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Universal Properties of Weakly Bound Two-Neutron Halo Nuclei

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abstract

We construct an effective field theory of a two-neutron halo nucleus in the limit where the two-neutron separation energy $B$ and the neutron-neutron two-body virtual energy $\epsilon_n$ are smaller than any other energy scale in the problem, but the scattering between the core and a single neutron is not fine-tuned, and the Efimov effect does not operate. The theory has one dimensionless coupling which formally runs to a Landau pole in the ultraviolet. We show that many properties of the system are universal in the double fine-tuning limit. The ratio of the mean-square matter radius and charge radius is found to be $\langle r^2_m \rangle/\langle r^2_c\rangle = A f(\epsilon_n/B)$, where $A$ is the mass number of the core and $f$ is a function of the ratio $\epsilon_n/B$ which we find explicitly. In particular, when $B\gg\epsilon_n$, $\langle r^2_m\rangle/\langle r^2_c\rangle = \frac23 A$. The shape of the the $E1$ dipole strength function also depends only on the ratio $\epsilon_n/B$ and is derived in explicit analytic form. We estimate that for the $^{22}$C nucleus higher-order corrections to our theory are of order 20% or less if the two-neutron separation energy is less than 100 keV and the $s$-wave scattering length between a neutron and a $^{20}$C nucleus is less than 2.8 fm.

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  • Non-Efimovian two-neutron halos with an $s$-wave core-neutron resonance nucl-th · 2025-07-25 · conditional · none · ref 9 · internal anchor

    Two-neutron halos with a near-threshold s-wave core-neutron resonance need no three-body parameter: two-body input fixes the halo, and applying the framework to carbon-22 rules out the reported 0.8 MeV resonance as too narrow.