English

Neutron-neutron scattering length from the $^6$He$(p,p\alpha)nn$ reaction

Nuclear Theory 2021-08-11 v2 Nuclear Experiment

Abstract

We propose a novel method to measure the neutron-neutron scattering length using the 6^{6}He(p,pα)nn(p,p\alpha)nn reaction in inverse kinematics at high energies. The method is based on the final state interaction (FSI) between the neutrons after the sudden knockout of the α\alpha particle. We show that the details of the neutron-neutron relative energy distribution allow for a precise extraction of the ss-wave scattering length. We present the state-of-the-art in regard to the theory of this distribution. The distribution is calculated in two steps. First, we calculate the ground-state wave function of 6^6He as a αnn\alpha n n three-body system. For this purpose we use Halo effective field theory (Halo EFT), which also provides uncertainty estimates for the results. We compare our results at this stage to model calculations done with the computer code FaCE. In a second step we determine the effects of the nnnn FSI using the nnnn t-matrix. We compare these FSI results to approximate FSI approaches based on standard FSI enhancement factors. While the final distribution is sensitive to the nnnn scattering length, it depends only weakly on the effective range. Throughout we emphasize the impact of theoretical uncertainties on the neutron-neutron relative energy distribution, and discuss the extent to which those uncertainties limit the extraction of the neutron-neutron scattering length from the reaction 6^{6}He(p,pα)nn(p,p\alpha)nn.

Keywords

Cite

@article{arxiv.2103.03224,
  title  = {Neutron-neutron scattering length from the $^6$He$(p,p\alpha)nn$ reaction},
  author = {Matthias Göbel and Thomas Aumann and Carlos A. Bertulani and Tobias Frederico and Hans-Werner Hammer and Daniel R. Phillips},
  journal= {arXiv preprint arXiv:2103.03224},
  year   = {2021}
}

Comments

Paper + supplemental material: 20+11 pages, 7+4 figures. Paper restructured, further explanations and discussions added, results unchanged. Accepted for publication in Phys. Rev. C