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The Belle Collaboration


Search for the decay B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} at the Belle experiment

T. V. Dong Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) and Institute of Modern Physics, Fudan University, Shanghai 200443    T. Luo Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) and Institute of Modern Physics, Fudan University, Shanghai 200443    I. Adachi High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    H. Aihara Department of Physics, University of Tokyo, Tokyo 113-0033    D. M. Asner Brookhaven National Laboratory, Upton, New York 11973    H. Atmacan University of Cincinnati, Cincinnati, Ohio 45221    V. Aulchenko Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    T. Aushev National Research University Higher School of Economics, Moscow 101000    R. Ayad Department of Physics, Faculty of Science, University of Tabuk, Tabuk 71451    V. Babu Deutsches Elektronen–Synchrotron, 22607 Hamburg    S. Bahinipati Indian Institute of Technology Bhubaneswar, Satya Nagar 751007    P. Behera Indian Institute of Technology Madras, Chennai 600036    K. Belous Institute for High Energy Physics, Protvino 142281    F. Bernlochner University of Bonn, 53115 Bonn    M. Bessner University of Hawaii, Honolulu, Hawaii 96822    B. Bhuyan Indian Institute of Technology Guwahati, Assam 781039    T. Bilka Faculty of Mathematics and Physics, Charles University, 121 16 Prague    J. Biswal J. Stefan Institute, 1000 Ljubljana    A. Bobrov Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    A. Bozek H. Niewodniczanski Institute of Nuclear Physics, Krakow 31-342    M. Bračko Faculty of Chemistry and Chemical Engineering, University of Maribor, 2000 Maribor J. Stefan Institute, 1000 Ljubljana    P. Branchini INFN - Sezione di Roma Tre, I-00146 Roma    T. E. Browder University of Hawaii, Honolulu, Hawaii 96822    A. Budano INFN - Sezione di Roma Tre, I-00146 Roma    M. Campajola INFN - Sezione di Napoli, I-80126 Napoli Università di Napoli Federico II, I-80126 Napoli    D. Červenkov Faculty of Mathematics and Physics, Charles University, 121 16 Prague    M.-C. Chang Department of Physics, Fu Jen Catholic University, Taipei 24205    P. Chang Department of Physics, National Taiwan University, Taipei 10617    A. Chen National Central University, Chung-li 32054    B. G. Cheon Department of Physics and Institute of Natural Sciences, Hanyang University, Seoul 04763    K. Chilikin P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991    H. E. Cho Department of Physics and Institute of Natural Sciences, Hanyang University, Seoul 04763    K. Cho Korea Institute of Science and Technology Information, Daejeon 34141    S.-J. Cho Yonsei University, Seoul 03722    S.-K. Choi Gyeongsang National University, Jinju 52828    Y. Choi Sungkyunkwan University, Suwon 16419    S. Choudhury Indian Institute of Technology Hyderabad, Telangana 502285    D. Cinabro Wayne State University, Detroit, Michigan 48202    S. Cunliffe Deutsches Elektronen–Synchrotron, 22607 Hamburg    T. Czank Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa 277-8583    S. Das Malaviya National Institute of Technology Jaipur, Jaipur 302017    G. De Nardo INFN - Sezione di Napoli, I-80126 Napoli Università di Napoli Federico II, I-80126 Napoli    G. De Pietro INFN - Sezione di Roma Tre, I-00146 Roma    R. Dhamija Indian Institute of Technology Hyderabad, Telangana 502285    F. Di Capua INFN - Sezione di Napoli, I-80126 Napoli Università di Napoli Federico II, I-80126 Napoli    J. Dingfelder University of Bonn, 53115 Bonn    Z. Doležal Faculty of Mathematics and Physics, Charles University, 121 16 Prague    S. Dubey University of Hawaii, Honolulu, Hawaii 96822    D. Epifanov Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    T. Ferber Deutsches Elektronen–Synchrotron, 22607 Hamburg    D. Ferlewicz School of Physics, University of Melbourne, Victoria 3010    B. G. Fulsom Pacific Northwest National Laboratory, Richland, Washington 99352    R. Garg Panjab University, Chandigarh 160014    V. Gaur Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061    N. Gabyshev Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    A. Garmash Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    A. Giri Indian Institute of Technology Hyderabad, Telangana 502285    P. Goldenzweig Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe    E. Graziani INFN - Sezione di Roma Tre, I-00146 Roma    T. Gu University of Pittsburgh, Pittsburgh, Pennsylvania 15260    K. Gudkova Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    T. Hara High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    O. Hartbrich University of Hawaii, Honolulu, Hawaii 96822    K. Hayasaka Niigata University, Niigata 950-2181    M. Hernandez Villanueva Deutsches Elektronen–Synchrotron, 22607 Hamburg    W.-S. Hou Department of Physics, National Taiwan University, Taipei 10617    C.-L. Hsu School of Physics, University of Sydney, New South Wales 2006    K. Inami Graduate School of Science, Nagoya University, Nagoya 464-8602    G. Inguglia Institute of High Energy Physics, Vienna 1050    A. Ishikawa High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    R. Itoh High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    M. Iwasaki Osaka City University, Osaka 558-8585    W. W. Jacobs Indiana University, Bloomington, Indiana 47408    E.-J. Jang Gyeongsang National University, Jinju 52828    S. Jia Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) and Institute of Modern Physics, Fudan University, Shanghai 200443    Y. Jin Department of Physics, University of Tokyo, Tokyo 113-0033    K. K. Joo Chonnam National University, Gwangju 61186    J. Kahn Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe    K. H. Kang Kyungpook National University, Daegu 41566    H. Kichimi High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801    C. Kiesling Max-Planck-Institut für Physik, 80805 München    C. H. Kim Department of Physics and Institute of Natural Sciences, Hanyang University, Seoul 04763    D. Y. Kim Soongsil University, Seoul 06978    S. H. Kim Seoul National University, Seoul 08826    Y.-K. Kim Yonsei University, Seoul 03722    T. D. Kimmel Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061    P. Kodyš Faculty of Mathematics and Physics, Charles University, 121 16 Prague    T. Konno Kitasato University, Sagamihara 252-0373    A. Korobov Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    S. Korpar Faculty of Chemistry and Chemical Engineering, University of Maribor, 2000 Maribor J. Stefan Institute, 1000 Ljubljana    E. Kovalenko Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    P. Križan Faculty of Mathematics and Physics, University of Ljubljana, 1000 Ljubljana J. Stefan Institute, 1000 Ljubljana    R. Kroeger University of Mississippi, University, Mississippi 38677    P. Krokovny Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    T. Kuhr Ludwig Maximilians University, 80539 Munich    R. Kulasiri Kennesaw State University, Kennesaw, Georgia 30144    M. Kumar Malaviya National Institute of Technology Jaipur, Jaipur 302017    R. Kumar Punjab Agricultural University, Ludhiana 141004    K. Kumara Wayne State University, Detroit, Michigan 48202    A. Kuzmin Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    Y.