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Adachi, I.; Aggarwal, L.; Ahmed, H.; Aihara, H.; Akopov, N.; Aloisio, A.; Anh Ky, N.; Asner, D. M.; Aushev, T.; Aushev, V.; Bae, H.; Bambade, P.; Banerjee, Sw; Baudot, J.; Bauer, M.; Beaubien, A.; Becker, J.; Behera, P. K.; Bennett, J. V.; Bernieri, E.; Bernlochner, F. U.; Bertacchi, V.; Bertemes, M.; Bertholet, E.; Bessner, M.; Bettarini, S.; Bhuyan, B.; Bianchi, F.; Bilka, T.; Biswas, D.; Bodrov, D.; Bolz, A.; Bondar, A.; Borah, J.; Bozek, A.; Bračko, M.; Branchini, P.; Browder, T. E.; Budano, A.; Bussino, S.; Campajola, M.; Cao, L.; Casarosa, G.; Cecchi, C.; Chang, M. -C.; Cheema, P.; Chekelian, V.; Chen, Y. Q.; Chilikin, K.; Chirapatpimol, K.; Cho, H. -E.; Cho, K.; Cho, S. -J.; Choi, S. -K.; Choudhury, S.; Cinabro, D.; Corona, L.; Cunliffe, S.; Das, S.; Dattola, F.; De La Cruz-Burelo, E.; de la Motte, S. A.; De Nardo, G.; de Nuccio, M.; de Pietro, G.; de Sangro, R.; Destefanis, M.; Dey, S.; de Yta-Hernandez, A.; Dhamija, R.; Di Canto, A.; Di Capua, F.; Doležal, Z.; Domínguez Jiménez, I.; Dong, T. V.; Dorigo, M.; Dort, K.; Dreyer, S.; Dubey, S.; Dujany, G.; Eliachevitch, M.; Epifanov, D.; Feichtinger, P.; Ferber, T.; Ferlewicz, D.; Fillinger, T.; Finocchiaro, G.; Fodor, A.; Forti, F.; Fulsom, B. G.; Ganiev, E.; Garmash, A.; Gaur, V.; Gaz, A.; Gellrich, A.; Ghevondyan, G.; Giordano, R.; Giri, A.; Glazov, A.; Gobbo, B.
Physical review letters, 03/2023, Letnik: 130, Številka: 9Journal Article
We study the processes $e^+e^-\to\omega\chi_{bJ}(1P)$ ($J$ = 0, 1, or 2) using samples at center-of-mass energies $\sqrt{s}$ = 10.701, 10.745, and 10.805 GeV, corresponding to 1.6, 9.8, and 4.7 fb$^{-1}$ of integrated luminosity, respectively. These data were collected with the Belle II detector during special operations of the SuperKEKB collider above the $\Upsilon(4S)$ resonance. We report the first observation of $\omega\chi_{bJ}(1P)$ signals at $\sqrt{s}$ = 10.745 GeV. By combining Belle II data with Belle results at $\sqrt{s}$ = 10.867 GeV, we find energy dependencies of the Born cross sections for $e^+e^-\to \omega\chi_{b1,b2}(1P)$ to be consistent with the shape of the $\Upsilon(10753)$ state. These data indicate that the internal structures of the $\Upsilon(10753)$ and $\Upsilon(10860)$ states may differ. Including data at $\sqrt{s}$ = 10.653 GeV, we also search for the bottomonium equivalent of the $X(3872)$ state decaying into $\omega\Upsilon(1S)$. No significant signal is observed for masses between 10.45 and 10.65 GeV/$c^2$.
