# Search for $X(3872)$ and $X(3915)$ decay into $\chi_{c1} \pi^0$ in $B$   decays at Belle

**Authors:** V. Bhardwaj, S. Jia, I. Adachi, H. Aihara, D. M. Asner, T. Aushev, R., Ayad, V. Babu, I. Badhrees, S. Bahinipati, V. Bansal, P. Behera, C. Bele\~no,, M. Berger, B. Bhuyan, T. Bilka, J. Biswal, A. Bobrov, A. Bondar, G., Bonvicini, A. Bozek, M. Bra\v{c}ko, T. E. Browder, M. Campajola, L. Cao, D., \v{C}ervenkov, P. Chang, 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,, S. Di Carlo, Z. Dole\v{z}al, T. V. Dong, S. Eidelman, D. Epifanov, J. E., Fast, T. Ferber, B. G. Fulsom, R. Garg, V. Gaur, N. Gabyshev, A. Garmash, A., Giri, P. Goldenzweig, D. Greenwald, O. Grzymkowska, J. Haba, T. Hara, K., Hayasaka, H. Hayashii, W.-S. Hou, C.-L. Hsu, T. Iijima, K. Inami, A., Ishikawa, R. Itoh, M. Iwasaki, Y. Iwasaki, W. W. Jacobs, Y. Jin, D. Joffe, K., K. Joo, T. Julius, A. B. Kaliyar, G. Karyan, Y. Kato, T. Kawasaki, C., Kiesling, C. H. Kim, D. Y. Kim, S. H. Kim, K. Kinoshita, P. Kody\v{s}, S., Korpar, D. Kotchetkov, P. Kri\v{z}an, R. Kroeger, P. Krokovny, T. Kuhr, R., Kulasiri, R. Kumar, Y.-J. Kwon, K. Lalwani, 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, D., Liventsev, P.-C. Lu, J. MacNaughton, C. MacQueen, M. Masuda, T. Matsuda, D., Matvienko, M. Merola, K. Miyabayashi, R. Mizuk, G. B. Mohanty, T. Mori, R., Mussa, M. Nakao, K. J. Nath, M. Nayak, M. Niiyama, N. K. Nisar, S. Nishida,, K. Nishimura, S. Ogawa, H. Ono, Y. Onuki, P. Pakhlov, G. Pakhlova, B. Pal, S., Pardi, H. Park, S.-H. Park, S. Patra, S. Paul, T. K. Pedlar, R. Pestotnik, L., E. Piilonen, V. Popov, E. Prencipe, P. K. Resmi, M. Ritter, A. Rostomyan, G., Russo, Y. Sakai, M. Salehi, S. Sandilya, L. Santelj, T. Sanuki, V. Savinov,, O. Schneider, G. Schnell, C. Schwanda, Y. Seino, K. Senyo, O. Seon, M. E., Sevior, C. P. Shen, J.-G. Shiu, B. Shwartz, F. Simon, A. Sokolov, E., Solovieva, M. Stari\v{c}, Z. S. Stottler, M. Sumihama, T. Sumiyoshi, W., Sutcliffe, M. Takizawa, U. Tamponi, K. Tanida, F. Tenchini, K. Trabelsi, M., Uchida, S. Uehara, T. Uglov, S. Uno, P. Urquijo, R. Van Tonder, G. Varner, B., Wang, C. H. Wang, M.-Z. Wang, P. Wang, X. L. Wang, M. Watanabe, S. Watanuki,, E. Won, S. B. Yang, H. Ye, J. Yelton, J. H. Yin, J. Zhang, Z. P. Zhang, V., Zhilich, V. Zhukova, V. Zhulanov

arXiv: 1904.07015 · 2019-06-19

## TL;DR

This paper searches for specific decay modes of the $X(3872)$ and $X(3915)$ particles in B meson decays, setting upper limits on their branching fractions and ratios, based on a large dataset from the Belle experiment.

## Contribution

It provides the first upper limits on the decay of $X(3872)$ and $X(3915)$ into $	ext{chi}_{c1} 	ext{pi}^0$ in B decays, improving understanding of these exotic states.

## Key findings

- Upper limit on $B^+ 	o X(3872) K^+$ with $X(3872) 	o 	ext{chi}_{c1} 	ext{pi}^0$
- Upper limit on $B^+ 	o X(3915) K^+$ with $X(3915) 	o 	ext{chi}_{c1} 	ext{pi}^0$
- Ratio $	ext{Br}(X(3872) 	o 	ext{chi}_{c1} 	ext{pi}^0)/	ext{Br}(X(3872) 	o J/\psi 	ext{pi}^+ 	ext{pi}^-)$ constrained to be less than 0.97

## Abstract

We report a search for $X(3872)$ and $X(3915)$ in $B^+ \to \chi_{c1} \pi^0 K^+$ decays. We set an upper limit of $\mathcal{B}(B^+ \to X(3872) K^+) \times \mathcal{B}(X(3872) \to \chi_{c1} \pi^0)$ $ < 8.1 \times 10^{-6}$ and $\mathcal{B}(B^+ \to X(3915) K^+) \times \mathcal{B}(X(3915) \to \chi_{c1} \pi^0)$ $ < 3.8 \times 10^{-5}$ at 90\% confidence level. We also measure $\mathcal{B}(X(3872) \to \chi_{c1} \pi^0)/\mathcal{B}(X(3872) \to J/\psi \pi^+ \pi^-) < 0.97$ at 90\% confidence level. The results reported here are obtained from $772 \times 10^{6}$ $B\overline{B}$ events collected at the $\Upsilon(4S)$ resonance with the Belle detector at the KEKB asymmetric-energy $e^+e^-$ collider.

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1904.07015/full.md

## References

30 references — full list in the complete paper: https://tomesphere.com/paper/1904.07015/full.md

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Source: https://tomesphere.com/paper/1904.07015