Abstract
We report searches for B0→invisible and B0→invisible+γ decays, where the energy of the photon is required to be larger than 0.5 GeV. These results are obtained from a 711 fb-1 data sample that contains 772×106BB¯ pairs and was collected near the ϒ(4S) resonance with the Belle detector at the KEKB e+e- collider. We observe no significant signal for either decay and set upper limits on their branching fractions at 90% confidence level of B(B0→invisible)<7.8×10-5 and B(B0→invisible+γ)<1.6×10-5.
| Original language | English |
|---|---|
| Article number | 012003 |
| Journal | Physical Review D |
| Volume | 102 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 2020 Jul 1 |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)
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Search for B0 decays to invisible final states (+γ) at Belle. / Belle Collaboration.
In: Physical Review D, Vol. 102, No. 1, 012003, 01.07.2020.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Search for B0 decays to invisible final states (+γ) at Belle
AU - Belle Collaboration
AU - Ku, Y.
AU - Chang, P.
AU - Adachi, I.
AU - Adamczyk, K.
AU - Aihara, H.
AU - Asner, D. M.
AU - Aushev, T.
AU - Ayad, R.
AU - Behera, P.
AU - Beleño, C.
AU - Bennett, J.
AU - Bhardwaj, V.
AU - Bilka, T.
AU - Biswal, J.
AU - Bonvicini, G.
AU - Bozek, A.
AU - Bračko, M.
AU - Chang, M. C.
AU - Chekelian, V.
AU - Chilikin, K.
AU - Cho, K.
AU - Choi, S. K.
AU - Choi, Y.
AU - Cinabro, D.
AU - Cunliffe, S.
AU - Dash, N.
AU - De Nardo, G.
AU - Dong, T. V.
AU - Eidelman, S.
AU - Epifanov, D.
AU - Fast, J. E.
AU - Fulsom, B. G.
AU - Garg, R.
AU - Gaur, V.
AU - Gabyshev, N.
AU - Garmash, A.
AU - Goldenzweig, P.
AU - Grzymkowska, O.
AU - Guan, Y.
AU - Hartbrich, O.
AU - Hayasaka, K.
AU - Hayashii, H.
AU - Hernandez Villanueva, M.
AU - Higuchi, T.
AU - Hou, W. S.
AU - Hsu, C. L.
AU - Huang, K.
AU - Inami, K.
AU - Inguglia, G.
AU - Won, E.
N1 - 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, and No. FT130100303; Austrian Science Fund (FWF); the National Natural Science Foundation of China under Contracts No. 11435013, No. 11475187, No. 11521505, No. 11575017, No. 11675166, and No. 11705209; 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 Ministry of Education, Youth and Sports of the Czech Republic under Contract No. LTT17020; the Carl Zeiss Foundation, the Deutsche Forschungsgemeinschaft, the Excellence Cluster Universe, and the VolkswagenStiftung; 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. 2018R1A4A1025334, No. 2018R1A6A1A06024970, No. 2018R1D1A1B07047294, No. 2019K1A3A7A09033840, and 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 No. 14.W03.31.0026; University of Tabuk research Grants No. S-1440-0321, No. S-0256-1438, and No. S-0280-1439 (Saudi Arabia); the Slovenian Research Agency; 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. 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, and No.?FT130100303; Austrian Science Fund (FWF); the National Natural Science Foundation of China under Contracts No.?11435013, No.?11475187, No.?11521505, No.?11575017, No.?11675166, and No.?11705209; 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 Ministry of Education, Youth and Sports of the Czech Republic under Contract No.?LTT17020; the Carl Zeiss Foundation, the Deutsche Forschungsgemeinschaft, the Excellence Cluster Universe, and the VolkswagenStiftung; 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.?2018R1A4A1025334, No.?2018R1A6A1A06024970, No.?2018R1D1A1B07047294, No.?2019K1A3A7A09033840, and 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 No.?14.W03.31.0026; University of Tabuk research Grants No.?S-1440-0321, No.?S-0256-1438, and No.?S-0280-1439 (Saudi Arabia); the Slovenian Research Agency; 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: © 2020 authors.
PY - 2020/7/1
Y1 - 2020/7/1
N2 - We report searches for B0→invisible and B0→invisible+γ decays, where the energy of the photon is required to be larger than 0.5 GeV. These results are obtained from a 711 fb-1 data sample that contains 772×106BB¯ pairs and was collected near the ϒ(4S) resonance with the Belle detector at the KEKB e+e- collider. We observe no significant signal for either decay and set upper limits on their branching fractions at 90% confidence level of B(B0→invisible)<7.8×10-5 and B(B0→invisible+γ)<1.6×10-5.
AB - We report searches for B0→invisible and B0→invisible+γ decays, where the energy of the photon is required to be larger than 0.5 GeV. These results are obtained from a 711 fb-1 data sample that contains 772×106BB¯ pairs and was collected near the ϒ(4S) resonance with the Belle detector at the KEKB e+e- collider. We observe no significant signal for either decay and set upper limits on their branching fractions at 90% confidence level of B(B0→invisible)<7.8×10-5 and B(B0→invisible+γ)<1.6×10-5.
UR - http://www.scopus.com/inward/record.url?scp=85092362661&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.102.012003
DO - 10.1103/PhysRevD.102.012003
M3 - Article
AN - SCOPUS:85092362661
VL - 102
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 1
M1 - 012003
ER -