Standard

Observation of the Singly Cabibbo Suppressed Decay ?c+ ?np+. / The BESIII Collaboration.

в: Physical Review Letters, Том 128, № 14, 142001, 08.04.2022.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

The BESIII Collaboration 2022, 'Observation of the Singly Cabibbo Suppressed Decay ?c+ ?np+', Physical Review Letters, Том. 128, № 14, 142001. https://doi.org/10.1103/PhysRevLett.128.142001

APA

The BESIII Collaboration (2022). Observation of the Singly Cabibbo Suppressed Decay ?c+ ?np+. Physical Review Letters, 128(14), [142001]. https://doi.org/10.1103/PhysRevLett.128.142001

Vancouver

The BESIII Collaboration. Observation of the Singly Cabibbo Suppressed Decay ?c+ ?np+. Physical Review Letters. 2022 апр. 8;128(14):142001. doi: 10.1103/PhysRevLett.128.142001

Author

The BESIII Collaboration. / Observation of the Singly Cabibbo Suppressed Decay ?c+ ?np+. в: Physical Review Letters. 2022 ; Том 128, № 14.

BibTeX

@article{23bd267d86c14901adb3972554f52d7f,
title = "Observation of the Singly Cabibbo Suppressed Decay ?c+ ?np+",
abstract = "The singly Cabibbo-suppressed decay ?c+?np+ is observed for the first time with a statistical significance of 7.3s by using 3.9 fb-1 of e+e-collision data collected at center-of-mass energies between 4.612 and 4.699 GeV with the BESIII detector at BEPCII. The branching fraction of ?c+?np+ is measured to be (6.6±1.2stat±0.4syst)×10-4. By taking the upper limit of branching fractions of ?c+?pp0 from the Belle experiment, the ratio of branching fractions between ?c+?np+ and ?c+?pp0 is calculated to be larger than 7.2 at the 90% confidence level, which disagrees with most predictions of the available phenomenological models. In addition, the branching fractions of the Cabibbo-favored decays ?c+?p+ and ?c+?0p+ are measured to be (1.31±0.08stat±0.05syst)×10-2 and (1.22±0.08stat±0.07syst)×10-2, respectively, which are consistent with previous results. ",
author = "{BESIII Collaboration} and M. Ablikim and Achasov, {M. N.} and P. Adlarson and S. Ahmed and M. Albrecht and R. Aliberti and A. Amoroso and An, {M. R.} and Q. An and Bai, {X. H.} and Y. Bai and O. Bakina and Ferroli, {R. Baldini} and I. Balossino and Y. Ban and K. Begzsuren and N. Berger and M. Bertani and D. Bettoni and F. Bianchi and J. Bloms and A. Bortone and I. Boyko and Briere, {R. A.} and H. Cai and X. Cai and A. Calcaterra and Cao, {G. F.} and N. Cao and Cetin, {S. A.} and Chang, {J. F.} and Chang, {W. L.} and G. Chelkov and Chen, {D. Y.} and G. Chen and Chen, {H. S.} and Chen, {M. L.} and Chen, {S. J.} and Chen, {X. R.} and Chen, {Y. B.} and Chen, {Z. J.} and Cheng, {W. S.} and G. Cibinetto and F. Cossio and Cui, {X. F.} and Dai, {H. L.} and Dai, {J. P.} and Dai, {X. C.} and Muchnoi, {N. Yu} and Nikolaev, {I. B.}",
note = "Funding Information: The BESIII Collaboration thanks the staff of BEPCII, the IHEP computing center, and the supercomputing center of the University of Science and Technology of China (USTC) for their strong support. The authors are grateful to Hai-Yang Cheng, Fanrong Xu, and Xianwei Kang for enlightening discussions. This work is supported in part by National Key R&D Program of China under Contracts No. 2020YFA0406400, No. 2020YFA0406300; National Natural Science Foundation of China (NSFC) under Contracts No. 11335008, No. 11625523, No. 11635010, No. 11735014, No. 11822506, No. 11835012, No. 11935015, No. 11935016, No. 11935018, No. 11961141012, No. 12022510, No. 12025502, No. 12035009, No. 12035013, No. 12061131003, No. 12005311, No. 11805086, No. 11705192, and No. 11950410506; the Fundamental Research Funds for the Central Universities, University of Science and Technology of China, Sun Yat-sen University, Lanzhou University, University of Chinese Academy of Sciences; 100 Talents Program of Sun Yat-sen University; the Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program; Joint Large-Scale Scientific Facility Funds of the NSFC and CAS under Contracts No. U1732263, No. U1832207, No. U1832103, No. U2032111; CAS Key Research Program of Frontier Sciences under Contract No. QYZDJ-SSW-SLH040; 100 Talents Program of CAS; China Postdoctoral Science Foundation under Contracts No. 2019M662152, No. 2020T130636; INPAC and Shanghai Key Laboratory for Particle Physics and Cosmology; ERC under Contract No. 758462; European Union Horizon 2020 research and innovation programme under Marie Sk{\l}odowska-Curie Grant Agreement No. 894790; German Research Foundation DFG under Contracts No. 443159800, Collaborative Research Center CRC 1044, FOR 2359, FOR 2359, GRK 214; Istituto Nazionale di Fisica Nucleare, Italy; Ministry of Development of Turkey under Contract No. DPT2006K-120470; National Science and Technology fund; Olle Engkvist Foundation under Contract No. 200-0605; STFC (U.K.); The Knut and Alice Wallenberg Foundation (Sweden) under Contract No. 2016.0157; The Royal Society, U.K. under Contracts No. DH140054, No. DH160214; The Swedish Research Council; U.S. Department of Energy under Contracts No. DE-FG02-05ER41374, No. DE-SC-0012069. Publisher Copyright: {\textcopyright} 2022 authors. Published by the American Physical Society.",
year = "2022",
month = apr,
day = "8",
doi = "10.1103/PhysRevLett.128.142001",
language = "English",
volume = "128",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "14",

