Measurement of branching fraction and final-state asymmetry for the $\bar{B}^{0}\to K^{0}_{S}K^{\mp}\pi^{\pm}$ decay
Belle Collaboration: Y.-T. Lai, I. Adachi, H. Aihara, S. Al Said, D., M. Asner, H. Atmacan, V. Aulchenko, T. Aushev, V. Babu, I. Badhrees, A. M., Bakich, V. Bansal, P. Behera, C. Bele\{n}o, B. Bhuyan, T. Bilka, J. Biswal,, A. Bobrov, A. Bozek, M. Bra\v{c}ko, L. Cao

TL;DR
This paper reports a precise measurement of the decay rate and asymmetry for the $ar{B}^{0} o K^{0}_{S}K^{ p}\pi^{ p}$ decay, revealing potential intermediate structures, based on extensive data from the Belle experiment.
Contribution
First measurement of the branching fraction and final-state asymmetry for this decay mode using Belle data, with insights into decay dynamics and possible intermediate resonances.
Findings
Branching fraction of (3.60±0.33±0.15)×10⁻⁶.
Final-state asymmetry of -8.5±8.9±0.2%.
Hints of peaking structures in differential distributions.
Abstract
We report a measurement of the branching fraction and final-state asymmetry for the decays. The analysis is based on a data sample of 711 collected at the resonance with the Belle detector at the KEKB asymmetric-energy collider. We obtain a branching fraction of and a final-state asymmetry of , where the first uncertainties are statistical and the second are systematic. Hints of peaking structures are seen in the differential branching fractions measured as functions of Dalitz variables.
Click any figure to enlarge with its caption.
Figure 1
Figure 2
Figure 3
Figure 4
Figure 5
Figure 6
Figure 7
Figure 8
Figure 9
Figure 10| (/GeV) | eff. | Yield | |||||
|---|---|---|---|---|---|---|---|
| yield | yield | ||||||
| 01.1 | 0.301 | ||||||
| 1.11.5 | 0.306 | ||||||
| 1.52.5 | 0.289 | ||||||
| 2.53.5 | 0.262 | ||||||
| 3.5 | 0.237 | ||||||
| 01.1 | 0.275 | ||||||
| 1.11.5 | 0.269 | ||||||
| 1.52.5 | 0.252 | ||||||
| 2.53.5 | 0.264 | ||||||
| 3.5 | 0.283 | ||||||
| 01.1 | 0.245 | ||||||
| 1.11.5 | 0.258 | ||||||
| 1.52.5 | 0.235 | ||||||
| 2.53.5 | 0.267 | ||||||
| 3.5 | 0.292 |
| Source | in % |
|---|---|
| 1.4 | |
| Tracking | 0.7 |
| identification | 0.8 |
| identification | 0.8 |
| 0.1 | |
| identification | 1.6 |
| Continuum suppression with NN | 2.1 |
| Reconstruction efficiency (MC statistics) | 0.1 |
| Signal PDF | 2.7 |
| Background PDF | 0.4 |
| Fit bias | 0.4 |
| Total | 4.3 |
| Source | in % |
|---|---|
| Detector bias | 0.6 |
| Signal PDF | 2.7 |
| Background PDF | 0.9 |
| Total | 2.9 |
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Measurement of branching fraction and final-state asymmetry for the decay
Y.-T. Lai
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
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
S. Al Said
Department of Physics, Faculty of Science, University of Tabuk, Tabuk 71451
Department of Physics, Faculty of Science, King Abdulaziz University, Jeddah 21589
D. M. Asner
Brookhaven National Laboratory, Upton, New York 11973
H. Atmacan
University of South Carolina, Columbia, South Carolina 29208
V. Aulchenko
Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090
Novosibirsk State University, Novosibirsk 630090
T. Aushev
Moscow Institute of Physics and Technology, Moscow Region 141700
V. Babu
Tata Institute of Fundamental Research, Mumbai 400005
I. Badhrees
Department of Physics, Faculty of Science, University of Tabuk, Tabuk 71451
King Abdulaziz City for Science and Technology, Riyadh 11442
A. M. Bakich
School of Physics, University of Sydney, New South Wales 2006
V. Bansal
Pacific Northwest National Laboratory, Richland, Washington 99352
P. Behera
Indian Institute of Technology Madras, Chennai 600036
C. Beleño
II. Physikalisches Institut, Georg-August-Universität Göttingen, 37073 Göttingen
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
University of Maribor, 2000 Maribor
J. Stefan Institute, 1000 Ljubljana
L. Cao
Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe
D. Červenkov
Faculty of Mathematics and Physics, Charles University, 121 16 Prague
P. Chang
Department of Physics, National Taiwan University, Taipei 10617
V. Chekelian
Max-Planck-Institut für Physik, 80805 München
A. Chen
National Central University, Chung-li 32054
