학술논문

Precise determination of the CKM matrix element $\left| V_{cb}\right|$ with $\bar B^0 \to D^{*\,+} \, \ell^- \, \bar \nu_\ell$ decays with hadronic tagging at Belle
Document Type
Working Paper
Author
The Belle CollaborationAbdesselam, A.Adachi, I.Adamczyk, K.Aihara, H.Said, S. AlArinstein, K.Arita, Y.Asner, D. M.Aso, T.Atmacan, H.Aulchenko, V.Aushev, T.Ayad, R.Aziz, T.Babu, V.Badhrees, I.Bahinipati, S.Bakich, A. M.Bala, A.Ban, Y.Bansal, V.Barberio, E.Barrett, M.Bartel, W.Bay, A.Behera, P.Belhorn, M.Belous, K.Berger, M.Bernlochner, F. U.Besson, D.Bhardwaj, V.Bhuyan, B.Biswal, J.Bloomfield, T.Blyth, S.Bobrov, A.Bondar, A.Bonvicini, G.Bookwalter, C.Boulahouache, C.Bozek, A.Bračko, M.Braun, N.Breibeck, F.Brodzicka, J.Browder, T. E.Waheed, E.Červenkov, D.Chang, M. -C.Chang, P.Chao, Y.Chekelian, V.Chen, A.Chen, K. -F.Chen, P.Cheon, B. G.Chilikin, K.Chistov, R.Cho, K.Chobanova, V.Choi, S. -K.Choi, Y.Cinabro, D.Crnkovic, J.Dalseno, J.Danilov, M.Dash, N.Di Carlo, S.Dingfelder, J.Doležal, Z.Dossett, D.Drásal, Z.Drutskoy, A.Dubey, S.Dutta, D.Dutta, K.Eidelman, S.Epifanov, D.Falke, S.Farhat, H.Fast, J. E.Feindt, M.Ferber, T.Frey, A.Frost, O.Fulsom, B. G.Gaur, V.Gabyshev, N.Ganguly, S.Garmash, A.Gelb, M.Gemmler, J.Getzkow, D.Gillard, R.Giordano, F.Glattauer, R.Goh, Y. M.Goldenzweig, P.Golob, B.Greenwald, D.Perdekamp, M. GrosseGrygier, J.Grzymkowska, O.Guan, Y.Guido, E.Guo, H.Haba, J.Hamer, P.Han, Y. L.Hara, K.Hara, T.Hasegawa, Y.Hasenbusch, J.Hayasaka, K.Hayashii, H.He, X. H.Heck, M.Hedges, M. T.Heffernan, D.Heider, M.Heller, A.Higuchi, T.Himori, S.Hirose, S.Horiguchi, T.Hoshi, Y.Hoshina, K.Hou, W. -S.Hsiung, Y. B.Hsu, C. -L.Huschle, M.Hyun, H. J.Igarashi, Y.Iijima, T.Imamura, M.Inami, K.Inguglia, G.Ishikawa, A.Itagaki, K.Itoh, R.Iwabuchi, M.Iwasaki, M.Iwasaki, Y.Iwata, S.Jacobs, W. W.Jaegle, I.Jeon, H. B.Jia, S.Jin, Y.Joffe, D.Jones, M.Joo, K. K.Julius, T.Kahn, J.Kakuno, H.Kaliyar, A. B.Kang, J. H.Kang, K. H.Kapusta, P.Karyan, G.Kataoka, S. U.Kato, E.Kato, Y.Katrenko, P.Kawai, H.Kawasaki, T.Keck, T.Kichimi, H.Kiesling, C.Kim, B. H.Kim, D. Y.Kim, H. J.Kim, H. -J.Kim, J. B.Kim, J. H.Kim, K. T.Kim, M. J.Kim, S. H.Kim, S. K.Kim, Y. J.Kinoshita, K.Kleinwort, C.Klucar, J.Ko, B. R.Kobayashi, N.Koblitz, S.Kodyš, P.Koga, Y.Korpar, S.Kotchetkov, D.Kouzes, R. T.Križan, P.Krokovny, P.Kronenbitter, B.Kuhr, T.Kulasiri, R.Kumar, R.Kumita, T.Kurihara, E.Kuroki, Y.Kuzmin, A.Kvasnička, P.Kwon, Y. -J.Lai, Y. -T.Lange, J. S.Lee, D. H.Lee, I. S.Lee, S. -H.Leitgab, M.Leitner, R.Levit, D.Lewis, P.Li, C. H.Li, H.Li, J.Li, L.Li, X.Li, Y.Gioi, L. LiLibby, J.Limosani, A.Liu, C.Liu, Y.Liu, Z. Q.Liventsev, D.Loos, A.Louvot, R.Lubej, M.Lukin, P.Luo, T.MacNaughton, J.Masuda, M.Matsuda, T.Matvienko, D.Matyja, A.Metzner, F.McOnie, S.Mikami, Y.Miyabayashi, K.Miyachi, Y.Miyake, H.Miyata, H.Miyazaki, Y.Mizuk, R.Mohanty, G. B.Mohanty, S.Mohapatra, D.Moll, A.Moon, H. K.Mori, T.Morii, T.Moser, H. -G.Mrvar, M.Müller, T.Muramatsu, N.Mussa, R.Nagamine, T.Nagasaka, Y.Nakahama, Y.Nakamura, I.Nakamura, K. R.Nakano, E.Nakano, H.Nakano, T.Nakao, M.Nakayama, H.Nakazawa, H.Nanut, T.Nath, K. J.Natkaniec, Z.Nayak, M.Nedelkovska, E.Negishi, K