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Observation of $X(3872)$ in $B \to X(3872) K\pi$ decays

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arxiv 1501.06867 v2 pith:XMGZH7K4 submitted 2015-01-27 hep-ex

A. Bala , V. Bhardwaj , K. Trabelsi , J. B. Singh , A. Abdesselam , I. Adachi , H. Aihara , K. Arinstein
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D. M. Asner V. Aulchenko T. Aushev R. Ayad T. Aziz S. Bahinipati A. M. Bakich V. Bansal E. Barberio B. Bhuyan A. Bobrov G. Bonvicini A. Bozek M. Bračko T. E. Browder D. Červenkov A. Chen B. G. Cheon R. Chistov K. Cho V. Chobanova S.-K. Choi Y. Choi D. Cinabro J. Dalseno J. Dingfelder Z. Doležal A. Drutskoy D. Dutta S. Eidelman D. Epifanov H. Farhat J. E. Fast T. Ferber O. Frost V. Gaur N. Gabyshev A. Garmash D. Getzkow Y. M. Goh B. Golob O. Grzymkowska J. Haba T. Hara H. Hayashii X. H. He A. Heller T. Horiguchi W.-S. Hou M. Huschle T. Iijima A. Ishikawa R. Itoh Y. Iwasaki I. Jaegle D. Joffe K. H. Kang E. Kato T. Kawasaki C. Kiesling D. Y. Kim J. B. Kim J. H. Kim K. T. Kim M. J. Kim S. H. Kim Y. J. Kim K. Kinoshita B. R. Ko P. Kodyš S. Korpar P. Križan P. Krokovny T. Kuhr R. Kumar A. Kuzmin Y.-J. Kwon J. S. Lange I. S. Lee Y. Li L. Li Gioi J. Libby D. Liventsev P. Lukin D. Matvienko K. Miyabayashi H. Miyake H. Miyata R. Mizuk G. B. Mohanty S. Mohanty A. Moll H. K. Moon R. Mussa E. Nakano M. Nakao Z. Natkaniec M. Nayak N. K. Nisar S. Nishida S. Ogawa S. Okuno S. L. Olsen P. Pakhlov G. Pakhlova C. W. Park H. Park R. Pestotnik M. Petrič L. E. Piilonen E. Ribežl M. Ritter Y. Sakai S. Sandilya L. Santelj T. Sanuki V. Savinov O. Schneider G. Schnell C. Schwanda K. Senyo O. Seon M. E. Sevior V. Shebalin C. P. Shen T.-A. Shibata J.-G. Shiu B. Shwartz A. Sibidanov F. Simon Y.-S. Sohn A. Sokolov E. Solovieva M. Starič M. Steder M. Sumihama T. Sumiyoshi K. Tanida G. Tatishvili Y. Teramoto F. Thorne V. Trusov M. Uchida S. Uehara T. Uglov Y. Unno S. Uno P. Urquijo Y. Usov P. Vanhoefer G. Varner A. Vinokurova V. Vorobyev M. N. Wagner C. H. Wang X. L. Wang Y. Watanabe K. M. Williams E. Won H. Yamamoto Y. Yamashita S. Yashchenko C. Z. Yuan Z. P. Zhang V. Zhilich V. Zhulanov M. Ziegler A. Zupanc
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abstract

We report the first observation of $B^0 \to X(3872) (K^{+}\pi^{-})$ and evidence for $B^+ \to X(3872) (K^{0}\pi^{+})$. We measure the product of branching fractions for the former to be ${\cal B}(B^0 \to X(3872) (K^+ \pi^-)) \times {\cal B}(X(3872) \to J/\psi \pi^+ \pi^-) = (7.9 \pm 1.3(\mbox{stat.})\pm 0.4(\mbox{syst.})) \times 10^{-6}$ and find that $B^{0}\to X(3872) K^{*}(892)^{0}$ does not dominate the $B^{0}\to X(3872)K^{+}\pi^{-}$ decay mode. We also measure ${\cal B}(B^+ \to X(3872) (K^0 \pi^+)) \times {\cal B}(X(3872) \to J/\psi \pi^+ \pi^-) = (10.6 \pm 3.0(\mbox{stat.}) \pm 0.9(\mbox{syst.})) \times 10^{-6}$. This study is based on the full data sample of 711~fb$^{-1}$ ($772\times 10^6 B\bar B$ pairs) collected at the $\Upsilon(4S)$ resonance with the Belle detector at the KEKB collider.

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  1. Radiative decay of $\chi_{c1}$ states in effective Lagrangian approach

    hep-ph 2025-06 conditional novelty 4.0 of 10

    A triangle-loop effective Lagrangian model predicts chi_c1(3872) radiative branching fractions tens of times above LHCb measurements, supporting a non-charmonium interpretation.

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