First measurements of absolute branching fractions of the $\Xi_c^+$ baryon at Belle
Belle Collaboration: Y.B.Li, C.P.Shen, I. Adachi, J. K. Ahn, H., Aihara, S. Al Said, D. M. Asner, H. Atmacan, T. Aushev, R. Ayad, V. Babu, A., M. Bakich, Y. Ban, V. Bansal, P. Behera, C. Bele\~no, M. Berger, V. Bhardwaj,, B. Bhuyan, T. Bilka, J. Biswal, A. Bobrov, A. Bozek

TL;DR
This paper reports the first absolute measurements of certain decay branching fractions of the $\\Xi_c^+$ baryon using data from the Belle detector, providing crucial normalization for future studies of this particle.
Contribution
It provides the first absolute branching fraction measurements of $\\Xi_c^+$ decays and the $ar{B}^0$ decay to $\\Lambda_c^-$ and $\\Xi_c^+$, establishing a new standard for $\\Xi_c^+$ decay rates.
Findings
Measured ${\cal B}(\Xi_c^+ \to \Xi^- \pi^+ \pi^+)$ as approximately 2.86%.
Measured ${\cal B}(\Xi_c^+ \to p K^- \pi^+)$ as approximately 0.45%.
Determined ${\cal B}(\bar{B}^0 \to \bar{\Lambda}_c^- \Xi_c^+)$ as approximately 1.16 x 10^{-3}.
Abstract
We present the first measurements of the absolute branching fractions of decays into and final states. Our analysis is based on a data set of pairs collected at the resonance with the Belle detector at the KEKB collider. We measure the absolute branching fraction of with the recoiling against in decays resulting in . We then measure the product branching fractions and . Dividing these product…
| Observable | Efficiency | Fit | decays |
|
|
Measured value | |||
| 3.66 | 10.3 | 5.3 | 4.5 | 1.82 | 13.1 | ||||
| 6.24 | 5.61 | 5.3 | 1.82 | 10.1 | |||||
| 7.32 | 9.53 | 5.3 | 1.82 | 13.3 | |||||
| 4.23 | 11.7 | 4.5 | 13.2 | ||||||
| 3.66 | 14.0 | 4.5 | 15.2 | ||||||
| 4.90 | 11.0 | 12.0 |
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The Belle Collaboration
First measurements of absolute branching fractions of the baryon at Belle
Y. B. Li
State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871
C. P. Shen
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
J. K. Ahn
Korea University, Seoul 136-713
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
T. Aushev
Moscow Institute of Physics and Technology, Moscow Region 141700
R. Ayad
Department of Physics, Faculty of Science, University of Tabuk, Tabuk 71451
V. Babu
Deutsches Elektronen–Synchrotron, 22607 Hamburg
A. M. Bakich
School of Physics, University of Sydney, New South Wales 2006
Y. Ban
State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871
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
M. Berger
Stefan Meyer Institute for Subatomic Physics, Vienna 1090
V. Bhardwaj
Indian Institute of Science Education and Research Mohali, SAS Nagar, 140306
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
T. E. Browder
University of Hawaii, Honolulu, Hawaii 96822
M. Campajola
INFN - Sezione di Napoli, 80126 Napoli
Università di Napoli Federico II, 80055 Napoli
L. Cao
Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe
D. Červenkov
Faculty of Mathematics and Physics, Charles University, 121 16 Prague
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
H. E. Cho
Hanyang University, Seoul 133-791
K. Cho
Korea Institute of Science and Technology Information, Daejeon 305-806
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
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
D. Dossett
School of Physics, University of Melbourne, Victoria 3010
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
T. Ferber
Deutsches Elektronen–Synchrotron, 22607 Hamburg
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
B. Grube
Department of Physics, Technische Universität München, 85748 Garching
O. Grzymkowska
H. Niewodniczanski Institute of Nuclear Physics, Krakow 31-342
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
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
Institute of High Energy Physics, Vienna 1050
A. Ishikawa
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
M. Iwasaki
Osaka City University, Osaka 558-8585
Y. Iwasaki
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
W. W. Jacobs
Indiana University, Bloomington, Indiana 47408
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
K. K. Joo
Chonnam National University, Kwangju 660-701
A. B. Kaliyar
Indian Institute of Technology Madras, Chennai 600036
G. Karyan
Deutsches Elektronen–Synchrotron, 22607 Hamburg
Y. Kato
Graduate School of Science, Nagoya University, Nagoya 464-8602
T. Kawasaki
Kitasato University, Sagamihara 252-0373
H. Kichimi
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
C. H. Kim
Hanyang University, Seoul 133-791
D. Y. Kim
Soongsil University, Seoul 156-743
H. J. Kim
Kyungpook National University, Daegu 702-701
K. T. 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
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
Liaoning Normal University, Dalian 116029
L. K. Li
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049
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
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
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
H. Miyata
Niigata University, Niigata 950-2181
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. J. Moon
Seoul National University, Seoul 151-742
