Zur Hauptnavigation wechseln Zur Suche wechseln Zum Hauptinhalt wechseln

Study of electromagnetic decays of orbitally excited Ξc baryons

  • J. Yelton
  • , I. Adachi
  • , J. K. Ahn
  • , H. Aihara
  • , S. Al Said
  • , D. M. Asner
  • , T. Aushev
  • , R. Ayad
  • , V. Babu
  • , S. Bahinipati
  • , P. Behera
  • , C. Beleño
  • , J. Bennett
  • , V. Bhardwaj
  • , B. Bhuyan
  • , T. Bilka
  • , J. Biswal
  • , G. Bonvicini
  • , A. Bozek
  • , M. Bračko
  • T. E. Browder, M. Campajola, D. Červenkov, M. C. Chang, P. Chang, V. Chekelian, A. Chen, B. G. Cheon, K. Chilikin, K. Cho, S. J. Cho, S. K. Choi, Y. Choi, S. Choudhury, D. Cinabro, S. Cunliffe, G. De Nardo, F. Di Capua, Z. DoleŽal, T. V. Dong, S. Eidelman, D. Epifanov, T. Ferber, B. G. Fulsom, R. Garg, V. Gaur, N. Gabyshev, A. Garmash, A. Giri, P. Goldenzweig, C. Hadjivasiliou, O. Hartbrich, K. Hayasaka, H. Hayashii, M. T. Hedges, M. Hernandez Villanueva, W. S. Hou, C. L. Hsu, T. Iijima, K. Inami, G. Inguglia, A. Ishikawa, R. Itoh, M. Iwasaki, Y. Iwasaki, W. W. Jacobs, S. Jia, Y. Jin, C. W. Joo, K. K. Joo, A. B. Kaliyar, K. H. Kang, G. Karyan, Y. Kato, T. Kawasaki, H. Kichimi, C. Kiesling, B. H. Kim, D. Y. Kim, S. H. Kim, Y. K. Kim, K. Kinoshita, P. Kodyš, S. Korpar, D. Kotchetkov, P. KriŽan, R. Kroeger, P. Krokovny, R. Kulasiri, R. Kumar, K. Kumara, A. Kuzmin, Y. J. Kwon, K. Lalwani, J. S. Lange, S. C. Lee, P. Lewis, L. K. Li, Y. B. Li, L. Li Gioi, J. Libby, K. Lieret, Z. Liptak, D. Liventsev, T. Luo, C. MacQueen, M. Masuda, T. Matsuda, D. Matvienko, J. T. McNeil, M. Merola, K. Miyabayashi, H. Miyata, R. Mizuk, G. B. Mohanty, S. Mohanty, T. J. Moon, T. Mori, M. Mrvar, R. Mussa, E. Nakano, M. Nakao, Z. Natkaniec, A. Natochii, M. Nayak, N. K. Nisar, S. Nishida, K. Ogawa, S. Ogawa, H. Ono, Y. Onuki, P. Oskin, P. Pakhlov, G. Pakhlova, S. Pardi, H. Park, S. H. Park, S. Patra, S. Paul, T. K. Pedlar, R. Pestotnik, L. E. Piilonen, T. Podobnik, V. Popov, E. Prencipe, M. T. Prim, M. Ritter, A. Rostomyan, N. Rout, G. Russo, D. Sahoo, Y. Sakai, S. Sandilya, L. Santelj, T. Sanuki, V. Savinov, G. Schnell, J. Schueler, C. Schwanda, Y. Seino, K. Senyo, M. E. Sevior, M. Shapkin, V. Shebalin, C. P. Shen, J. G. Shiu, B. Shwartz, J. B. Singh, A. Sokolov, E. Solovieva, M. Starič, Z. S. Stottler, J. F. Strube, M. Sumihama, K. Sumisawa, T. Sumiyoshi, W. Sutcliffe, M. Takizawa, U. Tamponi, K. Tanida, F. Tenchini, M. Uchida, T. Uglov, Y. Unno, S. Uno, P. Urquijo, Y. Usov, S. E. Vahsen, R. Van Tonder, G. Varner, A. Vinokurova, V. Vorobyev, E. Waheed, C. H. Wang, E. Wang, M. Z. Wang, P. Wang, X. L. Wang, M. Watanabe, E. Won, X. Xu, B. D. Yabsley, W. Yan, S. B. Yang, H. Ye, J. H. Yin, Z. P. Zhang, V. Zhilich, V. Zhukova, V. Zhulanov
  • University of Florida
  • KEK and Graduate University for Advanced Studies (Sokendai)
  • High Energy Accelerator Research Organization (KEK)
  • Korea University
  • University of Tokyo
  • Faculty of Sciences, King Abdulaziz University
  • University of Tabuk
  • Brookhaven National Laboratory
  • National Research University Higher School of Economics
  • Deutsches Elektronen-Synchrotron (DESY)
  • Indian Institute of Technology Bhubaneswar
  • Indian Institute of Technology Madras
  • Georg August Universität Göttingen
  • University of Mississippi
  • Indian Institute of Science Education and Research Mohali
  • Indian Institute of Technology Guwahati
  • Charles University
  • Jožef Stefan Institute
  • Wayne State University
  • Henryk Niewodniczanski Institute of Nuclear Physics Polish Academy of Sciences
  • University of Maribor
  • University of Hawaii
  • INFN Sezione di Napoli
  • Università di Napoli Federico II
  • Fu Jen Catholic University
  • National Taiwan University
  • Max-Planck-Institut für Physik
  • National Central University
  • Hanyang University
  • P.N. Lebedev Physical Institute of the Russian Academy of Sciences
  • Korea Institute of Science and Technology Information
  • Yonsei University
  • Gyeongsang National University
  • Sungkyunkwan University
  • Indian Institute of Technology Hyderabad
  • Fudan University
  • Budker Institute of Nuclear Physics (SB RAS)
  • Novosibirsk State University
  • Pacific Northwest National Laboratory
  • Panjab University
  • Virginia Polytechnic Institute and State University
  • Humanoid Technologies Lab (H2T)
  • Niigata University
  • Nara Women's University
  • University of Sydney
  • Nagoya University
  • Österreichische Akademie der Wissenschaften
  • Osaka Prefecture University
  • Indiana University Bloomington
  • Chonnam National University
  • Tata Institute of Fundamental Research, Mumbai
  • Kyungpook National University
  • Kitasato University
  • Seoul National University
  • Soongsil University
  • Univ. of Cincinnati
  • Univ. of Ljubljana
  • Kennesaw State University
  • Punjab Agricultural University
  • Malaviya National Institute of Technology Jaipur
  • Justus-Liebig-Universität Gießen
  • University of Bonn
  • Beijing University
  • University of Munich
  • University of Melbourne
  • Osaka University
  • University of Miyazaki
  • Utkal University
  • INFN Sez. di Torino
  • Tel Aviv University
  • Toho University
  • Nippon Dental University
  • National Research Nuclear University MEPhI
  • Luther College, Decorah
  • Forschungszentrum Jülich (FZJ)
  • Tohoku University
  • University of Pittsburgh
  • Biodonostia Health Research Institute-CIBERNED-UPV-EHU
  • Basque Foundation for Science
  • Yamagata University
  • Institute for High Energy Physics (IHEP)
  • Gifu University
  • Tokyo Metropolitan University
  • Showa Pharmaceutical University
  • Japan Atomic Energy Agency
  • Tokyo Institute of Technology
  • National United University
  • Institute of High Energy Physics Chinese Academy of Science
  • Soochow University
  • University of Science and Technology of China