-J. Kwon Yonsei University, Seoul 03722    M. Laurenza INFN - Sezione di Roma Tre, I-00146 Roma Dipartimento di Matematica e Fisica, Università di Roma Tre, I-00146 Roma    S. C. Lee Kyungpook National University, Daegu 41566    J. Li Kyungpook National University, Daegu 41566    L. K. Li University of Cincinnati, Cincinnati, Ohio 45221    Y. B. Li Peking University, Beijing 100871    L. Li Gioi Max-Planck-Institut für Physik, 80805 München    J. Libby Indian Institute of Technology Madras, Chennai 600036    K. Lieret Ludwig Maximilians University, 80539 Munich    D. Liventsev Wayne State University, Detroit, Michigan 48202 High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801    C. MacQueen School of Physics, University of Melbourne, Victoria 3010    M. Masuda Earthquake Research Institute, University of Tokyo, Tokyo 113-0032 Research Center for Nuclear Physics, Osaka University, Osaka 567-0047    T. Matsuda University of Miyazaki, Miyazaki 889-2192    D. Matvienko Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090 P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991    M. Merola INFN - Sezione di Napoli, I-80126 Napoli Università di Napoli Federico II, I-80126 Napoli    F. Metzner Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe    K. Miyabayashi Nara Women’s University, Nara 630-8506    R. Mizuk P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991 National Research University Higher School of Economics, Moscow 101000    G. B. Mohanty Tata Institute of Fundamental Research, Mumbai 400005    M. Nakao High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    A. Natochii University of Hawaii, Honolulu, Hawaii 96822    L. Nayak Indian Institute of Technology Hyderabad, Telangana 502285    M. Niiyama Kyoto Sangyo University, Kyoto 603-8555    N. K. Nisar Brookhaven National Laboratory, Upton, New York 11973    S. Nishida High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    K. Nishimura University of Hawaii, Honolulu, Hawaii 96822    S. Ogawa Toho University, Funabashi 274-8510    H. Ono Nippon Dental University, Niigata 951-8580 Niigata University, Niigata 950-2181    Y. Onuki Department of Physics, University of Tokyo, Tokyo 113-0033    P. Oskin P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991    P. Pakhlov P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991 Moscow Physical Engineering Institute, Moscow 115409    G. Pakhlova National Research University Higher School of Economics, Moscow 101000 P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991    S. Pardi INFN - Sezione di Napoli, I-80126 Napoli    H. Park Kyungpook National University, Daegu 41566    S.-H. Park High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801    S. Patra Indian Institute of Science Education and Research Mohali, SAS Nagar, 140306    S. Paul Department of Physics, Technische Universität München, 85748 Garching Max-Planck-Institut für Physik, 80805 München    T. K. Pedlar Luther College, Decorah, Iowa 52101    R. Pestotnik J. Stefan Institute, 1000 Ljubljana    L. E. Piilonen Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061    T. Podobnik Faculty of Mathematics and Physics, University of Ljubljana, 1000 Ljubljana J. Stefan Institute, 1000 Ljubljana    V. Popov National Research University Higher School of Economics, Moscow 101000    E. Prencipe Forschungszentrum Jülich, 52425 Jülich    M. T. Prim University of Bonn, 53115 Bonn    A. Rostomyan Deutsches Elektronen–Synchrotron, 22607 Hamburg    N. Rout Indian Institute of Technology Madras, Chennai 600036    G. Russo Università di Napoli Federico II, I-80126 Napoli    D. Sahoo Tata Institute of Fundamental Research, Mumbai 400005    S. Sandilya Indian Institute of Technology Hyderabad, Telangana 502285    A. Sangal University of Cincinnati, Cincinnati, Ohio 45221    L. Santelj Faculty of Mathematics and Physics, University of Ljubljana, 1000 Ljubljana J. Stefan Institute, 1000 Ljubljana    T. Sanuki Department of Physics, Tohoku University, Sendai 980-8578    V. Savinov University of Pittsburgh, Pittsburgh, Pennsylvania 15260    G. Schnell Department of Physics, University of the Basque Country UPV/EHU, 48080 Bilbao IKERBASQUE, Basque Foundation for Science, 48013 Bilbao    J. Schueler University of Hawaii, Honolulu, Hawaii 96822    C. Schwanda Institute of High Energy Physics, Vienna 1050    Y. Seino Niigata University, Niigata 950-2181    K. Senyo Yamagata University, Yamagata 990-8560    M. E. Sevior School of Physics, University of Melbourne, Victoria 3010    M. Shapkin Institute for High Energy Physics, Protvino 142281    C. Sharma Malaviya National Institute of Technology Jaipur, Jaipur 302017    J.-G. Shiu Department of Physics, National Taiwan University, Taipei 10617    F. Simon Max-Planck-Institut für Physik, 80805 München    E. Solovieva P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991    M. Starič J. Stefan Institute, 1000 Ljubljana    M. Sumihama Gifu University, Gifu 501-1193    K. Sumisawa High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    T. Sumiyoshi Tokyo Metropolitan University, Tokyo 192-0397    M. Takizawa Showa Pharmaceutical University, Tokyo 194-8543 J-PARC Branch, KEK Theory Center, High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 Meson Science Laboratory, Cluster for Pioneering Research, RIKEN, Saitama 351-0198    U. Tamponi INFN - Sezione di Torino, I-10125 Torino    K. Tanida Advanced Science Research Center, Japan Atomic Energy Agency, Naka 319-1195    F. Tenchini Deutsches Elektronen–Synchrotron, 22607 Hamburg    K. Trabelsi Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay    M. Uchida Tokyo Institute of Technology, Tokyo 152-8550    Y. Unno Department of Physics and Institute of Natural Sciences, Hanyang University, Seoul 04763    S. Uno High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193    R. Van Tonder University of Bonn, 53115 Bonn    G. Varner University of Hawaii, Honolulu, Hawaii 96822    K. E. Varvell School of Physics, University of Sydney, New South Wales 2006    E. Waheed High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801    C. H. Wang National United University, Miao Li 36003    E. Wang University of Pittsburgh, Pittsburgh, Pennsylvania 15260    P. Wang Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049    M. Watanabe Niigata University, Niigata 950-2181    S. Watanuki Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay    O. Werbycka H. Niewodniczanski Institute of Nuclear Physics, Krakow 31-342    E. Won Korea University, Seoul 02841    B. D. Yabsley School of Physics, University of Sydney, New South Wales 2006    W. Yan Department of Modern Physics and State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026    S. B. Yang Korea University, Seoul 02841    H. Ye Deutsches Elektronen–Synchrotron, 22607 Hamburg    J. H. Yin Korea University, Seoul 02841    Z. P. Zhang Department of Modern Physics and State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026    V. Zhilich Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090 Novosibirsk State University, Novosibirsk 630090    V. Zhukova P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
Abstract