B. G. Cheon
Hanyang University, Seoul 133-791
K. Chilikin
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
K. Cho
Korea Institute of Science and Technology Information, Daejeon 305-806
S.-K. Choi
Gyeongsang National University, Chinju 660-701
Y. Choi
Sungkyunkwan University, Suwon 440-746
S. Choudhury
Indian Institute of Technology Hyderabad, Telangana 502285
D. Cinabro
Wayne State University, Detroit, Michigan 48202
S. Cunliffe
Deutsches Elektronen–Synchrotron, 22607 Hamburg
N. Dash
Indian Institute of Technology Bhubaneswar, Satya Nagar 751007
S. Di Carlo
LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, Orsay
Z. Doležal
Faculty of Mathematics and Physics, Charles University, 121 16 Prague
T. V. Dong
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
S. Eidelman
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
D. Epifanov
Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090
Novosibirsk State University, Novosibirsk 630090
J. E. Fast
Pacific Northwest National Laboratory, Richland, Washington 99352
A. Frey
II. Physikalisches Institut, Georg-August-Universität Göttingen, 37073 Göttingen
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
M. Gelb
Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe
A. Giri
Indian Institute of Technology Hyderabad, Telangana 502285
P. Goldenzweig
Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe
D. Greenwald
Department of Physics, Technische Universität München, 85748 Garching
Y. Guan
Indiana University, Bloomington, Indiana 47408
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
J. Haba
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
T. Hara
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
K. Hayasaka
Niigata University, Niigata 950-2181
H. Hayashii
Nara Women’s University, Nara 630-8506
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. Huang
Department of Physics, National Taiwan University, Taipei 10617
T. Iijima
Kobayashi-Maskawa Institute, Nagoya University, Nagoya 464-8602
Graduate School of Science, Nagoya University, Nagoya 464-8602
K. Inami
Graduate School of Science, Nagoya University, Nagoya 464-8602
G. Inguglia
Deutsches Elektronen–Synchrotron, 22607 Hamburg
A. Ishikawa
Department of Physics, Tohoku University, Sendai 980-8578
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
Y. Iwasaki
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
S. Jia
Beihang University, Beijing 100191
Y. Jin
Department of Physics, University of Tokyo, Tokyo 113-0033
D. Joffe
Kennesaw State University, Kennesaw, Georgia 30144
A. B. Kaliyar
Indian Institute of Technology Madras, Chennai 600036
G. Karyan
Deutsches Elektronen–Synchrotron, 22607 Hamburg
T. Kawasaki
Kitasato University, Sagamihara 252-0373
H. Kichimi
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
C. Kiesling
Max-Planck-Institut für Physik, 80805 München
D. Y. Kim
Soongsil University, Seoul 156-743
H. J. Kim
Kyungpook National University, Daegu 702-701
J. B. Kim
Korea University, Seoul 136-713
S. H. Kim
Hanyang University, Seoul 133-791
K. Kinoshita
University of Cincinnati, Cincinnati, Ohio 45221
P. Kodyš
Faculty of Mathematics and Physics, Charles University, 121 16 Prague
S. Korpar
University of Maribor, 2000 Maribor
J. Stefan Institute, 1000 Ljubljana
D. Kotchetkov
University of Hawaii, Honolulu, Hawaii 96822
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
R. Kumar
Punjab Agricultural University, Ludhiana 141004
A. Kuzmin
Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090
Novosibirsk State University, Novosibirsk 630090
Y.-J. Kwon
Yonsei University, Seoul 120-749
K. Lalwani
Malaviya National Institute of Technology Jaipur, Jaipur 302017
J. S. Lange
Justus-Liebig-Universität Gießen, 35392 Gießen
I. S. Lee
Hanyang University, Seoul 133-791
J. K. Lee
Seoul National University, Seoul 151-742
J. Y. Lee
Seoul National University, Seoul 151-742
S. C. Lee
Kyungpook National University, Daegu 702-701
C. H. Li
School of Physics, University of Melbourne, Victoria 3010
L. K. Li
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049
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
Z. Liptak
University of Hawaii, Honolulu, Hawaii 96822
