Abstract
For the first time we search for the in at , 10.58, and 10.867 GeV with data samples of , , and , respectively, accumulated with the Belle detector at the KEKB asymmetric energy electron-positron collider. No significant signal is observed in the mass range between 3.8 and . The upper limit at 90% confidence level on the product of the Born cross section for and branching fraction for is determined to be at near 10.6 GeV.
Original language | English |
---|---|
Article number | 012012 |
Journal | Physical Review D |
Volume | 104 |
Issue number | 1 |
DOIs | |
Publication status | Published - 2021 Jul 1 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics
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Search for the in at near 10.6 GeV at Belle. / Jia, S.; Shen, C. P.; Adachi, I. et al.
In: Physical Review D, Vol. 104, No. 1, 012012, 01.07.2021.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Search for the in at near 10.6 GeV at Belle
AU - Jia, S.
AU - Shen, C. P.
AU - Adachi, I.
AU - Aihara, H.
AU - Al Said, S.
AU - Asner, D. M.
AU - Aushev, T.
AU - Ayad, R.
AU - Babu, V.
AU - Behera, P.
AU - Belous, K.
AU - Bennett, J.
AU - Bessner, M.
AU - Bhardwaj, V.
AU - Bhuyan, B.
AU - Bilka, T.
AU - Biswal, J.
AU - Bobrov, A.
AU - Bonvicini, G.
AU - Bozek, A.
AU - Bračko, M.
AU - Branchini, P.
AU - Browder, T. E.
AU - Budano, A.
AU - Campajola, M.
AU - Červenkov, D.
AU - Chang, M. C.
AU - Chang, P.
AU - Chekelian, V.
AU - Chen, A.
AU - Cheon, B. G.
AU - Chilikin, K.
AU - Cho, H. E.
AU - Cho, K.
AU - Cho, S. J.
AU - Choi, S. K.
AU - Choi, Y.
AU - Choudhury, S.
AU - Cinabro, D.
AU - Cunliffe, S.
AU - Das, S.
AU - Dash, N.
AU - De Nardo, G.
AU - De Pietro, G.
AU - Dhamija, R.
AU - Di Capua, F.
AU - Doležal, Z.
AU - Dong, T. V.
AU - Epifanov, D.
AU - Ferber, T.
AU - Fulsom, B. G.
AU - Garg, R.
AU - Gaur, V.
AU - Gabyshev, N.
AU - Garmash, A.
AU - Giri, A.
AU - Goldenzweig, P.
AU - Graziani, E.
AU - Gu, T.
AU - Gudkova, K.
AU - Hadjivasiliou, C.
AU - Halder, S.
AU - Hara, T.
AU - Hartbrich, O.
AU - Hayasaka, K.
AU - Hayashii, H.
AU - Hou, W. S.
AU - Hsu, C. L.
AU - Inami, K.
AU - Ishikawa, A.
AU - Itoh, R.
AU - Iwasaki, M.
AU - Iwasaki, Y.
AU - Jacobs, W. W.
AU - Jin, Y.
AU - Joo, K. K.
AU - Kaliyar, A. B.
AU - Kang, K. H.
AU - Karyan, G.
AU - Kato, Y.
AU - Kawasaki, T.
AU - Kiesling, C.
AU - Kim, D. Y.
AU - Kim, K. H.
AU - Kim, S. H.
AU - Kim, Y. K.
AU - Kinoshita, K.
AU - Kodyš, P.
AU - Konno, T.
AU - Korobov, A.
AU - Korpar, S.
AU - Kovalenko, E.
AU - Križan, P.
AU - Kroeger, R.
AU - Krokovny, P.
AU - Kuhr, T.
AU - Kumar, M.
AU - Kumara, K.
AU - Kuzmin, A.
AU - Kwon, Y. J.
AU - Lalwani, K.
AU - Lange, J. S.
AU - Laurenza, M.
AU - Lee, S. C.
AU - Li, C. H.
AU - Li, J.
AU - Li, L. K.
AU - Li, Y. B.
AU - Li Gioi, L.
AU - Libby, J.
AU - Lieret, K.
AU - Liventsev, D.