This letter presents a search for the rare flavor-changing neutral current process B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} using data taken with the Belle detector at the KEKB asymmetric energy e+ee^{+}e^{-} collider. The analysis is based on the entire Υ(4S)\Upsilon(4S) resonance data sample of 711 fb1\rm fb^{-1}, corresponding to 772×106BB¯772\times 10^{6}B\bar{B} pairs. In our search we fully reconstruct the companion BB meson produced in the process e+eΥ(4S)BB¯e^{+}e^{-}\rightarrow\Upsilon(4S)\rightarrow B\bar{B} from its hadronic decay modes, and look for the decay B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} in the rest of the event. No evidence for a signal is found. We report an upper limit on the branching fraction (B0K0τ+τ)<3.1×103\mathcal{B}({B^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-}})<3.1\times 10^{-3} at 90% confidence level. This is the first direct limit on (B0K0τ+τ)\mathcal{B}({B^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-}}).

pacs:
3.20.He, 14.40.Nd

The decay B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} (charge-conjugate processes are implied throughout this letter) is of interest for the testing of Lepton Flavor Universality (LFU) and for searches of physics beyond the Standard Model (SM). This decay is highly suppressed in the SM and can only proceed via a flavor-changing neutral current, with a predicted branching fraction of order 𝒪(107)\mathcal{O}(10^{-7}) [1]. The branching fraction can be enhanced if new physics (NP) effects contribute [2, 3, 4, 5]. The flavor-changing neutral current processes such as B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} can provide very powerful tests for the SM and its extensions. In particular, the decay is a third-generation equivalent of the B0K0+B^{0}\rightarrow K^{\ast 0}\ell^{+}\ell^{-} decay, where \ell is an electron or a muon. Hence, compared with electron and muon modes, the decay is expected to be more sensitive to new physics in a model which has a coupling proportionate to the particle mass [6] or only couples to the third generation [7].

Semileptonic BB decay measurements in recent years show significant deviations from SM expectations, for both charged and neutral current transitions. The first type of transition has been measured in the decay bcν¯b\rightarrow c\ell\bar{\nu}_{\ell} via R(D())=[(BD()τ+ντ)]/[(BD()+ν)]R(D^{(*)})=[\mathcal{B}(B\rightarrow D^{(*)}\tau^{+}\nu_{\tau})]/[\mathcal{B}(B\rightarrow D^{(*)}\ell^{+}\nu_{\ell})] by the BaBar [8, 9], Belle [10, 11, 12, 13] and LHCb [14, 15] experiments. While these decays are tree-level processes, which are not very sensitive to NP, the measured results show a deviation of about three standard deviations, 3σ\sigma, from the SM predictions (combined significance) [16]. The neutral current transition bs+b\rightarrow s\ell^{+}\ell^{-} is highly suppressed in the SM and very sensitive to NP. The LFU ratio between muon and electron in the decay mode BK()+B\rightarrow K^{(*)}\ell^{+}\ell^{-} as measured by Belle [17, 18, 19] and BaBar [20] are consistent with the SM, while LHCb result [21, 22, 23] is 3.1σ\sigma lower than the SM prediction. Many theoretical models are introduced to explain these anomalies such as the NP contribution to the Wilson coefficients [3, 4] and the leptoquark model [5]. These approaches lead to an enhancement of the bsτ+τb\rightarrow s\tau^{+}\tau^{-} branching fraction up to 11-5×1045\times 10^{-4}, 3 orders of magnitude larger than the SM predictions. The predicted branching fraction of B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} is larger than that of B+K+τ+τB^{+}\rightarrow K^{+}\tau^{+}\tau^{-} as shown in Ref. [3].

