Abstract

We study the $^{11}\mathrm{Li}$ and $^{22}\mathrm{C}$ nuclei at leading order (LO) in halo effective field theory (Halo EFT). Using the value of the $^{22}\mathrm{C}$ rms matter radius deduced in Ref. [1] as an input in a LO calculation, we simultaneously constrained the values of the two-neutron (2$n$) separation energy of $^{22}\mathrm{C}$ and the virtual-state energy of the $^{20}\mathrm{C}-$neutron system (hereafter denoted $^{21}$C). The 1$-\sigma$ uncertainty of the input rms matter radius datum, along with the theory error estimated from the anticipated size of the higher-order terms in the Halo EFT expansion, gave an upper bound of about 100 keV for the 2$n$ separation energy. We also study the electric dipole excitation of 2$n$ halo nuclei to a continuum state of two neutrons and the core at LO in Halo EFT. We first compare our results with the $^{11}\mathrm{Li}$ data from a Coulomb dissociation experiment and obtain good agreement within the theoretical uncertainty of a LO calculation. We then obtain the low-energy spectrum of $B(E1)$ of this transition at several different values of the 2$n$ separation energy of $^{22}\mathrm{C}$ and the virtual-state energy of $^{21}\mathrm{C}$. Our predictions can be compared to the outcome of an ongoing experiment on the Coulomb dissociation of $^{22}\mathrm{C}$ to obtain tighter constraints on the two- and three-body energies in the $^{22}\mathrm{C}$ system.

Highlights

  • Introduction[1], Tanaka et al measured the reaction cross-section of 22C on a hydrogen target and, using Glauber calculations, deduced a 22C rms matter radius of 5.4 ± 0.9 fm, implying that 22C is an S-wave two-neturon halo nucleus

  • The effects of interactions that are higher order in the Halo EFT power counting are estimated from the size of the ignored higher-order terms and included as theory error bands

  • We study the E1 excitation of 2n halo nuclei to the three-body continuum

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Summary

Introduction

[1], Tanaka et al measured the reaction cross-section of 22C on a hydrogen target and, using Glauber calculations, deduced a 22C rms matter radius of 5.4 ± 0.9 fm, implying that 22C is an S-wave two-neturon halo nucleus. This conclusion is supported by data on high-energy twoneutron removal from 22C [6]. [7], to calculate the rms matter radius of 22C as a model-independent function of EB and Enc. Since the virtual-state energy of the unbound [8] 21C is not well known [9], we used Halo EFT to find constraints in the (EB, Enc) plane using Tanaka et al.’s value of the rms matter radius. These findings will be published in Ref. [11]

Matter radius constraints on the binding energy
Conclusion
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