AU - Masuda, M.
AU - Matsuda, T.
AU - Matvienko, D.
AU - Merola, M.
AU - Metzner, F.
AU - Miyabayashi, K.
AU - Miyata, H.
AU - Mizuk, R.
AU - Mussa, R.
AU - Nakao, M.
AU - Natkaniec, Z.
AU - Natochii, A.
AU - Nayak, L.
AU - Niiyama, M.
AU - Nisar, N. K.
AU - Nishida, S.
AU - Nishimura, K.
AU - Ogawa, S.
AU - Ono, H.
AU - Oskin, P.
AU - Pakhlov, P.
AU - Pakhlova, G.
AU - Pardi, S.
AU - Park, S. H.
AU - Paul, S.
AU - Pedlar, T. K.
AU - Pestotnik, R.
AU - Piilonen, L. E.
AU - Podobnik, T.
AU - Popov, V.
AU - Prencipe, E.
AU - Prim, M. T.
AU - Rostomyan, A.
AU - Rout, N.
AU - Russo, G.
AU - Sahoo, D.
AU - Sandilya, S.
AU - Sangal, A.
AU - Santelj, L.
AU - Sanuki, T.
AU - Savinov, V.
AU - Schnell, G.
AU - Schwanda, C.
AU - Seino, Y.
AU - Senyo, K.
AU - Sevior, M. E.
AU - Shapkin, M.
AU - Sharma, C.
AU - Shiu, J. G.
AU - Shwartz, B.
AU - Sokolov, A.
AU - Solovieva, E.
AU - Starič, M.
AU - Stottler, Z. S.
AU - Sumihama, M.
AU - Takizawa, M.
AU - Tanida, K.
AU - Tao, Y.
AU - Tenchini, F.
AU - Trabelsi, K.
AU - Uglov, T.
AU - Unno, Y.
AU - Uno, K.
AU - Uno, S.
AU - Urquijo, P.
AU - Usov, Y.
AU - Vahsen, S. E.
AU - Van Tonder, R.
AU - Varner, G.
AU - Vinokurova, A.
AU - Waheed, E.
AU - Wang, C. H.
AU - Wang, E.
AU - Wang, M. Z.
AU - Wang, P.
AU - Watanuki, S.
AU - Werbycka, O.
AU - Won, E.
AU - Xu, X.
AU - Yabsley, B. D.
AU - Yan, W.
AU - Yang, S. B.
AU - Ye, H.
AU - Yelton, J.
AU - Yin, J. H.
AU - Yuan, C. Z.
AU - Yusa, Y.
AU - Zhang, Z. P.
AU - Zhilich, V.
AU - Zhukova, V.
N1 - Funding Information: Ministry of Education, Culture, Sports, Science and Technology Japan Society for the Promotion of Science Nagoya University Australian Research Council Bundesministerium für Bildung und Forschung Austrian Science Fund National Natural Science Foundation of China Key Research Program of Frontier Sciences Chinese Academy of Sciences CAS Center for Excellence in Particle Physics Shanghai Pujiang Program Science and Technology Commission of Shanghai Municipality Ministerstvo Školství, Mládeže a T?lovýchovy H2020 European Research Council Carl-Zeiss-Stiftung Deutsche Forschungsgemeinschaft Excellence Cluster Universe Volkswagen Foundation Department of Atomic Energy, Government of India Department of Science and Technology, Ministry of Science and Technology, India Istituto Nazionale di Fisica Nucleare Sezione di Padova National Research Foundation of Korea Radiation Science Research Institute Foreign Large-size Research Facility Application Supporting project Korea Institute of Science and Technology Information KREONET/GLORIAD Ministerstwo Nauki i Szkolnictwa Wy?szego National Science Centre Ministry of Science and Higher Education of the Russian Federation HSE University Basic Research Program University of Tabuk Javna Agencija za Raziskovalno Dejavnost RS Ikerbasque, Basque Foundation for Science Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung Ministry of Education Ministry of Science and Technology, Taiwan U.S. Department of Energy National Science Foundation Funding Information: We thank the KEKB group for the excellent operation of the accelerator; the KEK cryogenics group for the efficient operation of the solenoid; and the KEK computer group, and the Pacific Northwest National Laboratory (PNNL) Environmental Molecular Sciences Laboratory (EMSL) computing group for strong computing support; and the National Institute of Informatics, and Science Information NETwork 5 (SINET5) for valuable network support. We acknowledge support from the Ministry of Education, Culture, Sports, Science, and Technology (MEXT) of Japan, the Japan Society for the Promotion of Science (JSPS), and the Tau-Lepton Physics Research Center of Nagoya