R. Mussa
INFN - Sezione di Torino, 10125 Torino
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
M. Niiyama
Kyoto University, Kyoto 606-8502
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
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. Pakhlov
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
Moscow Physical Engineering Institute, Moscow 115409
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.-H. Park
Yonsei University, Seoul 120-749
S. Patra
Indian Institute of Science Education and Research Mohali, SAS Nagar, 140306
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
M. Ritter
Ludwig Maximilians University, 80539 Munich
A. Rostomyan
Deutsches Elektronen–Synchrotron, 22607 Hamburg
G. Russo
Università di Napoli Federico II, 80055 Napoli
D. Sahoo
Tata Institute of Fundamental Research, Mumbai 400005
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
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
J. Schueler
University of Hawaii, Honolulu, Hawaii 96822
C. Schwanda
Institute of High Energy Physics, Vienna 1050
A. J. Schwartz
University of Cincinnati, Cincinnati, Ohio 45221
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
V. Shebalin
University of Hawaii, Honolulu, Hawaii 96822
J.-G. Shiu
Department of Physics, National Taiwan University, Taipei 10617
B. Shwartz
Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090
Novosibirsk State University, Novosibirsk 630090
F. Simon
Max-Planck-Institut für Physik, 80805 München
A. Sokolov
Institute for High Energy Physics, Protvino 142281
E. Solovieva
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Moscow 119991
M. Starič
J. Stefan Institute, 1000 Ljubljana
Z. S. Stottler
Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061
J. F. Strube
Pacific Northwest National Laboratory, Richland, Washington 99352
M. Sumihama
Gifu University, Gifu 501-1193
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
Theoretical Research Division, Nishina Center, RIKEN, Saitama 351-0198
U. Tamponi
INFN - Sezione di Torino, 10125 Torino
K. Tanida
Advanced Science Research Center, Japan Atomic Energy Agency, Naka 319-1195
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
Y. Ushiroda
High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801
SOKENDAI (The Graduate University for Advanced Studies), Hayama 240-0193
S. E. Vahsen
University of Hawaii, Honolulu, Hawaii 96822
R. Van Tonder
Institut für Experimentelle Teilchenphysik, Karlsruher Institut für Technologie, 76131 Karlsruhe
G. Varner
University of Hawaii, Honolulu, Hawaii 96822
A. Vinokurova
Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090
Novosibirsk State University, Novosibirsk 630090
B. Wang
Max-Planck-Institut für Physik, 80805 München
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
S. Watanuki
Department of Physics, Tohoku University, Sendai 980-8578
E. Won
Korea University, Seoul 136-713
S. B. Yang
Korea University, Seoul 136-713
H. Ye
Deutsches Elektronen–Synchrotron, 22607 Hamburg
J. Yelton
University of Florida, Gainesville, Florida 32611
J. H. Yin
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049
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 present the first measurements of the absolute branching fractions of decays into and final states. Our analysis is based on a data set of pairs collected at the resonance with the Belle detector at the KEKB collider. We measure the absolute branching fraction of with the recoiling against in decays resulting in . We then measure the product branching fractions and . Dividing these product branching fractions by yields: and . Our result for can be combined with branching fractions measured relative to to set the absolute scale for many branching fractions.
pacs:
14.20.Lq, 13.30.Eg, 13.25.Hw
††preprint:
Intended for P.R.L
Author: Y. B. Li, C. P. Shen
Committee: J. Yelton(chair),
B. Grube, U. Tamponi
In recent decades there has been significant experimental progress on the measurements of the weak decays of charmed baryons PDG . However, given the limited knowledge of the large nonperturbative effects of quantum chromodynamics, it is difficult to reliably calculate the decay amplitudes of charmed baryons from first principles. Furthermore, in exclusive charmed-baryon decays the heavy quark expansion does not work. Hence experimental data are needed to extract the nonperturbative quantities in the decay amplitudes input1 ; input2 ; input3 ; input4 and to provide important information to constrain phenomenological models of such decays QCD-theory1 ; QCD-theory2 ; QCD-theory3 ; QCD-theory4 ; QCD-theory5 ; QCD-theory6 ; QCD-theory7 ; QCD-theory8 .
During last few years, Belle and BESIII have measured absolute branching fractions of the and charmed baryons lc_belle ; lc_bes ; myxic . However, the absolute branching fraction of the remaining member of the charmed-baryon SU(3) flavor antitriplet, the , has not been measured. Branching fractions of decays have been measured relative to the mode. A measurement of the absolute branching fraction is needed to infer the absolute branching fractions of other decays. The comparison of decays with those of and can also provide an important test of SU(3) flavor symmetry Savage:1989qr .