}

RIS

TY - JOUR

T1 - Observation of the Singly Cabibbo Suppressed Decay ?c+ ?np+

AU - BESIII Collaboration

AU - Ablikim, M.

AU - Achasov, M. N.

AU - Adlarson, P.

AU - Ahmed, S.

AU - Albrecht, M.

AU - Aliberti, R.

AU - Amoroso, A.

AU - An, M. R.

AU - An, Q.

AU - Bai, X. H.

AU - Bai, Y.

AU - Bakina, O.

AU - Ferroli, R. Baldini

AU - Balossino, I.

AU - Ban, Y.

AU - Begzsuren, K.

AU - Berger, N.

AU - Bertani, M.

AU - Bettoni, D.

AU - Bianchi, F.

AU - Bloms, J.

AU - Bortone, A.

AU - Boyko, I.

AU - Briere, R. A.

AU - Cai, H.

AU - Cai, X.

AU - Calcaterra, A.

AU - Cao, G. F.

AU - Cao, N.

AU - Cetin, S. A.

AU - Chang, J. F.

AU - Chang, W. L.

AU - Chelkov, G.

AU - Chen, D. Y.

AU - Chen, G.

AU - Chen, H. S.

AU - Chen, M. L.

AU - Chen, S. J.

AU - Chen, X. R.

AU - Chen, Y. B.

AU - Chen, Z. J.

AU - Cheng, W. S.

AU - Cibinetto, G.

AU - Cossio, F.

AU - Cui, X. F.

AU - Dai, H. L.

AU - Dai, J. P.

AU - Dai, X. C.

AU - Muchnoi, N. Yu

AU - Nikolaev, I. B.