University; the Australian Research Council including Grants No. DP180102629, No. DP170102389, No. DP170102204, No. DP150103061, No. FT130100303; Austrian Federal Ministry of Education, Science and Research (FWF) and FWF Austrian Science Fund No. P 31361-N36; the National Natural Science Foundation of China under Contracts No. 11435013, No. 11475187, No. 11521505, No. 11575017, No. 11675166, No. 11705209; No. 11761141009; No. 11975076; No. 12042509; No. 12005040; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS), Grant No. QYZDJ-SSW-SLH011; the CAS Center for Excellence in Particle Physics (CCEPP); the Shanghai Pujiang Program under Grant No. 18PJ1401000; the Shanghai Science and Technology Committee (STCSM) under Grant No. 19ZR1403000; the Ministry of Education, Youth and Sports of the Czech Republic under Contract No. LTT17020; Horizon 2020 ERC Advanced Grant No. 884719 and ERC Starting Grant No. 947006 “InterLeptons” (European Union); the Carl Zeiss Foundation, the Deutsche Forschungsgemeinschaft, the Excellence Cluster Universe, and the VolkswagenStiftung; the Department of Atomic Energy (Project Identification No. RTI 4002) and the Department of Science and Technology of India; the Istituto Nazionale di Fisica Nucleare of Italy; National Research Foundation (NRF) of Korea Grants No. 2016R1D1A1B01010135, No. 2016R1D1A1B02012900, No. 2018R1A2B3003643, No. 2018R1A6A1A06024970, No. 2018R1D1A1B07047294, No. 2019K1A3A7A09033840, No. 2019R1I1A3A01058933; Radiation Science Research Institute, Foreign Large-size Research Facility Application Supporting project, the Global Science Experimental Data Hub Center of the Korea Institute of Science and Technology Information and KREONET/GLORIAD; the Polish Ministry of Science and Higher Education and the National Science Center; the Ministry of Science and Higher Education of the Russian Federation, Agreement 14.W03.31.0026, and the HSE University Basic Research Program, Moscow; University of Tabuk research Grants No. S-1440-0321, No. S-0256-1438, and No. S-0280-1439 (Saudi Arabia); the Slovenian Research Agency Grants No. J1-9124 and No. P1-0135; Ikerbasque, Basque Foundation for Science, Spain; the Swiss National Science Foundation; the Ministry of Education and the Ministry of Science and Technology of Taiwan; and the United States Department of Energy and the National Science Foundation. Publisher Copyright: © 2021 Published by the American Physical Society
PY - 2021/7/1
Y1 - 2021/7/1
N2 - For the first time we search for the in at , 10.58, and 10.867 GeV with data samples of , , and , respectively, accumulated with the Belle detector at the KEKB asymmetric energy electron-positron collider. No significant signal is observed in the mass range between 3.8 and . The upper limit at 90% confidence level on the product of the Born cross section for and branching fraction for is determined to be at near 10.6 GeV.
AB - For the first time we search for the in at , 10.58, and 10.867 GeV with data samples of , , and , respectively, accumulated with the Belle detector at the KEKB asymmetric energy electron-positron collider. No significant signal is observed in the mass range between 3.8 and . The upper limit at 90% confidence level on the product of the Born cross section for and branching fraction for is determined to be at near 10.6 GeV.
UR - http://www.scopus.com/inward/record.url?scp=85112771353&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85112771353&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.104.012012
DO - 10.1103/PhysRevD.104.012012
M3 - Article
AN - SCOPUS:85112771353
SN - 2470-0010
VL - 104
JO - Physical Review D
JF - Physical Review D
IS - 1
M1 - 012012
ER -