Along with the reference mode , is a particularly important decay mode as it is the one most often used to reconstruct candidates at hadron collider experiments, such as LHCb. For example, the decay has been used to study the properties of and to search for higher excited states via LHCB1 ; LHCB2 , to search for new states in the mode LHCB4 , to measure the doubly charmed baryon via LHCB5 , as well as to measure the ratio of fragmentation fractions of relative to LHCB6 ; LHCB7 .
In experiments, the decay has been observed by the FOCUS and SELEX Collaborations and the branching fraction ratio is measured to be selex1 ; focu ; selex2 ; PDG . A few models have been developed to predict the decay rates of . For example, the has been predicted to be based on the SU(3) flavor symmetry geng . Theory predicts to be based on the measured ratio and the -spin symmetry that relates and yu1 ; LHCB7 . The decay , which proceeds via a transition, has been predicted to have a branching fraction of the order BXL_theroy , but there has been no experimental measurement. The world average of the product branching fraction is with large uncertainty PDG ; belle-old1 ; babar-old2 .
In this Letter, we perform an analysis of with reconstructed via its decay, and reconstructed both inclusively and exclusively via the decay modes and charge-conjugate . We present first a measurement of the absolute branching fraction for using a missing-mass technique, which is explained below. For this analysis we fully reconstruct the tag-side decay. We subsequently measure the product branching fractions and without reconstructing the recoiling decay in the event as the signal decays are fully reconstructed. Dividing these product branching fractions by the result for yields the and .
This analysis is based on the full data sample of 711 fb*-1* collected at the resonance by the Belle detector Belle at the KEKB asymmetric-energy collider KEKB . To determine detection efficiency and optimize signal event selections, meson decay events are generated using evtgen evtgen and inclusive decays are generated using pythia pythia . The events are then processed by a detector simulation based on geant3 geant3 . Monte Carlo (MC) simulated samples of events with or , and events with at a center-of-mass energy of GeV are used to examine possible peaking backgrounds.
Selection of signal and candidates uses well reconstructed tracks and particle identification as described in Ref. liyb . For the inclusive analysis of the decay, the tag-side meson candidate, , is reconstructed using a neural network based on a full hadron-reconstruction algorithm FR . Each candidate has an associated output value from the multivariate analysis, which ranges from 0 to 1. A candidate with larger is more likely to be a true meson. If multiple candidates are found in an event, the candidate with the largest value is selected. To improve the purity of the sample, we require , GeV/, and GeV, where the latter two intervals correspond to approximately 3 standard deviations, . and are defined as and , where is the beam energy, is the four-momentum of the daughter in the center-of-mass system (CMS). candidates are selected using the same method as in Ref. myxic . A signal region is defined by MeV/. Here and throughout the text, represents a measured invariant mass and denotes the nominal mass of the particle PDG .
The mass recoiling against the in is calculated using . To improve the recoil-mass resolution we use . Here, , and are four-momenta of the initial system, the tagged meson, and the reconstructed baryon, respectively.
Figure 1 (left) shows the distribution of of the candidates versus of the selected signal candidates after all selection requirements in the studied mass region of GeV/. Candidates are observed in the signal region defined by the solid box. To check possible peaking backgrounds, we define and sidebands, which are represented by the dashed and dash-dotted boxes. The normalized contribution of the and sidebands is estimated as being half the number of events in the blue dashed boxes minus one fourth the number of events in the red dash-dotted boxes. The distribution in the signal and the sideband boxes is shown in Figure 1 (right).
To extract the signal yields we perform an unbinned maximum likelihood fit to the distribution. A double-Gaussian function with its parameters fixed to those from a fit to the MC-simulated signal distribution is used to model the signal shape and a first-order polynomial is used for the background shape since we find no peaking background in the and sideband events. For all the fits described in this paper, the signal and background yields, and the parameters of the background shape are left free. The fit results are shown in Figure 1 (right).
The fitted number of signal events is . This corresponds to a statistical significance of estimated using , where and are the maximum likelihood values of the fits without and with a signal component, respectively. The signal significance becomes 3.1 once we convolve the likelihood with a Gaussian function whose width equals the total systematic uncertainty. The signal significance found using alternative fits to the distribution as described in the section on systematic uncertainties, is greater than 3.0 in all cases. The branching fraction is
[TABLE]
where , is the number of events, and PDG . The reconstruction efficiency, , is obtained from the MC simulation. The is taken from Ref. PDG .