The presence of at least two neutrinos in the final state originating from the decays of τ+τ\tau^{+}\tau^{-} pair make analysis of the decay challenging. To date only a search for the decay B+K+τ+τB^{+}\rightarrow K^{+}\tau^{+}\tau^{-} has been conducted by the BaBar collaboration setting an upper limit (B+K+τ+τ)<2.25×103\mathcal{B}(B^{+}\rightarrow K^{+}\tau^{+}\tau^{-})<2.25\times 10^{-3} at 90% confidence level (CL) [24].

In this letter, we present the first search for the rare decay B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-}. Our analysis is based on the complete data set collected at the center of mass (c.m.) energy equal to the Υ(4S)\Upsilon(4S) resonance mass by the Belle detector [25] at the KEKB asymmetric-energy e+ee^{+}e^{-} collider [26]. This data sample corresponds to an integrated luminosity of 711 fb1\rm fb^{-1}, containing 772×106BB¯772\times 10^{6}B\bar{B} pairs. We use a full reconstruction technique [27] in this analysis where the companion BB meson in the process e+eΥ(4S)BB¯e^{+}e^{-}\rightarrow\Upsilon(4S)\rightarrow B\bar{B} is reconstructed in hadronic decay modes, referred to as BtagB_{\rm tag}. We then search for the signal BB meson, BsigB_{\rm sig}, in the rest of the event not used in the BtagB_{\rm tag} reconstruction.

The Belle detector [25] is a large-solid-angle magnetic spectrometer consisting of a silicon vertex detector (SVD), a 50-layer central drift chamber (CDC), an array of aerogel threshold Cherenkov counters (ACC), a barrel-like arrangement of time-of-flight scintillation counters (TOF), and an electromagnetic calorimeter comprised of CsI(Tl) crystals (ECL). All these components are located inside a superconducting solenoid coil that provides a 1.5 T magnetic field. An iron flux-return located outside of the coil is instrumented with resistive plate chambers to detect KL0K_{L}^{0} mesons and to identify muons (KLM).

We use Monte Carlo (MC) simulation samples, generated with EvtGen [28], to optimize the signal selection, determine the selection efficiencies, as well as to obtain the signal and background fitting models. The detector response is simulated using GEANT3 [29]. Simulated events are overlaid with random trigger data taken for each run period to reproduce the effect of beam-associated backgrounds. A signal sample containing 50 million Υ(4S)B0B¯0\Upsilon(4S)\rightarrow B^{0}\bar{B}^{0} events is generated where one BB decays to all possible final states, according to its measured or estimated branching fractions [30], and the other decays via B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-}, using the model described in Ref. [31]. Background MC samples consist of B+BB^{+}B^{-}, B0B¯0B^{0}\bar{B}^{0}, and continuum e+eqq¯e^{+}e^{-}\rightarrow q\bar{q} (q=u,d,s,cq=u,d,s,c), where the size of each sample is six times larger than that of collision data. Rare BB meson decay processes such as charmless hadronic, radiative, and electroweak decays are simulated separately in a sample designated Rare B. Semileptonic buνb\rightarrow u\ell\nu decays are simulated in a dedicated uνu\ell\nu sample. The sizes of the RareBRare~{}B and uνu\ell\nu samples are 50 and 20 times larger than that of collision data, respectively.

A candidate BtagB_{\rm tag} meson is reconstructed in one of the 489 hadronic decay channel using a hierarchical NeuroBayes-based (NB) full-reconstruction algorithm [27]. In this algorithm, the continuum backgrounds are suppressed by employed event shape variables such as the polar angle of BtagB_{\rm tag}, the cosine of the angle between the thrust axis [32] and z-direction, and the modified second Fox-Wolfram moment [33]. All the input variables which used during the reconstruction are mapped to a single classifier output, 𝒪NB{\cal O}_{\rm NB}, which represents the quality of BtagB_{\rm tag}, ranges from zero for combinatorial background and continuum events to unity for an unambiguous BtagB_{\rm tag}. Event selection also exploits the energy difference ΔE=EBtagEcm/2\Delta E=E_{\rm Btag}-E_{\rm cm}/2 and the beam-energy-constrained mass Mbc=(Ecm/2)2/c4|pBtag|2/c2M_{\rm bc}=\sqrt{(E_{\rm cm}/2)^{2}/c^{4}-|\vec{p}_{\rm Btag}|^{2}/c^{2}}, where EcmE_{\rm cm} is the e+ee^{+}e^{-} energy, and EBtagE_{\rm Btag} and pBtag\vec{p}_{\rm Btag} are the reconstructed energy and momentum of the BtagB_{\rm tag} candidate, respectively. All the quantities are measured in the c.m. frame. We require each BtagB_{\rm tag} candidate to satisfy ln(𝒪NB)>7\ln({\cal O}_{\rm NB})>-7, |ΔE|<0.06|\Delta E|<0.06 GeV, and 5.275<Mbc<5.2905.275<M_{\rm bc}<5.290 GeV/c2c^{2}. The net tagging efficiency which is defined as number of truly reconstructed B-tag divided for total number of generated event is 0.24%. It is slightly higher than that reported in Ref. [27], due to lower average particle multiplicity in this signal sample compared to generic sample. The signal side of the B0K0ττ+B^{0}\rightarrow K^{\ast 0}\tau^{-}\tau^{+} sample contains of leptons and only two hadron tracks. The possibility of the interference from signal side to the tag side reconstruction is lower than that of the generic samples, where both BB mesons decay generically. The tagging efficiency is calibrated by comparing the known branching fraction from PDG [30] of the decays BD()νB\rightarrow D^{(*)}\ell\nu_{\ell} and the measured values which use this hadron tag reconstruction method [34].