D. Liventsev
Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
P.-C. Lu
Department of Physics, National Taiwan University, Taipei 10617
M. Lubej
J. Stefan Institute, 1000 Ljubljana
T. Luo
Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) and Institute of Modern Physics, Fudan University, Shanghai 200443
J. MacNaughton
University of Miyazaki, Miyazaki 889-2192
M. Masuda
Earthquake Research Institute, University of Tokyo, Tokyo 113-0032
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, 80126 Napoli
Università di Napoli Federico II, 80055 Napoli
K. Miyabayashi
Nara Women’s University, Nara 630-8506
R. Mizuk
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
Moscow Physical Engineering Institute, Moscow 115409
Moscow Institute of Physics and Technology, Moscow Region 141700
G. B. Mohanty
Tata Institute of Fundamental Research, Mumbai 400005
T. Mori
Graduate School of Science, Nagoya University, Nagoya 464-8602
M. Mrvar
J. Stefan Institute, 1000 Ljubljana
R. Mussa
INFN - Sezione di Torino, 10125 Torino
E. Nakano
Osaka City University, Osaka 558-8585
M. Nakao
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
K. J. Nath
Indian Institute of Technology Guwahati, Assam 781039
M. Nayak
Wayne State University, Detroit, Michigan 48202
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
N. K. Nisar
University of Pittsburgh, Pittsburgh, Pennsylvania 15260
S. Nishida
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
S. Ogawa
Toho University, Funabashi 274-8510
G. Pakhlova
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
Moscow Institute of Physics and Technology, Moscow Region 141700
B. Pal
Brookhaven National Laboratory, Upton, New York 11973
S. Pardi
INFN - Sezione di Napoli, 80126 Napoli
H. Park
Kyungpook National University, Daegu 702-701
S. Paul
Department of Physics, Technische Universität München, 85748 Garching
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
V. Popov
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
Moscow Institute of Physics and Technology, Moscow Region 141700
E. Prencipe
Forschungszentrum Jülich, 52425 Jülich
A. Rabusov
Department of Physics, Technische Universität München, 85748 Garching
M. Ritter
Ludwig Maximilians University, 80539 Munich
A. Rostomyan
Deutsches Elektronen–Synchrotron, 22607 Hamburg
G. Russo
INFN - Sezione di Napoli, 80126 Napoli
Y. Sakai
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
M. Salehi
University of Malaya, 50603 Kuala Lumpur
Ludwig Maximilians University, 80539 Munich
S. Sandilya
University of Cincinnati, Cincinnati, Ohio 45221
L. Santelj
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
T. Sanuki
Department of Physics, Tohoku University, Sendai 980-8578
V. Savinov
University of Pittsburgh, Pittsburgh, Pennsylvania 15260
O. Schneider
École Polytechnique Fédérale de Lausanne (EPFL), Lausanne 1015
G. Schnell
University of the Basque Country UPV/EHU, 48080 Bilbao
IKERBASQUE, Basque Foundation for Science, 48013 Bilbao
C. Schwanda
Institute of High Energy Physics, Vienna 1050
Y. Seino
Niigata University, Niigata 950-2181
K. Senyo
Yamagata University, Yamagata 990-8560
O. Seon
Graduate School of Science, Nagoya University, Nagoya 464-8602
M. E. Sevior
School of Physics, University of Melbourne, Victoria 3010
C. P. Shen
Beihang University, Beijing 100191
T.-A. Shibata
Tokyo Institute of Technology, Tokyo 152-8550
J.-G. Shiu
Department of Physics, National Taiwan University, Taipei 10617
E. Solovieva
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
Moscow Institute of Physics and Technology, Moscow Region 141700
M. Starič
J. Stefan Institute, 1000 Ljubljana
M. Sumihama
Gifu University, Gifu 501-1193
T. Sumiyoshi
Tokyo Metropolitan University, Tokyo 192-0397
W. Sutcliffe
Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe
M. Takizawa
Showa Pharmaceutical University, Tokyo 194-8543
J-PARC Branch, KEK Theory Center, High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
Theoretical Research Division, Nishina Center, RIKEN, Saitama 351-0198
K. Tanida
Advanced Science Research Center, Japan Atomic Energy Agency, Naka 319-1195
Y. Tao
University of Florida, Gainesville, Florida 32611
F. Tenchini
Deutsches Elektronen–Synchrotron, 22607 Hamburg