For the analysis of the exclusive decays, we reconstruct from with and modes, with no . The daughters of the , , and candidates are fit to common vertices. If there is more than one candidate in an event, the one with the smallest from the vertex fit is selected. The requirements of , and are applied to reconstructed , , and candidates, respectively, with selection efficiencies above 96%, 95%, and 95%. and signals are defined as MeV/ and MeV/ corresponding to about . The signal interval is the same as in the inclusive analysis of decays. signal candidates are identified using the beam-constrained mass and the energy difference . Here, and are defined as and above, but calculated using the momenta of the signal candidate tracks directly.
After the event selections, the distributions of versus in the signal region defined by and corresponding to about are shown in Figures 2(a1) and 2(a2). The central solid boxes are the and signal regions. The backgrounds from non- and non- events are estimated with the and sidebands, represented by the dashed and dash-dotted boxes in Figures 2(a1) and 2(a2). The normalized contributions from the and sidebands are estimated using half the number of events in the blue dashed boxes minus one fourth the number of events in the red dash-dotted boxes. Figure 2 shows the and distributions in the and signal regions from the selected candidates with (b1-c1) and (b2-c2) decay modes.
We perform a two-dimensional (2D) maximum likelihood fit to the and distributions to extract the number of signal events with . For the distribution, the signal shape is modeled using a Gaussian function and the background is described using an ARGUS function argus . For the distribution, the signal shape is a double-Gaussian and the background is a first-order polynomial. All shape parameters of the signal functions are fixed to the values obtained from the fits to the MC simulated signal distributions. The fit results are shown in Figure 2.
The signal yields are (6.9 significance and 6.8 with systematic uncertainties included) and (4.5 significance and 4.4 with systematic uncertainties included). We use the efficiencies from MC simulations to measure and as and , respectively.
We divide the above product branching fractions by the value of and for the first time measure , , and the ratio between them. These are listed in Table 1.
There are several sources of systematic uncertainties in the branching fraction measurements. The uncertainties related to reconstruction efficiency include those for tracking efficiency (0.35% per track), particle identification efficiency (0.9% per kaon, 0.9% per pion, and 3.3% per proton), as well as reconstruction efficiency (3.0% per lambda ). We assume these reconstruction-efficiency-related uncertainties are independent and sum them in quadrature. We estimate the systematic uncertainties associated with the fitting procedures by changing the order of the background polynomial, the range of the fit, and by enlarging the mass resolution by 10%. The observed deviations from the nominal fit results are taken as systematic uncertainties. The uncertainty on is taken from Ref. PDG . The uncertainty due to the tagging efficiency is 4.5% FRerr . A relative systematic uncertainty on is 1.23% PDG . The systematic uncertainty on is 1.37% n4serr . For the branching fractions and the corresponding ratio, some common systematic uncertainties, including tracking, particle identification, decay branching fraction, selection, and the total number of pairs, cancel. We summarize the sources of systematic uncertainties in Table 1, assume them to be independent, and add them in quadrature to obtain the total systematic uncertainties.
We report the first measurements of the absolute branching fractions
[TABLE]
where the first uncertainties are statistical and the second systematic. The measured value is consistent with the theoretical prediction within uncertainties geng . The measured central value of is smaller than that of the theoretical predictions yu1 ; LHCB7 , perhaps indicating a large -spin symmetry breaking effect in the singly-Cabibbo-suppressed charmed-baryon decays. The branching fraction is measured for the first time to be and agrees well with that of myxic which is consistent with the expectation from isospin symmetry. The product branching fractions are
[TABLE]
The first of these branching fraction measurements is consistent with previous measurements, with improved precision, and supersedes the Belle measurement belle-old1 . The ratio is measured to be , which is consistent with world-average value of PDG within uncertainties. Our measured branching fractions, e.g. for , can be combined with branching fractions measured relative to to yield other absolute branching fractions.
In summary, based on pairs collected at the resonance with the Belle detector, we perform an analysis of inclusively using a hadronic -tagging method based on a full reconstruction algorithm FR , and exclusively with decays into and final states. These are the first measurements of the absolute branching fractions and .
We thank Professor Fu-sheng Yu for useful discussions and comments. We thank the KEKB group for excellent operation of the accelerator; the KEK cryogenics group for efficient solenoid operations; and the KEK computer group, the NII, and PNNL/EMSL for valuable computing and SINET5 network support. We acknowledge support from MEXT, JSPS and Nagoya’s TLPRC (Japan); ARC (Australia); FWF (Austria); NSFC and CCEPP (China); MSMT (Czechia); CZF, DFG, EXC153, and VS (Germany); DST (India); INFN (Italy); MOE, MSIP, NRF, RSRI, FLRFAS project and GSDC of KISTI and KREONET/GLORIAD (Korea); MNiSW and NCN (Poland); MSHE (Russia); ARRS (Slovenia); IKERBASQUE (Spain); SNSF (Switzerland); MOE and MOST (Taiwan); and DOE and NSF (USA).
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