For events where a BtagB_{\rm tag} is reconstructed, we search for the decay B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} in the rest of the event. The remaining tracks are examined to remove duplicate ones due to the curling of low transverse momentum particles (pt<0.3p_{t}<0.3 GeV/cc). A pair of tracks is considered as duplicate if the cosine of the angle between them is either larger than 0.9 or smaller than 0.1, and the difference in transverse momentum is less than 0.1 GeV/cc. All tracks are constrained to originate from the interaction point (IP) by the requirements |dr|<2|dr|<2 cm and |dz|<4|dz|<4 cm, where drdr and dzdz are the impact parameter with respect to IP in the transverse and longitudinal directions, respectively. We select events as signal candidates if there are four remaining tracks with zero net charge. The number of signal candidates doubles after removing duplicate tracks.

We reconstruct candidate K0K^{\ast 0} mesons from K0K+πK^{\ast 0}\rightarrow K^{+}\pi^{-} decays using two of the four remaining tracks. We identify kaons and pions based on combined information from the CDC, ACC, and TOF [35]. A charged track is identified as a kaon if the likelihood ratio K=K/(K+π)>0.6\mathcal{R}_{K}=\mathcal{L}_{K}/(\mathcal{L}_{K}+\mathcal{L}_{\pi})>0.6, and as a pion if K<0.4\mathcal{R}_{K}<0.4, where i\mathcal{L}_{i} is the PID likelihood for the particle type ii. The momenta of K+K^{+} and π\pi^{-} candidates are required to be greater than 0.1 GeV/cc. The flavor of the reconstructed K0K^{\ast 0} and hence the corresponding flavor of BsigB_{\rm sig} is required to be opposite to that of BtagB_{\rm tag}. This requirement rejects 20% of the events. We fit the vertex for K0K^{\ast 0} candidates, and reject candidates if the vertex fit fails. If more than one K0K^{\ast 0} candidate is successfully reconstructed, the one having the reconstructed mass closest to the known K0K^{\ast 0} mass is retained. We require the mass of the reconstructed K0K^{\ast 0} candidate to be in the range [0.8, 1.0] GeV/c2c^{2}, which is approximately twice the decay width of K0K^{\ast 0}. We consider three τ\tau decay modes in this analysis: τeν¯eντ\tau^{-}\rightarrow e^{-}\bar{\nu}_{e}\nu_{\tau}, τμν¯μντ\tau^{-}\rightarrow\mu^{-}\bar{\nu}_{\mu}\nu_{\tau}, and τπντ\tau^{-}\rightarrow\pi^{-}\nu_{\tau}, resulting in six different decay topologies: K0e+eK^{\ast 0}e^{+}e^{-}, K0eμ±K^{\ast 0}e^{\mp}\mu^{\pm}, K0μ+μK^{\ast 0}\mu^{+}\mu^{-}, K0eπ±K^{\ast 0}e^{\mp}\pi^{\pm}, K0μπ±K^{\ast 0}\mu^{\mp}\pi^{\pm}, and K0π+πK^{\ast 0}\pi^{+}\pi^{-}. We regard the two remaining tracks not used in the BtagB_{\rm tag} or the K0K^{\ast 0} candidates as τ\tau decay products. The reconstructed mass of these two tracks is required to be less than 2.5 GeV/c2c^{2}.

All the tracks and clusters in a signal event are used for the reconstruction of BtagB_{\rm tag} and BsigB_{\rm sig}. However, there are still tracks and clusters from beam background and possible duplicate tracking reconstruction. We require that there be no extra π0\pi^{0} nor KS0K_{S}^{0} candidates, and at most one KL0K_{L}^{0} candidate cluster, to allow for beam-associated backgrounds or electronic noise. We reconstruct KL0K_{L}^{0} candidates based on the hit patterns in the KLM subdetector not associated with any charged track. A π0\pi^{0} candidate is reconstructed from π0γγ\pi^{0}\rightarrow\gamma\gamma in which neither daughter photon is included in the reconstructed BtagB_{\rm tag} and whose reconstructed mass is within 25 MeV/c2c^{2} of the nominal π0\pi^{0} mass [30], corresponding to 3σ3\sigma of the π0\pi^{0} mass resolution. Energy of photon candidates must exceed 50 MeV and we require their shower shape, characterized as the ratio of total energy detected in a 3×33\times 3 versus 5×55\times 5 array of ECL crystals in which the center crystal has the maximum detected energy, to be larger than 0.75. We reconstruct candidate KS0K_{S}^{0} from KS0π+πK_{S}^{0}\rightarrow\pi^{+}\pi^{-} decays, where the reconstructed mass is within 15 MeV/c2c^{2} of the nominal mass, corresponding to 3σ3\sigma of KS0K_{S}^{0} mass resolution.

