# Search for $\Omega(2012)\to K\Xi(1530) \to K\pi\Xi$ at Belle

**Authors:** Belle Collaboration: S. Jia, C. P. Shen, I. Adachi, J. K. Ahn, H., Aihara, S. Al Said, D. M. Asner, T. Aushev, R. Ayad, V. Babu, S. Bahinipati,, A. M. Bakich, P. Behera, C. Bele\~no, J. Bennett, M. Berger, V. Bhardwaj, T., Bilka, J. Biswal, A. Bobrov, A. Bozek, M. Bra\v{c}ko, T. E. Browder, M., Campajola, L. Cao, D. \v{C}ervenkov, V. Chekelian, A. Chen, B. G. Cheon, K., Chilikin, H. E. Cho, K. Cho, S.-K. Choi, Y. Choi, S. Choudhury, D. Cinabro,, S. Cunliffe, N. Dash, G. De Nardo, F. Di Capua, S. Di Carlo, Z. Dole\v{z}al,, T. V. Dong, S. Eidelman, D. Epifanov, J. E. Fast, B. G. Fulsom, V. Gaur, N., Gabyshev, A. Garmash, A. Giri, P. Goldenzweig, B. Golob, O. Grzymkowska, O., Hartbrich, K. Hayasaka, H. Hayashii, W.-S. Hou, K. Huang, T. Iijima, K., Inami, G. Inguglia, A. Ishikawa, R. Itoh, M. Iwasaki, Y. Iwasaki, W. W., Jacobs, Y. Jin, D. Joffe, K. K. Joo, A. B. Kaliyar, K. H. Kang, G. Karyan, Y., Kato, T. Kawasaki, H. Kichimi, D. Y. Kim, H. J. Kim, K. T. Kim, S. H. Kim, K., Kinoshita, P. Kody\v{s}, S. Korpar, D. Kotchetkov, P. Kri\v{z}an, R. Kroeger,, P. Krokovny, R. Kumar, A. Kuzmin, Y.-J. Kwon, J. S. Lange, I. S. Lee, J. K., Lee, J. Y. Lee, S. C. Lee, L. K. Li, Y. B. Li, L. Li Gioi, J. Libby, K., Lieret, D. Liventsev, P.-C. Lu, J. MacNaughton, C. MacQueen, M. Masuda, T., Matsuda, D. Matvienko, J. T. McNeil, M. Merola, H. Miyata, R. Mizuk, T. Mori,, R. Mussa, T. Nakano, M. Nakao, K. J. Nath, M. Nayak, M. Niiyama, N. K. Nisar,, S. Nishida, K. Nishimura, K. Ogawa, S. Ogawa, H. Ono, Y. Onuki, W. Ostrowicz,, P. Pakhlov, G. Pakhlova, B. Pal, T. Pang, S. Pardi, S.-H. Park, S. Patra, S., Paul, T. K. Pedlar, R. Pestotnik, L. E. Piilonen, V. Popov, E. Prencipe, M., Ritter, A. Rostomyan, G. Russo, Y. Sakai, M. Salehi, S. Sandilya, L. Santelj,, T. Sanuki, V. Savinov, O. Schneider, G. Schnell, J. Schueler, C. Schwanda, Y., Seino, K. Senyo, O. Seon, M. E. Sevior, V. Shebalin, J.-G. Shiu, A. Sokolov,, E. Solovieva, M. Stari\v{c}, J. F. Strube, M. Sumihama, T. Sumiyoshi, W., Sutcliffe, M. Takizawa, U. Tamponi, K. Tanida, F. Tenchini, M. Uchida, T., Uglov, Y. Unno, S. Uno, P. Urquijo, Y. Usov, S. E. Vahsen, R. Van Tonder, G., Varner, A. Vinokurova, A. Vossen, B. Wang, C. H. Wang, M.-Z. Wang, P. Wang,, E. Won, S. B. Yang, H. Ye, J. Yelton, J. H. Yin, C. Z. Yuan, Y. Yusa, Z. P., Zhang, V. Zhilich, V. Zhukova

arXiv: 1906.00194 · 2019-08-20

## TL;DR

This study searches for the decay of the $	ext{Omega}(2012)$ baryon into $K	o	ext{pi}	o	ext{Xi}$ using Belle data, finding no significant signals and setting upper limits on decay ratios.

## Contribution

First search for the $	ext{Omega}(2012)$ decay into $K	o	ext{pi}	o	ext{Xi}$ at Belle, providing constraints on theoretical models.

## Key findings

- No significant $	ext{Omega}(2012)$ signals observed.
- Established 90\% credibility level upper limits on decay ratios.
- Results constrain models predicting $	ext{Omega}(2012)$ as a $K	ext{Xi}(1530)$ molecule.

## Abstract

Using data samples of $e^+e^-$ collisions collected at the $\Upsilon(1S)$, $\Upsilon(2S)$, and $\Upsilon(3S)$ resonances with the Belle detector, we search for the three-body decay of the $\Omega(2012)$ baryon to $K\pi\Xi$. This decay is predicted to dominate for models describing the $\Omega(2012)$ as a $K\Xi(1530)$ molecule. No significant $\Omega(2012)$ signals are observed in the studied channels, and 90\% credibility level upper limits on the ratios of the branching fractions relative to $K \Xi$ decay modes are obtained.

## Full text

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## Figures

21 figures with captions in the complete paper: https://tomesphere.com/paper/1906.00194/full.md

## References

22 references — full list in the complete paper: https://tomesphere.com/paper/1906.00194/full.md

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Source: https://tomesphere.com/paper/1906.00194