N1 - Funding Information: The BESIII Collaboration thanks the staff of BEPCII, the IHEP computing center, and the supercomputing center of the University of Science and Technology of China (USTC) for their strong support. The authors are grateful to Hai-Yang Cheng, Fanrong Xu, and Xianwei Kang for enlightening discussions. This work is supported in part by National Key R&D Program of China under Contracts No. 2020YFA0406400, No. 2020YFA0406300; National Natural Science Foundation of China (NSFC) under Contracts No. 11335008, No. 11625523, No. 11635010, No. 11735014, No. 11822506, No. 11835012, No. 11935015, No. 11935016, No. 11935018, No. 11961141012, No. 12022510, No. 12025502, No. 12035009, No. 12035013, No. 12061131003, No. 12005311, No. 11805086, No. 11705192, and No. 11950410506; the Fundamental Research Funds for the Central Universities, University of Science and Technology of China, Sun Yat-sen University, Lanzhou University, University of Chinese Academy of Sciences; 100 Talents Program of Sun Yat-sen University; the Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program; Joint Large-Scale Scientific Facility Funds of the NSFC and CAS under Contracts No. U1732263, No. U1832207, No. U1832103, No. U2032111; CAS Key Research Program of Frontier Sciences under Contract No. QYZDJ-SSW-SLH040; 100 Talents Program of CAS; China Postdoctoral Science Foundation under Contracts No. 2019M662152, No. 2020T130636; INPAC and Shanghai Key Laboratory for Particle Physics and Cosmology; ERC under Contract No. 758462; European Union Horizon 2020 research and innovation programme under Marie Skłodowska-Curie Grant Agreement No. 894790; German Research Foundation DFG under Contracts No. 443159800, Collaborative Research Center CRC 1044, FOR 2359, FOR 2359, GRK 214; Istituto Nazionale di Fisica Nucleare, Italy; Ministry of Development of Turkey under Contract No. DPT2006K-120470; National Science and Technology fund; Olle Engkvist Foundation under Contract No. 200-0605; STFC (U.K.); The Knut and Alice Wallenberg Foundation (Sweden) under Contract No. 2016.0157; The Royal Society, U.K. under Contracts No. DH140054, No. DH160214; The Swedish Research Council; U.S. Department of Energy under Contracts No. DE-FG02-05ER41374, No. DE-SC-0012069. Publisher Copyright: © 2022 authors. Published by the American Physical Society.

PY - 2022/4/8

Y1 - 2022/4/8

N2 - The singly Cabibbo-suppressed decay ?c+?np+ is observed for the first time with a statistical significance of 7.3s by using 3.9 fb-1 of e+e-collision data collected at center-of-mass energies between 4.612 and 4.699 GeV with the BESIII detector at BEPCII. The branching fraction of ?c+?np+ is measured to be (6.6±1.2stat±0.4syst)×10-4. By taking the upper limit of branching fractions of ?c+?pp0 from the Belle experiment, the ratio of branching fractions between ?c+?np+ and ?c+?pp0 is calculated to be larger than 7.2 at the 90% confidence level, which disagrees with most predictions of the available phenomenological models. In addition, the branching fractions of the Cabibbo-favored decays ?c+?p+ and ?c+?0p+ are measured to be (1.31±0.08stat±0.05syst)×10-2 and (1.22±0.08stat±0.07syst)×10-2, respectively, which are consistent with previous results.

AB - The singly Cabibbo-suppressed decay ?c+?np+ is observed for the first time with a statistical significance of 7.3s by using 3.9 fb-1 of e+e-collision data collected at center-of-mass energies between 4.612 and 4.699 GeV with the BESIII detector at BEPCII. The branching fraction of ?c+?np+ is measured to be (6.6±1.2stat±0.4syst)×10-4. By taking the upper limit of branching fractions of ?c+?pp0 from the Belle experiment, the ratio of branching fractions between ?c+?np+ and ?c+?pp0 is calculated to be larger than 7.2 at the 90% confidence level, which disagrees with most predictions of the available phenomenological models. In addition, the branching fractions of the Cabibbo-favored decays ?c+?p+ and ?c+?0p+ are measured to be (1.31±0.08stat±0.05syst)×10-2 and (1.22±0.08stat±0.07syst)×10-2, respectively, which are consistent with previous results.

UR - http://www.scopus.com/inward/record.url?scp=85128907360&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.128.142001

DO - 10.1103/PhysRevLett.128.142001

M3 - Article

C2 - 35476477

AN - SCOPUS:85128907360

VL - 128

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 14

M1 - 142001

ER -

ID: 36108470