M. Uchida
Tokyo Institute of Technology, Tokyo 152-8550
T. Uglov
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
Moscow Institute of Physics and Technology, Moscow Region 141700
Y. Unno
Hanyang University, Seoul 133-791
S. Uno
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
P. Urquijo
School of Physics, University of Melbourne, Victoria 3010
Y. Usov
Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090
Novosibirsk State University, Novosibirsk 630090
R. Van Tonder
Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe
G. Varner
University of Hawaii, Honolulu, Hawaii 96822
K. E. Varvell
School of Physics, University of Sydney, New South Wales 2006
B. Wang
University of Cincinnati, Cincinnati, Ohio 45221
C. H. Wang
National United University, Miao Li 36003
M.-Z. Wang
Department of Physics, National Taiwan University, Taipei 10617
P. Wang
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049
X. L. Wang
Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) and Institute of Modern Physics, Fudan University, Shanghai 200443
E. Widmann
Stefan Meyer Institute for Subatomic Physics, Vienna 1090
E. Won
Korea University, Seoul 136-713
H. Yamamoto
Department of Physics, Tohoku University, Sendai 980-8578
S. B. Yang
Korea University, Seoul 136-713
H. Ye
Deutsches Elektronen–Synchrotron, 22607 Hamburg
C. Z. Yuan
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049
Y. Yusa
Niigata University, Niigata 950-2181
Z. P. Zhang
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
V. Zhulanov
Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090
Novosibirsk State University, Novosibirsk 630090
Abstract
We report a measurement of the branching fraction and final-state asymmetry for the decays. The analysis is based on a data sample of 711 collected at the resonance with the Belle detector at the KEKB asymmetric-energy collider. We obtain a branching fraction of and a final-state asymmetry of , where the first uncertainties are statistical and the second are systematic. Hints of peaking structures are seen in the differential branching fractions measured as functions of Dalitz variables.
pacs:
14.40.Nd, 13.25.Hw, 13.25.-k, 11.30.Er
††preprint:
Belle Preprint 2019-06
KEK Preprint 2019-4
The Belle Collaboration
Three-body charmless hadronic decays are sensitive to violation localized in their Dalitz plane cp_dalitz ; cp_dalitz_1 . Charmless decays are suppressed in the standard model (SM), and decays with an even number of kaons, such as charge_conjugate , have a smaller decay rate compared to those with an odd number of kaons. These proceed via trees and -exchange, and via a penguin process with a virtual loop; the latter provides an opportunity to search for physics beyond the SM since new heavy particles may cause deviations from SM predictions.
Previous measurements by the BABAR babar_Btokpik0 ; babar_kstk0 and LHCb LHCb_Btokpik0_latest ; LHCb_kstk ; LHCb_kstks experiments found hints of structures in the low and mass regions that have highly asymmetric helicity angular distributions. However, the yields are not sufficient to draw firm conclusions with a full Dalitz analysis. Similar studies on were performed by Belle kkpi_1 , BABAR kkpi_2 , and LHCb kkpi_3 ; kkpi_4 , in which strong evidence of localized violation was found in the low region.
By using the full data set of Belle, we expect to measure the branching fraction and final-state asymmetry of decays more precisely. Using the charges of final-state particles, the latter is defined as
[TABLE]
where denotes the measured signal yield of the corresponding final states, and . Here is distinct from the direct asymmetry (); rather it is an asymmetry between the decay final states of and where leads to a . We measure this quantity since it can be more precisely determined than for this decay mode. This is the first measurement of such an asymmetry for the three-body decay. In addition, we use the splot method to obtain background-subtracted yields for the Dalitz variables , , and , and hence determine their differential branching fractions. The total branching fraction is extracted by integrating the differential branching fraction.
