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Momentum-space probability density of ${}^6$He in Halo Effective Field Theory
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abstract
We compute the momentum-space probability density of ${}^6$He at leading order in Halo EFT. In this framework, the ${}^6$He nucleus is treated as a three-body problem with a ${}^4$He core ($c$) and two valence neutrons ($n$). This requires the $nn$ and $nc$ t-matrices as well as a $cnn$ force as input in the Faddeev equations. Since the $nc$ t-matrix corresponds to an energy-dependent potential, we consider the consequent modifications to the standard normalization and orthogonality conditions. We find that these are small for momenta within the domain of validity of Halo EFT. In this regime, the ${}^6$He probability density is regulator independent, provided the cutoff is significantly above the EFT breakdown scale.
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Renormalizing Two-Neutron Halo Nuclei Without Neutron-Core Interaction
The Hongo-Son two-neutron halo EFT needs an extra renormalization condition—one input radius or scattering amplitude—before charge and matter radii can be predicted separately, and the resulting coupling has a Landau pole.
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