8–10 Mar 2021
Yukawa Institute for Theoretical Physics, Kyoto University
Asia/Tokyo timezone

Low-energy neutron-neutron scattering studied with pion photoproduction on the deuteron

8 Mar 2021, 16:40
20m
Panasonic hall (Yukawa Institute for Theoretical Physics, Kyoto University)

Panasonic hall

Yukawa Institute for Theoretical Physics, Kyoto University

Speaker

Satoshi Nakamura (University of Science and Technology of China)

Description

The low-energy neutron-neutron scattering has been studied by analyzing the final $nn$ interactions in $nd\to nnp$ ($n$,$p$,$d$ are neutron, proton and deuteron, respectively) and $\pi^- d\to nn \gamma$ data. The resulting neutron-neutron scattering length ($a_{nn}$) differs from the proton-proton one ($a_{pp}$), indicating the charge symmetry breaking of the nuclear force. However, the situation is not conclusive enough because the result from $nd\to nnp$ does not agree with that from $\pi^- d\to nn \gamma$. Also, the analysis of $nd\to nnp$ could suffer from three-nucleon force effects which have not been well-established yet, while the $\pi^- d\to nn \gamma$ data have a hard-to-control uncertainty of the neutron detection efficiency. Thus an independent and different determination of $a_{nn}$ is highly desirable. We discuss the possibility of extracting $a_{nn}$ and effective range $r_{nn}$ from cross section data ($d^2\sigma/dM_{nn}/d\Omega_\pi$), as a function of the $nn$ invariant mass $M_{nn}$, for $\pi^+$ photoproduction on the deuteron ($\gamma d\to \pi^+nn$). The analysis is based on a $\gamma d\to \pi^+nn$ reaction model in which realistic elementary amplitudes for $\gamma p\to \pi^+n$, $NN\to NN$, and $\pi N\to \pi N$ are built in. We show that $M_{nn}$ dependence (lineshape) of a ratio $R_{\rm th}$, $d^2\sigma/dM_{nn}/d\Omega_\pi$ normalized by $d\sigma/d\Omega_\pi$ for $\gamma p\to\pi^+ n$ and the nucleon momentum distribution inside the deuteron, at the kinematics with $\theta_\pi=0^\circ$ and $E_\gamma\sim 250$ MeV is particularly useful for extracting $a_{nn}$ and $r_{nn}$ from the corresponding data $R_{\rm exp}$. It is found that $R_{\rm exp}$ with 2% error, resolved into the $M_{nn}$ bin width of 0.04 MeV (corresponding to the $p_\pi$ bin width of 0.05 MeV$/c$), can determine $a_{nn}$ and $r_{nn}$ with uncertainties of $\pm 0.21$ fm and $\pm 0.06$ fm, respectively, for the case of $a_{nn}=-18.9$ fm and $r_{nn}=2.75$ fm. The requirement of such narrow bin widths indicates that the momenta of the incident photon and the emitted $\pi^+$ have to be measured with high resolutions. This can be achieved by utilizing virtual photons of very small $Q^2$ from electron scattering at Mainz MAMI facility. The proposed method for determining $a_{nn}$ and $r_{nn}$ from $\gamma d\to \pi^+ nn$ has a great experimental advantage over the previous one utilizing $\pi^- d\to\gamma nn$ for being free from the formidable task of controlling the neutron detection efficiency and its uncertainty. This presentation is based on our recent work [1]. [1] S.X. Nakamura, T. Ishikawa, and T. Sato, arXiv:2003.02497.

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