Table of Contents
Fetching ...

Possible Existence of $^3_φ$H, $^4_φ$H, $^4_φ$He, and $^5_φ$He Nuclei

Rimantas Lazauskas, Roman Ya. Kezerashvili, Igor Filikhin

Abstract

Motivated by recent HAL QCD simulations of the $φN$ interaction in the $^4S_{3/2}$ channel and its modification in the $^2S_{1/2}$ channel, we develop a first-principles few-body framework that embeds these potentials into configuration-space Faddeev--Yakubovsky equations. We predict bound $^4_φ\mathrm{H}$, $^4_φ\mathrm{He}$, and $^5_φ\mathrm{He}$ nuclei by performing calculations for $φ$-mesic $φNNN$ and $φNNNN$ systems. Both spin-dependent and spin-independent $φN$ interactions are considered, leading to deeply and moderately bound states, respectively. The deeply bound states originate from the strong attraction in the $^2S_{1/2}$ $φN$ channel. Coulomb shifts of the binding energies are evaluated. Our findings provide the binding mechanism and demonstrate the importance of short-range $φN$ attraction.

Possible Existence of $^3_φ$H, $^4_φ$H, $^4_φ$He, and $^5_φ$He Nuclei

Abstract

Motivated by recent HAL QCD simulations of the interaction in the channel and its modification in the channel, we develop a first-principles few-body framework that embeds these potentials into configuration-space Faddeev--Yakubovsky equations. We predict bound , , and nuclei by performing calculations for -mesic and systems. Both spin-dependent and spin-independent interactions are considered, leading to deeply and moderately bound states, respectively. The deeply bound states originate from the strong attraction in the channel. Coulomb shifts of the binding energies are evaluated. Our findings provide the binding mechanism and demonstrate the importance of short-range attraction.
Paper Structure (1 section, 6 equations, 1 figure, 2 tables)

This paper contains 1 section, 6 equations, 1 figure, 2 tables.

Table of Contents

  1. Acknowledgments

Figures (1)

  • Figure 1: The upper ($a$) and ($b$) panels illustrate the distinct topological decompositions of the fully interacting $\phi NNN$ and $\phi NNNN$ clusters, respectively, into their substructures. The lower panel presents the Jacobi coordinate systems associated with each of these cluster partitions. Low panels: ($a$) K-like and H-like components, as $\Phi^l_{12,3}$ and $\Phi^l_{12,34}$, respectively. Permuting the particle indices yields 12 $\mathcal{K}$-type components and 6 $\mathcal{H}$-like components; ($b$) The five independent 5-body FYE components are denoted as K, H, T, S, F. The permutation of particle indexes gives 60 K-type amplitudes and 30 for each H, T, S, and F-type amplitudes Lazauskas2018aLazauskas2018b. Ultimately, this yields a system of 180 Faddeev-Yakubovsky equations.