4). As was found earlier, these bound states are created by the critical eigenstates of the three-body Pauli projector in the 0+ and 2+ functional spaces, respectively. These special eigenstates of the Pauli projector are responsible for the quantum phase transitions from a weakly bound "gas-like" phase to a deep "quantum liquid" phase. In contrast to the bound states, for the Hoyle resonance 02+ and its analog state 22+, dominant contributions come from the (λ, )=(0,0) and (λ, )=(2,2) configurations, respectively. The estimated probability density functions for the 12C(01+) ground and 21+ excited bound states show mostly a triangular structure, where the α particles move at a distance of about 2.5 fm from each other. However, the spatial structure of the Hoyle resonance and its analog state have a strongly different structure, like 8Be + α. In the Hoyle state, the last α particle moves far from the doublet at the distance between R=3.0 fm and R=5.0 fm. In the Hoyle analog 22+ state the two alpha particles move at a distance of about 15 fm, but the last α particle can move far from the doublet at the distance up to R=30.0 fm.

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