We determine the number of signal candidates by fitting the distribution of extra calorimeter energy, EECLextraE_{\rm ECL}^{\rm extra}, which is defined as the total energy of the neutral clusters detected in the ECL not associated with either BtagB_{\rm tag} or BsigB_{\rm sig}. We reduce the contribution of beam-associated backgrounds while estimating EECLextraE_{\rm ECL}^{\rm extra} by only counting clusters with energy greater than 0.15, 0.05 and 0.10 GeV for the backward, barrel, and forward regions, respectively. In signal events EECLextraE_{\rm ECL}^{\rm extra} should be zero or have a small value due to the residual energy from beam-associated backgrounds or mismatched tracks. Background events tend to have larger values due to contributions from additional neutral clusters. We select events with EECLextra<0.2E_{\rm ECL}^{\rm extra}<0.2 GeV as the signal region and those with EECLextra<2E_{\rm ECL}^{\rm extra}<2 GeV for sideband studies. The selection criteria in this study are chosen to maximize the search sensitivity in the signal region following the Punzi figure of merit [36].

In the c.m. frame, the BtagB_{\rm tag} and BsigB_{\rm sig} have opposite flight directions, and the BtagB_{\rm tag} is fully reconstructed and its four-vector is determined. The momentum of BsigB_{\rm sig} is thus derived from the BtagB_{\rm tag} reconstruction. Its direction is opposite the BtagB_{\rm tag} and its magnitude is calculated as |pBsig|=(Ecm/2)2/c2mB2c2|\vec{p}_{B\rm{sig}}|=\sqrt{(E_{\rm{cm}}/2)^{2}/c^{2}-m_{B}^{2}c^{2}}, where pBsig\vec{p}_{B\rm{sig}} is the momentum vector of BsigB_{\rm sig}, Ecm/2E_{\rm{cm}}/2 is the beam energy measured in c.m frame, and mBm_{B} is the nominal B0B^{0} meson mass [30]. We calculate the τ+τ\tau^{+}\tau^{-} pair invariant mass, Mτ+τM_{\tau^{+}\tau^{-}}, by subtracting the reconstructed K0K^{\ast 0} c.m. four-vector from the BsigB_{\rm sig}’s giving its kinematic limits. We require Mτ+τM_{\tau^{+}\tau^{-}} to be greater than 3.55 GeV/c2c^{2} to suppress combinatorial background.

After the selections above, the remaining background is final-state dependent. We classify the remaining events into signal modes based on final-state particles for further background suppression. We identify electron candidates using an electron likelihood ratio, e=e/(e+e¯)\mathcal{R}_{e}=\mathcal{L}_{e}/(\mathcal{L}_{e}+\mathcal{L}_{\bar{e}}), e¯\bar{e} indicates non-electron hypothesis. e\mathcal{L}_{e} (e¯\mathcal{L}_{\bar{e}}) are calculated based on dE/dxdE/dx information from the CDC, the ratio of the energy deposited in the ECL to the momentum measured by the CDC and SVD, the shower shape in the ECL, hit information from the ACC, and matching between the position of the charged track and the ECL cluster [37]. Muon candidates are identified using a muon likelihood ratio, μ=μ/(μ+π+K)\mathcal{R}_{\mu}=\mathcal{L}_{\mu}/(\mathcal{L}_{\mu}+\mathcal{L}_{\pi}+\mathcal{L}_{K}), which is estimated based on the difference between the range of the track in KLM, estimated assuming no hadronic interactions, and the actual range observed in the KLM. A χ2\chi^{2} from extrapolating a track to the signals identified in the KLM using a Kalman filter also contributes to the likelihood [38]. Tracks are identified as electrons if e>0.8\mathcal{R}_{e}>0.8, as muons if not satisfying the electron requirement and have μ>0.8\mathcal{R}_{\mu}>0.8, and as a pion if not either an electron or a muon. The average of electron (muon) identification efficiency for the selection e(μ)>0.8\mathcal{R}_{e(\mu)}>0.8 is 92 (92)% with pion fake rate of 0.25 (2.5)%. In the signal decay modes K0π+πK^{\ast 0}\pi^{+}\pi^{-} and K0±πK^{\ast 0}\ell^{\pm}\pi^{\mp}, there remains a large background contribution from the decay B0D()+νB^{0}\rightarrow D^{(*)-}\ell^{+}\nu_{\ell}, where D()K0π(π0)D^{(*)-}\rightarrow K^{\ast 0}\pi^{-}(\pi^{0}). We suppress this by requiring the invariant mass MK0πM_{K^{\ast 0}\pi^{-}} to lie outside the DD^{-} mass region, MK0π<1.84M_{K^{\ast 0}\pi^{-}}<1.84 GeV/c2c^{2} or MK0π>1.94M_{K^{\ast 0}\pi^{-}}>1.94 GeV/c2c^{2}, where MK0πM_{K^{\ast 0}\pi^{-}} is the combination of the K0K^{\ast 0} candidate and a track that is opposite to the charge of the kaon candidate in the K0K^{\ast 0} decay. Combinatorial background is also significant in these signal modes, and so the 𝒪NB{\cal O}_{\rm NB} selection criterion is tightened to ln(𝒪NB)>4{\ln(\cal O}_{\rm NB})>-4 for these modes.

