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Resonance-like structure near the $\eta d$ threshold in the $\gamma{d}${$\to$}$\pi^0\eta{d}$ reaction

Authors :
Ishikawa, T.
Fujimura, H.
Fukasawa, H.
Hashimoto, R.
He, Q.
Honda, Y.
Iwata, T.
Kaida, S.
Kasagi, J.
Kawano, A.
Kuwasaki, S.
Maeda, K.
Masumoto, S.
Miyabe, M.
Miyahara, F.
Mochizuki, K.
Muramatsu, N.
Nakamura, A.
Nawa, K.
Obara, Y.
Ogushi, S.
Okada, Y.
Okamura, K.
Onodera, Y.
Ozawa, K.
Sakamoto, Y.
Sato, M.
Shimizu, H.
Sugai, H.
Suzuki, K.
Tajima, Y.
Takahashi, S.
Taniguchi, Y.
Tsuchikawa, Y.
Yamazaki, H.
Yamazaki, R.
Yoshida, H. Y.
Publication Year :
2021

Abstract

To investigate the interaction between the nucleon $N$ and nucleon resonance $N(1535)1/2^-$, the $\eta d$ threshold structure connected to the isoscalar $S$-wave $N$-$N(1535)1/2^-$ system has been experimentally studied in the $\gamma{d}${$\to$}$\pi^0\eta{d}$ reaction at incident photon energies ranging from the reaction threshold to 1.15 GeV. A strong enhancement is observed near the $\eta d$ threshold over the three-body phase-space contribution in the $\eta d$ invariant-mass distribution. An analysis incorporating the known isovector resonance $\mathcal{D}_{12}$ with a spin-parity of $2^+$ in the $\pi^0d$ channel reveals the existence of a narrow isoscalar resonance-like structure with $1^-$ in the $\eta d$ system. Using a Flatt\'e parametrization, the mass is found to be $2.427_{-0.006}^{+0.013}$ GeV, close to the $\eta d$ threshold, and the width is $\left(0.029_{-0.029}^{+0.006}{\rm\ GeV}\right)+\left(0.00_{-0.00}^{+0.41}\right) p_\eta c$, where $p_\eta$ denotes the $\eta$ momentum in the rest frame of the $\eta d$ system. The observed structure would be attributed to a predicted isoscalar $1^-$ $\eta NN$ bound state from $\eta NN$ and $\pi NN$ coupled-channel calculation, or an $\eta d$ virtual state owing to strong $\eta d$ attraction.<br />Comment: 6 pages, 3 figures

Subjects

Subjects :
Nuclear Experiment

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2105.10887
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevC.104.L052201