Bayesian three-body modeling of 22C reveals it is bound by less than 0.35 MeV with s-wave dominance and highlights the need for final-state interactions in dipole strength calculations, with ~50% uncertainties.
How Many-Body Correlations andα Clustering Shape 6He.Phys
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NCSMC enables ab initio predictions of structure, resonances, and reactions in halo nuclei such as 6He, 8B, 11Be, and 15C from chiral interactions alone.
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Uncertainty quantified three-body model applied to the two-neutron halo $^{22}$C
Bayesian three-body modeling of 22C reveals it is bound by less than 0.35 MeV with s-wave dominance and highlights the need for final-state interactions in dipole strength calculations, with ~50% uncertainties.
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Halo Nuclei from Ab Initio Nuclear Theory
NCSMC enables ab initio predictions of structure, resonances, and reactions in halo nuclei such as 6He, 8B, 11Be, and 15C from chiral interactions alone.