After we apply above selection criteria, our simulation predicts that the remaining backgrounds with low EECLextraE_{\rm ECL}^{\rm extra} are primarily B0B¯0B^{0}\bar{B}^{0} events in which a BtagB_{\rm tag} is properly reconstructed opposite B0D+νB^{0}\rightarrow D^{-}\ell^{+}\nu_{\ell} decaying to DK0ν¯D^{-}\rightarrow K^{\ast 0}\ell^{-}\bar{\nu}_{\ell}. Such events have the same final-state particles as signal events. The different number of missing neutrinos results in a different missing mass distribution, MmissM_{\rm miss}. We calculate this by subtracting the measured part of the four-momentum of BsigB_{\rm sig} from the derived four-momentum of BsigB_{\rm sig} from the recoil against BtagB_{\rm tag}. In addition to the missing mass, we find MK0πM_{K^{\ast 0}\pi^{-}} is also powerful distinguishing signal from the remaining background. For K0+K^{\ast 0}\ell^{-}\ell^{+} modes, we calculate MK0πM_{K^{\ast 0}\pi^{-}} by combining the negatively charged lepton with the K0K^{\ast 0} assuming a pion mass. We optimize selection criteria based on Mmiss2M_{\rm miss}^{2} and MK0πM_{K^{\ast 0}\pi^{-}} together mode-by-mode. These are summarized in Table 1. Since the number of missing neutrinos from the K0π+πK^{\ast 0}\pi^{+}\pi^{-} mode is the same as that from the B0D+νB^{0}\rightarrow D^{-}\ell^{+}\nu_{\ell} background, the Mmiss2M_{\rm miss}^{2} is ineffective in rejecting this background. We only apply the selection Mmiss2<9M_{\rm miss}^{2}<9 GeV2/c4\rm{GeV}^{2}/c^{4} to reject combinatorial background which is significant in this mode. Despite the continuum suppression performed by the full reconstruction algorithm, a small fraction of continuum events remains in the K0π+πK^{\ast 0}\pi^{+}\pi^{-} signal mode. In this case, further constraints on the event shape are imposed. Specifically, the event thrust is required to be smaller than 0.85, the cosine of the angle between the thrust of BsigB_{\rm sig} and that of BtagB_{\rm tag} must be smaller than 0.85, and the modified second Fox-Wolfram moment is required to be less than 0.4.

Table 1: Summary of the selection criteria imposed on MK0πM_{K^{\ast 0}\pi^{-}} and Mmiss2M_{\rm miss}^{2} for each of the signal modes.
Signal Mode MK0πM_{K^{\ast 0}\pi^{-}} Mmiss2M_{\rm miss}^{2}
(GeV/c2c^{2}) (GeV2/c4\rm{GeV}^{2}/c^{4})
K0e+eK^{\ast 0}e^{+}e^{-} >1.4>1.4 >3.2>3.2
K0eμ±K^{\ast 0}e^{\mp}\mu^{\pm} >1.4>1.4 >1.6>1.6
K0μ+μK^{\ast 0}\mu^{+}\mu^{-} >1.6>1.6 >1.6>1.6
K0πe±K^{\ast 0}\pi^{\mp}e^{\pm} >1.4>1.4 >2.0>2.0
K0πμ±K^{\ast 0}\pi^{\mp}\mu^{\pm} >1.4>1.4 >2.0>2.0
K0π+πK^{\ast 0}\pi^{+}\pi^{-} >1.5>1.5 <9<9
Refer to caption
(a)
Refer to caption
(b)
Figure 1: Fit results for Mmiss2M_{\rm miss}^{2} (upper) and EECLextraE_{\rm ECL}^{\rm extra} (lower) for the decays B0D()νB^{0}\rightarrow D^{(*)}\ell\nu_{\ell}. The dots with error bars represent the data, and the blue line indicates the fitted results. The dashed lines indicate different fit components. EECLextraE_{\rm ECL}^{\rm extra} is plotted with the selection Mmiss2<0.5GeV2M_{\rm miss}^{2}<0.5~{}\rm{GeV}^{2}/c4c^{4}.

We estimate the signal reconstruction efficiency after applying all of the selection criteria and BtagB_{\rm tag} efficiency corrections. The overall selection efficiency, determined using simulated B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} decays, is approximately (1.23±0.05)×105(1.23\pm 0.05)\times 10^{-5}, where the uncertainty is statistical. The signal yield is extracted with a binned extended maximum-likelihood fit to the EECLextraE_{\rm ECL}^{\rm extra} distribution, with a bin width of 0.1 GeV. The probability density functions (PDFs) for signal and background components are taken from MC expectations after applying the B-tag efficiency correction. To reduce the uncertainty due to low statistics, a simulation sample three times larger than the data is used to construct the background PDFs, the signal PDF is derived from 50 million Υ(4S)B0B¯0\Upsilon(4S)\rightarrow B^{0}\bar{B}^{0} signal events, and signal modes are combined in the fit. The B+BB^{+}B^{-} and B0B¯0B^{0}\bar{B}^{0} samples are normalized to the data and their ratio is fixed in the fit. Contributions from RareBRare~{}B and uνu\ell\nu_{\ell} components in the final sample are negligible, and are normalized to the number of BB¯B\bar{B} pairs and fixed in the fit. We float the BB¯B\bar{B}, continuum, and signal normalizations. We have validated the fitting procedure in tests with MC samples.