.Neichi, K.Ng, C.Niebuhr, C.Niiyama, M.Nisar, N. K.Nishida, S.Nishimura, K.Nitoh, O.Nozaki, T.Ogawa, A.Ogawa, S.Ohshima, T.Okuno, S.Olsen, S. L.Ono, H.Ono, Y.Onuki, Y.Ostrowicz, W.Oswald, C.Ozaki, H.Pakhlov, P.Pakhlova, G.Pal, B.Palka, H.Panzenböck, E.Park, C. -S.Park, C. W.Park, H.Park, K. S.Paul, S.Peak, L. S.Pedlar, T. K.Peng, T.Pesántez, L.Pestotnik, R.Peters, M.Petrič, M.Piilonen, L. E.Poluektov, A.Prasanth, K.Prim, M.Prothmann, K.Pulvermacher, C.Purohit, M. V.Rauch, J.Reisert, B.Ribežl, E.Ritter, M.Rorie, J.Rostomyan, A.Rozanska, M.Rummel, S.Ryu, S.Sahoo, H.Salehi, M.Saito, T.Sakai, K.Sakai, Y.Sandilya, S.Santel, D.Santelj, L.Sanuki, T.Sasaki, J.Sasao, N.Sato, Y.Savinov, V.Schlüter, T.Schneider, O.Schnell, G.Schönmeier, P.Schram, M.Schwanda, C.Schwartz, A. J.Schwenker, B.Seidl, R.Seino, Y.Semmler, D.Senyo, K.Seon, O.Seong, I. S.Sevior, M. E.Shang, L.Shapkin, M.Shebalin, V.Shen, C. P.Shibata, T. -A.Shibuya, H.Shimizu, N.Shinomiya, S.Shiu, J. -G.Shwartz, B.Sibidanov, A.Simon, F.Singh, J. B.Sinha, R.Smerkol, P.Sohn, Y. -S.Sokolov, A.Soloviev, Y.Solovieva, E.Stanič, S.Starič, M.Steder, M.Strube, J. F.Stypula, J.Sugihara, S.Sugiyama, A.Sumihama, M.Sumisawa, K.Sumiyoshi, T.Suzuki, K.Suzuki, S.Suzuki, S. Y.Suzuki, Z.Takeichi, H.Takizawa, M.Tamponi, U.Tanaka, M.Tanaka, S.Tanida, K.Taniguchi, N.Taylor, G. N.Tenchini, F.Teramoto, Y.Tikhomirov, I.Trabelsi, K.Trusov, V.Tsuboyama, T.Uchida, M.Uchida, T.Uehara, S.Ueno, K.Uglov, T.Unno, Y.Uno, S.Uozumi, S.Urquijo, P.Ushiroda, Y.Usov, Y.Vahsen, S. E.Van Hulse, C.Vanhoefer, P.Varner, G.Varvell, K. E.Vervink, K.Vinokurova, A.Vorobyev, V.Vossen, A.Wagner, M. N.Wang, B.Wang, C. H.Wang, J.Wang, M. -Z.Wang, P.Wang, X. L.Watanabe, M.Watanabe, Y.Wedd, R.Wehle, S.White, E.Widmann, E.Wiechczynski, J.Williams, K. M.Won, E.Yabsley, B. D.Yamada, S.Yamamoto, H.Yamaoka, J.Yamashita, Y.Yamauchi, M.Yashchenko, S.Ye, H.Yelton, J.Yook, Y.Yuan, C. Z.Yusa, Y.Zhang, C. C.Zhang, L. M.Zhang, Z. P.Zhao, L.Zhilich, V.Zhukova, V.Zhulanov, V.Ziegler, M.Zivko, T.Zupanc, A.Zwahlen, N.
Source
Subject
High Energy Physics - Experiment
Language
Abstract
The precise determination of the CKM matrix element $\left| V_{cb}\right|$ is important for carrying out tests of the flavour sector of the Standard Model. In this article we present a preliminary analysis of the $\bar B^0 \to D^{*\,+} \, \ell^- \, \bar \nu_\ell$ decay mode and its charge conjugate, selected in events that contain a fully reconstructed $B$-meson, using 772 million $e^+ \, e^- \to \Upsilon(4S) \to B \bar B$ events recorded by the Belle detector at KEKB. Unfolded differential decay rates of four kinematic variables fully describing the $\bar B^0 \to D^{*\,+} \, \ell^- \, \bar \nu_\ell$ decay in the $B$-meson rest frame are presented. We measure the total branching fraction $\mathcal{B}( \bar B^0 \to D^{*\,+} \, \ell^- \, \bar \nu_\ell ) = \left(4.95 \pm 0.11 \pm 0.22 \right) \times 10^{-2}$, where the errors are statistical and systematic respectively. The value of $\left|V_{cb} \right|$ is determined to be $\left( 37.4 \pm 1.3 \right) \times 10^{-3}$. Both results are in good agreement with current world averages.