Our measurement is based on a data sample of 711 , corresponding to pairs, collected with the Belle detector Belle operating at the KEKB asymmetric-energy collider KEKB . The Belle detector is a large-solid-angle magnetic spectrometer that consists 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, all located inside a superconducting solenoid that provides a 1.5 T magnetic field. An iron flux-return yoke located outside the solenoid is instrumented to detect mesons and muons. The detector is described in detail elsewhere Belle .
This analysis uses two data sets with different inner-detector configurations. The first data set of 140 was collected with a beam pipe of radius 2.0 cm and with 3 layers of SVD, while the second data set of 571 was recorded with a beam pipe of radius 1.5 cm and 4 layers of SVD svd2 . Large samples of Monte Carlo (MC) events for signal and backgrounds are generated with EvtGen ref:EvtGen and subsequently simulated with GEANT3 geant with the configurations of the Belle detector. These samples are used to obtain the expected distributions of various physical quantities for signal and backgrounds, to optimize the selection criteria as well as to determine the signal detection efficiency.
The selection criteria for the final-state charged particles in the reconstruction are based on information obtained from the tracking systems (SVD and CDC) and the charged-hadron identification (PID) systems, namely the CDC, ACC, and TOF. The charged kaons and pions are required to have an impact parameter within cm of the interaction point (IP) in the transverse plane, and within cm along the beam direction. The likelihood values of each track for kaon and pion hypotheses ( and ) are determined from the information provided by the PID system. A track is identified as a kaon if otherwise it is treated as a pion. The efficiency for identifying a pion (kaon) is about 88% (86%), which depends on the momenta of the track, while the probability for a pion or a kaon to be misidentified is less than 10%. The efficiency and misidentification probabilities are averaged over the momentum of the final-state particles. The candidates are reconstructed via the decay, and the identification is enhanced by selecting on the output of a neural network (NN) NN , which combines seven kinematic variables of the nisKs . The invariant mass of the candidates is required to be within MeV/ of the world average, which corresponds to about three times the resolution. The vertex fit is required to converge with a goodness-of-fit value less than 20.
mesons are identified with two kinematic variables calculated in the center-of-mass (CM) frame: the beam-energy-constrained-mass , and the energy difference , where is the beam energy, and () is the momentum (energy) of the reconstructed meson. The candidates are required to have 5.255 GeV/ and 0.15 GeV, and the signal region is defined as 5.272 GeV/ 5.288 GeV/ and 0.05 GeV. We require a successful vertex fit for candidates, where the trajectory is included in the fit, with 100. We find that 9% of events have more than one candidate. In such cases, we choose the candidate with the smallest value. According to simulation, our best entry selection method chooses the correct candidate in 99% of cases.
The dominant background arises from the continuum process. To suppress this, we construct a Fisher discriminant Fisher from 17 modified Fox-Wolfram moments KSFW . To further improve the distinguishing power, we combine the output of the Fisher discriminant with four more variables in a NN. These are: the cosine of the angle between the reconstructed flight direction and the beam direction in the CM frame, the offset along the axis between the vertex of the reconstructed and the vertex formed by the remaining tracks, the cosine of the angle between the thrust axis thrust of the reconstructed and that of the rest of the event in the CM frame, and a meson flavor tagging quality variable. The NN is trained with signal and continuum MC samples. The NN output () ranges from to 1, and it is required to be greater than 0.7. This removes 93% of the continuum background while 82% of the signal is retained. We transform to , where is 0.7 and is the maximum value of .
Background events from decays mediated via the transition (generic decays) may have peaking structures in the signal region. They are mainly due to the decays with two-body final states of mesons and , e.g., , , , , and . These decays can be identified by peaks at the nominal and masses in the distributions of the invariant masses of two of the final-state particles (, , , where we allow for a change in the mass hypothesis of a charged kaon or pion). We exclude events within of the nominal mass of the peaking structures to suppress the contributions from mesons and .
The rare background coming from transitions is studied with a large MC sample in which the branching fractions are much larger than the measured or expected value. Two modes are found to have peaks near the signal region: and , including their intermediate resonant modes. The remaining rare events have a relatively flat distribution.
The signal yield and are extracted from a three-dimensional extended unbinned maximum likelihood fit, with the likelihood defined as
[TABLE]
where,
[TABLE]
is the total number of candidate events, is the number of events in category , denotes the event index, is the charge of the in the -th event, is the value of final-state asymmetry of the -th category, represents the value of the corresponding three-dimensional probability density function (PDF), and , , and are the , , and values of the -th event, respectively.