We test the analysis procedure and shape of the simulated EECLextraE_{\rm ECL}^{\rm extra} distribution using B0D+νB^{0}\rightarrow D^{-}\ell^{+}\nu_{\ell} decays, with DK0πD^{-}\rightarrow K^{\ast 0}\pi^{-}. The analysis steps and selection criteria for the decay are the same as those for the B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} decay, except the requirement on Mmiss2M_{\rm miss}^{2} is removed and the selection on MK0πM_{K^{\ast 0}\pi^{-}} is reversed, requiring 1.84<MK0π<1.941.84<M_{K^{\ast 0}\pi^{-}}<1.94 GeV/c2c^{2}. We divided the sample into the two sub-samples, one with Mmiss2<0.5M_{\rm miss}^{2}<0.5 GeV2/c4\rm{GeV}^{2}/c^{4} and the other with Mmiss2>0.5M_{\rm miss}^{2}>0.5 GeV2/c4\rm{GeV}^{2}/c^{4}. The first sub-sample where events are mainly from B0D+νB^{0}\rightarrow D^{-}\ell^{+}\nu_{\ell} is useful for checking the signal shape. The latter containing mostly background events is used for validate the background shape. Within statistics, the signal and background models obtained from simulation are in good agreement with the data and are used to model the signal and background in the final fit. As a cross-check, we measure the branching fraction of the decay B0D+νB^{0}\rightarrow D^{-}\ell^{+}\nu_{\ell} from a fit to the EECLextraE_{\rm ECL}^{\rm extra} distributions, similar to our search for the decay B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-}, and also to the Mmiss2M_{\rm miss}^{2} distribution. Results of these fits are shown in Fig. 1. The branching fraction measured by fitting to EECLextraE_{\rm ECL}^{\rm extra} for the first sub-sample is (2.45±0.17)%(2.45\pm 0.17)\% and to Mmiss2M_{\rm miss}^{2} is (2.37±0.15)%(2.37\pm 0.15)\%, where the quoted uncertainties are statistical only. The results are in good agreement with the world average of 2.31±0.102.31\pm 0.10% [30]. We obtained a zero signal for the fit to EECLextraE_{\rm ECL}^{\rm extra} distribution of the second sub-sample (Mmiss2>0.5M_{\rm miss}^{2}>0.5 GeV2/c4\rm{GeV}^{2}/c^{4}) as expected.

We perform the fit to EECLextraE_{\rm ECL}^{\rm extra} for the decay B0K0τ+τB^{0}\rightarrow K^{\ast 0}\tau^{+}\tau^{-} using the procedure as described above, where all signal modes have been combined. The numbers of signal and background events in the signal window [0; 0.2] GeV obtained from the fit are Nsig=4.9±6.0N_{\rm sig}=-4.9\pm 6.0 and Nbkg=122.4±4.9N_{\rm bkg}=122.4\pm 4.9, respectively. We find no evidence for a signal. Data are consistent with background as shown in Fig. 2, where the background-only model is fitted to data and a signal with branching fraction of 3.1×1033.1\times 10^{-3} is superimposed on the top.

Refer to caption
Figure 2: Distribution of EECLextraE_{\rm ECL}^{\rm extra} combined for all signal modes. The dots with error bars show the data, the blue line shows the fitted results with the background-only model, and the dashed lines show fit results for the different components. A signal (red region) with a branching fraction of 3.1×1033.1\times 10^{-3}, corresponding to the upper limit at 90% CL, is superimposed on the top of the fit.

Systematic uncertainties on the number of background events, the signal reconstruction efficiency, and number of BB¯B\bar{B} pairs arise from several sources and affect the branching fraction upper limit. The uncertainty on number of BB¯B\bar{B} pairs is 1.8%. The statistical uncertainty on the selection efficiency due to limited MC sample size is estimated to be 4.0%. The uncertainty associated with the BtagB_{\rm tag} efficiency is 5.1%, which is estimated using various decays as studied in Ref. [34]. Tracking uncertainty is assigned to be 1.4% for the four BsigB_{\rm sig} charged tracks. The uncertainty due to the charged track selection is estimated to be 4.1%. Particle identification impacts K0K^{\ast 0} reconstruction and signal mode separation, hence the uncertainties from electron, muon, and pion identification are weighted following their fraction in the signal mode. The total particle identification uncertainty is 2.55%. The difference in reconstruction efficiency for π0\pi^{0} and KS0K_{S}^{0} leads to a systematic uncertainty in application of the corresponding vetoes. Their uncertainties are estimated to be 0.17% and 1.56% for π0\pi^{0} and KS0K_{S}^{0}, respectively. The uncertainty on the branching fraction of τ\tau is 0.57%. The total systematic uncertainty is 8.5% calculated by summing the above uncertainties in quadrature.

The systematic uncertainty due to the statistical error of the PDF templates is estimated by varying bin contents of the templates following the Poisson distribution and repeating the fit to the data. This step is repeated 1000 times for each of the PDF. The standard deviation of the number of signal distribution obtained from the fits is considered as systematics uncertainty. The total uncertainty is 4.59 events.

The signal yield obtained from the extended maximum-likelihood fit is translated into an upper limit on the BK0τ+τB\rightarrow K^{\ast 0}\tau^{+}\tau^{-} branching fraction using the CLs method [39, 40]. We account for statistical and systematic uncertainties on the number of background events and signal efficiencies by modeling them as Gaussian functions with standard deviations given by their uncertainties. Our observed upper limit on the BK0τ+τB\rightarrow K^{\ast 0}\tau^{+}\tau^{-} branching fraction is 3.1×1033.1\times 10^{-3} at 90% CL.

In conclusion, we have performed a search for the decay BK0τ+τB\rightarrow K^{\ast 0}\tau^{+}\tau^{-} using the full Belle data set collected at the c.m. energy of the Υ(4S)\Upsilon(4S) resonance. We find no signal and set an upper limit on the branching fraction to be 3.1×1033.1\times 10^{-3} at 90% CL. This is the first experimental limit on the decay BK0τ+τB\rightarrow K^{\ast 0}\tau^{+}\tau^{-}.

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 DP180102629, DP170102389, DP170102204, DP150103061, 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; 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 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 Grant Nos. 2016R1D1A1B01010135, 2016R1D1A1B02012900, 2018R1A2B3003643, 2018R1A6A1A06024970, 2019K1A3A7A09033840, 2019R1I1A3A01058933, 2021R1A6A1A03043957, 2021R1F1A1060423, 2021R1F1A1064008; 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 S-1440-0321, S-0256-1438, and S-0280-1439 (Saudi Arabia); the Slovenian Research Agency Grant Nos. J1-9124 and 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.

References