Publikation: Beitrag in FachzeitschriftArtikelBegutachtung

17 Zitate (Scopus)

Abstract

Using 980 fb-1 of data collected with the Belle detector operating at the KEKB asymmetric-energy e+e- collider, we report a study of the electromagnetic decays of excited charmed baryons Ξc(2790) and Ξc(2815). A clear signal (8.6 standard deviations) is observed for Ξc(2815)0→Ξc0γ, and we measure: B[Ξc(2815)0 → Ξc0γ]B[Ξc(2815)0 → Ξc(2645)+π- → Ξc0π+π-]=0.41±0.05±0.03. We also present evidence (3.8 standard deviations) for the similar decay of the Ξc(2790)0 and measure: B[Ξc(2790)0 → Ξc0γ]B[Ξc(2790)0 → Ξc′+π- → Ξc+γπ-]=0.13±0.03±0.02. The first quoted uncertainties are statistical and the second systematic. We find no hint of the analogous decays of the Ξc(2815)+ and Ξc(2790)+ baryons and set upper limits at the 90% confidence level of: B[Ξc(2815)+ → Ξc+γ]B[Ξc(2815)+ → Ξc(2645)0π+ → Ξc+π-π+]<0.09, and B[Ξc(2790)+ → Ξc+γ]B[Ξc(2790)+ → Ξc′0π+ → Ξc0γπ+]<0.06. Approximate values of the partial widths of the decays are extracted, which can be used to discriminate between models of the underlying quark structure of these excited states.

OriginalspracheEnglisch
Aufsatznummer071103
FachzeitschriftPhysical Review D
Jahrgang102
Ausgabenummer7
DOIs
PublikationsstatusVeröffentlicht - 26 Okt. 2020

Fingerprint

Untersuchen Sie die Forschungsthemen von „Study of electromagnetic decays of orbitally excited Ξc baryons“. Zusammen bilden sie einen einzigartigen Fingerprint.

Dieses zitieren