With all the selection criteria applied, the signal MC sample contains 98% of the correctly-reconstructed signal events (‘true’ signal) and 2% self-crossfeed (scf) events. In the fit, the ratio of scf to true signal events is fixed. The signal yield () is the combined yield of the true signal PDF and the scf PDF. In addition to the signal, five more categories are included in the fit: continuum background, generic background, , , and the remaining rare background. The true signal PDF is described by the product of a sum of two Gaussian functions in , a sum of three Gaussian functions in , and an asymmetric Gaussian function in . These signal PDF shapes are calibrated including possible data-MC differences obtained from a study of a control mode: with . The continuum background PDF is described by the product of an ARGUS function argus in , a second-order polynomial in , and a combination of a Gaussian and an asymmetric Gaussian function in . The shape parameters of the continuum background PDF are free in the data fit, except for the ARGUS endpoint which is fixed to 5.2892 GeV/. For the other contributions (scf, generic , , , and rare ), their PDFs are described by a smoothed histogram in and , and an asymmetric Gaussian function in whose shape is based on MC. The yield of each category is floated. Except for the signal, is fixed to zero for the other background categories.
The signal-enhanced projections of the fit are shown in Fig. 1. We obtain a signal yield of with a statistical significance of 13 standard deviations, and an of . The significance is defined as , where and are the likelihood values obtained by the fit with and without the signal yield fixed to zero, respectively.
The branching fraction is calculated using
[TABLE]
where , , , and are the fitted signal yield, the number of pairs (), the reconstruction efficiency of the signal, and the efficiency calibration factor, respectively. We assume that charged and neutral pairs are produced equally at the . The reconstruction efficiency for the signal () is which is determined by MC only and with all the selection criteria applied. The last quantity contains calibrations due to various systematic effects , where ) and ) are the corrections due to and identification with requirements on and , and are obtained by a control sample study of with , is due to the requirement on and is obtained from data with a control sample study, and is due to fit bias and is obtained from an ensemble test on the fitter.
Figure 2 shows the background-subtracted Dalitz plot obtained with the method. Structures around the regions 2 GeV2/ and 7 GeV2/ 23 GeV2/ are visible. We also obtain background-subtracted distributions after separating into five bins, and then calculate the differential branching fractions as functions of the three Dalitz variables with the yield and reconstruction efficiency within each bin. We use a similar binning scheme as the one in the measurement at Belle kkpi_1 . Figure 3 shows the differential branching fractions as functions of the three Dalitz variables including comparison to the MC with a three-body phase space decay model. Large deviations from phase space expectations are found in the second bin (around 1.2 GeV/) of the spectrum and at the fourth and fifth bin (around 3.0 GeV/ - 4.2 GeV/) in the spectrum. In addition, no obvious structure is observed in the low-mass regions of both and , which is consistent with previous two-body decay measurements of LHCb_kstk and babar_kstk0 ; LHCb_kstks .
To investigate the localized final-state asymmetry, differential branching fractions separately for the and final states are shown in Fig. 4. Within each bin of the Dalitz variables, the results are consistent with no asymmetry. The details of differential branching fraction calculation in each bin are summarized in Table 1.
Sources of various systematic uncertainties in the branching fraction calculation are shown in Table 2. The uncertainty due to the total number of pairs is 1.4%. The uncertainty due to the charged-track reconstruction efficiency is estimated to be 0.35% per track by using partially reconstructed with events. The uncertainties due to and identification are obtained by the control sample study of with . The uncertainty due to the branching fraction is based on the world average value PDG . The uncertainty due to identification is estimated to be 1.6% based on a , control sample Ks_sys . The uncertainty due to continuum suppression with the requirement on is obtained from a with a decay control sample. The uncertainty of the reconstruction efficiency is due to limited MC statistics. The uncertainty due to the fixed signal and background PDF shapes is estimated by the deviation of fitted signal yield when varying the parameters of the PDFs in different cases. For all the smoothed histograms, we vary the binning conditions of those histograms. For the other PDFs with fixed parameterization, the fixed parameters are randomized by using a Gaussian random number to repeat data fits with various parameter sets, and the uncertainty of the yield distribution is quoted. The uncertainty due to fit bias is obtained from an ensemble test on the fitter.
