Observation of the decays χcJ → $$ {\mathrm{nK}}_{\mathrm{S}}^0\overline{\Lambda} $$ + c.c

A bstract By analyzing 4 . 48 × 10 8 ψ (3686) events collected with the BESIII detector, we observe the decays χ cJ → $$ {nK}_S^0\overline{\Lambda} $$ nK S 0 Λ ¯ + c . c . ( J = 0, 1, 2) for the first time, via the radiative transition ψ (3686) → γχ cJ . The branching fractions are determined to be...

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Published in:The journal of high energy physics Vol. 2021; no. 11
Main Authors: Ablikim, M., Achasov, M. N., Adlarson, P., Ahmed, S., Albrecht, M., Aliberti, R., Amoroso, A., An, M. R., An, Q., Bai, X. H., Bai, Y., Bakina, O., Baldini Ferroli, R., Balossino, I., Ban, Y., Begzsuren, K., Berger, N., Bertani, M., Bettoni, D., Bianchi, F., Bloms, J., Bortone, A., Boyko, I., Briere, R. A., Cai, H., Cai, X., Calcaterra, A., Cao, G. F., Cao, N., Cetin, S. A., Chang, J. F., Chang, W. L., Chelkov, G., Chen, D. Y., Chen, G., Chen, H. S., Chen, M. L., Chen, S. J., Chen, X. R., Chen, Y. B., Chen, Z. J., Cheng, W. S., Cibinetto, G., Cossio, F., Cui, X. F., Dai, H. L., Dai, J. P., Dai, X. C., Dbeyssi, A., de Boer, R. E., Dedovich, D., Deng, Z. Y., Denig, A., Denysenko, I., Destefanis, M., De Mori, F., Ding, Y., Dong, C., Dong, J., Dong, L. Y., Dong, M. Y., Dong, X., Du, S. X., Fan, Y. L., Fang, J., Fang, S. S., Fang, Y., Farinelli, R., Fava, L., Feldbauer, F., Felici, G., Feng, C. Q., Feng, J. H., Fritsch, M., Fu, C. D., Gao, Y., Gao, Y. G., Garzia, I., Ge, P. T., Geng, C., Gersabeck, E. M., Gilman, A., Goetzen, K., Gong, L., Gong, W. X., Gradl, W., Greco, M., Gu, L. M., Gu, M. H., Gu, Y. T., Guan, C. Y., Guo, A. Q., Guo, L. B., Guo, R. P., Guo, Y. P., Guskov, A., Han, T. T., Han, W. Y., Hao, X. Q., Harris, F. A.
Format: Journal Article
Language:English
Published: 01-11-2021
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Summary:A bstract By analyzing 4 . 48 × 10 8 ψ (3686) events collected with the BESIII detector, we observe the decays χ cJ → $$ {nK}_S^0\overline{\Lambda} $$ nK S 0 Λ ¯ + c . c . ( J = 0, 1, 2) for the first time, via the radiative transition ψ (3686) → γχ cJ . The branching fractions are determined to be (6 . 65 ± 0 . 26 stat ± 0 . 41 syst ) × 10 − 4 , (1 . 66 ± 0 . 12 stat ± 0 . 12 syst ) × 10 − 4 , and (3 . 58 ± 0 . 16 stat ± 0 . 23 syst ) × 10 − 4 for J = 0, 1, and 2, respectively.
ISSN:1029-8479
1029-8479
DOI:10.1007/JHEP11(2021)217