Sources of various systematic uncertainties on are listed in Table 3. The uncertainty due to and detection bias are obtained by control sample studies of and phipi , and kspi , respectively. The uncertainties due to the fixed signal and background PDF shapes are treated in the same way as those in the uncertainty on the branching fraction. The systematic uncertainties due to PDF’s are also estimated from the deviation of the fitted value of with varying the conditions of those PDFs in different cases.
In conclusion, we have performed a measurement of the branching fraction and asymmetry of the decay based on a data sample of 711 fb*-1* collected by Belle. We obtain a branching fraction of and an of , where their first uncertainty is statistical and the second is systematic. The measured value is consistent with no asymmetry. Hints of peaking structures are seen in the regions 2 GeV2/ and 7 GeV2/ 23 GeV2/ in the Dalitz plot. A cross-check was performed by calculating the differential branching fraction after projecting onto each Dalitz variable, and hints of peaking structures are found near 1.2 GeV/ in and around 4.2 GeV/ in when compared to the phase space MC. No obvious structure is seen either in low and spectra, which are also consistent with the BABAR and LHCb results babar_kstk0 ; LHCb_kstk ; LHCb_kstks . No localized final-state asymmetry is observed. In the near future, experiments with large data sets such as Belle II and LHCb can provide a more detailed analysis exploiting the full Dalitz plot to search for intermediate resonances and localized final-state asymmetry.
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, the National Institute of Informatics, and the PNNL/EMSL computing group for valuable computing and SINET4 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; Austrian Science Fund under Grant No. P 22742-N16 and P 26794-N20; the National Natural Science Foundation of China under Contracts No. 10575109, No. 10775142, No. 10875115, No. 11175187, No. 11475187 and No. 11575017; the Chinese Academy of Science Center for Excellence in Particle Physics; the Ministry of Education, Youth and Sports of the Czech Republic under Contract No. LG14034; 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; the WCU program of the Ministry of Education, National Research Foundation (NRF) of Korea Grants No. 2011-0029457, No. 2012-0008143, No. 2012R1A1A2008330, No. 2013R1A1A3007772, No. 2014R1A2A2A01005286, No. 2014R1A2A2A01002734, No. 2015R1A2A2A01003280 , No. 2015H1A2A1033649; the Basic Research Lab program under NRF Grant No. KRF-2011-0020333, Center for Korean J-PARC Users, No. NRF-2013K1A3A7A06056592; the Brain Korea 21-Plus program and Radiation Science Research Institute; the Polish Ministry of Science and Higher Education and the National Science Center; the Ministry of Science and Higher Education of Russian Federation, Agreement 14.W03.31.0026; the Slovenian Research Agency; Ikerbasque, Basque Foundation for Science and the Euskal Herriko Unibertsitatea (UPV/EHU) under program UFI 11/55 (Spain); the Swiss National Science Foundation; the Ministry of Education and the Ministry of Science and Technology of Taiwan; and the U.S. Department of Energy and the National Science Foundation. This work is supported by a Grant-in-Aid from MEXT for Science Research in a Priority Area (“New Development of Flavor Physics”) and from JSPS for Creative Scientific Research (“Evolution of Tau-lepton Physics”).
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1(1) I. Bediaga et al. , Phys. Rev. D 80 , 096006 (2009).
- 2(2) I. Bediaga et al. , Phys. Rev. D 86 , 036005 (2012).
- 3(3) Throughout this paper, inclusion of charge-conjugate decay modes is implied unless otherwise stated.
- 4(4) P. del Amo Sanchez et al. , (BABAR Collaboration), Phys. Rev. D 82 , 031101 (2010).
- 5(5) B. Aubert et al. , (BABAR Collaboration), Phys. Rev. D 74 , 072008 (2016).
- 6(6) R. Aaij et al. , (LH Cb Collaboration), J. High Energy Phys. 11 (2017) 027.
- 7(7) R. Aaij et al. , (LH Cb Collaboration), New Journal of Physics. 16 (2014) 123001.
- 8(8) R. Aaij et al. , (LH Cb Collaboration), J. High Energy Phys. 01 (2016) 012.
