| Literature DB >> 24074072 |
J P Lees1, V Poireau, V Tisserand, E Grauges, A Palano, G Eigen, B Stugu, D N Brown, L T Kerth, Yu G Kolomensky, M J Lee, G Lynch, H Koch, T Schroeder, C Hearty, T S Mattison, J A McKenna, R Y So, A Khan, V E Blinov, A R Buzykaev, V P Druzhinin, V B Golubev, E A Kravchenko, A P Onuchin, S I Serednyakov, Yu I Skovpen, E P Solodov, K Yu Todyshev, A N Yushkov, D Kirkby, A J Lankford, M Mandelkern, B Dey, J W Gary, O Long, G M Vitug, C Campagnari, M Franco Sevilla, T M Hong, D Kovalskyi, J D Richman, C A West, A M Eisner, W S Lockman, A J Martinez, B A Schumm, A Seiden, D S Chao, C H Cheng, B Echenard, K T Flood, D G Hitlin, P Ongmongkolkul, F C Porter, R Andreassen, C Fabby, Z Huard, B T Meadows, M D Sokoloff, L Sun, P C Bloom, W T Ford, A Gaz, U Nauenberg, J G Smith, S R Wagner, R Ayad, W H Toki, B Spaan, K R Schubert, R Schwierz, D Bernard, M Verderi, S Playfer, D Bettoni, C Bozzi, R Calabrese, G Cibinetto, E Fioravanti, I Garzia, E Luppi, L Piemontese, V Santoro, R Baldini-Ferroli, A Calcaterra, R de Sangro, G Finocchiaro, S Martellotti, P Patteri, I M Peruzzi, M Piccolo, M Rama, A Zallo, R Contri, E Guido, M Lo Vetere, M R Monge, S Passaggio, C Patrignani, E Robutti, B Bhuyan, V Prasad, M Morii, A Adametz, U Uwer, H M Lacker, P D Dauncey, U Mallik, C Chen, J Cochran, W T Meyer, S Prell, A E Rubin, A V Gritsan, N Arnaud, M Davier, D Derkach, G Grosdidier, F Le Diberder, A M Lutz, B Malaescu, P Roudeau, A Stocchi, G Wormser, D J Lange, D M Wright, J P Coleman, J R Fry, E Gabathuler, D E Hutchcroft, D J Payne, C Touramanis, A J Bevan, F Di Lodovico, R Sacco, G Cowan, J Bougher, D N Brown, C L Davis, A G Denig, M Fritsch, W Gradl, K Griessinger, A Hafner, E Prencipe, R J Barlow, G D Lafferty, E Behn, R Cenci, B Hamilton, A Jawahery, D A Roberts, R Cowan, D Dujmic, G Sciolla, R Cheaib, P M Patel, S H Robertson, P Biassoni, N Neri, F Palombo, L Cremaldi, R Godang, P Sonnek, D J Summers, X Nguyen, M Simard, P Taras, G De Nardo, D Monorchio, G Onorato, C Sciacca, M Martinelli, G Raven, C P Jessop, J M LoSecco, K Honscheid, R Kass, J Brau, R Frey, N B Sinev, D Strom, E Torrence, E Feltresi, M Margoni, M Morandin, M Posocco, M Rotondo, G Simi, F Simonetto, R Stroili, S Akar, E Ben-Haim, M Bomben, G R Bonneaud, H Briand, G Calderini, J Chauveau, Ph Leruste, G Marchiori, J Ocariz, S Sitt, M Biasini, E Manoni, S Pacetti, A Rossi, C Angelini, G Batignani, S Bettarini, M Carpinelli, G Casarosa, A Cervelli, F Forti, M A Giorgi, A Lusiani, B Oberhof, E Paoloni, A Perez, G Rizzo, J J Walsh, D Lopes Pegna, J Olsen, A J S Smith, R Faccini, F Ferrarotto, F Ferroni, M Gaspero, L Li Gioi, G Piredda, C Bünger, O Grünberg, T Hartmann, T Leddig, C Voß, R Waldi, T Adye, E O Olaiya, F F Wilson, S Emery, G Hamel de Monchenault, G Vasseur, Ch Yèche, F Anulli, D Aston, D J Bard, J F Benitez, C Cartaro, M R Convery, J Dorfan, G P Dubois-Felsmann, W Dunwoodie, M Ebert, R C Field, B G Fulsom, A M Gabareen, M T Graham, C Hast, W R Innes, P Kim, M L Kocian, D W G S Leith, P Lewis, D Lindemann, B Lindquist, S Luitz, V Luth, H L Lynch, D B MacFarlane, D R Muller, H Neal, S Nelson, M Perl, T Pulliam, B N Ratcliff, A Roodman, A A Salnikov, R H Schindler, A Snyder, D Su, M K Sullivan, J Va'vra, A P Wagner, W F Wang, W J Wisniewski, M Wittgen, D H Wright, H W Wulsin, V Ziegler, W Park, M V Purohit, R M White, J R Wilson, A Randle-Conde, S J Sekula, M Bellis, P R Burchat, T S Miyashita, E M T Puccio, M S Alam, J A Ernst, R Gorodeisky, N Guttman, D R Peimer, A Soffer, S M Spanier, J L Ritchie, A M Ruland, R F Schwitters, B C Wray, J M Izen, X C Lou, F Bianchi, F De Mori, A Filippi, D Gamba, S Zambito, L Lanceri, L Vitale, F Martinez-Vidal, A Oyanguren, P Villanueva-Perez, H Ahmed, J Albert, Sw Banerjee, F U Bernlochner, H H F Choi, G J King, R Kowalewski, M J Lewczuk, T Lueck, I M Nugent, J M Roney, R J Sobie, N Tasneem, T J Gershon, P F Harrison, T E Latham, H R Band, S Dasu, Y Pan, R Prepost, S L Wu.
Abstract
We measure the mass difference Δm0 between the D*(2010)+ and the D0 and the natural linewidth Γ of the transition D*(2010)+ → D0π+. The data were recorded with the BABAR detector at center-of-mass energies at and near the Υ(4S) resonance, and correspond to an integrated luminosity of approximately 477 fb(-1). The D0 is reconstructed in the decay modes D0 → K- π+ and D0 → K- π+ π- π+. For the decay mode D0 → K- π+ we obtain Γ = (83.4±1.7±1.5) keV and Δm0 = (145425.6±0.6±1.7) keV, [corrected] where the quoted errors are statistical and systematic, respectively. For the D0 → K- π+ π- π+ mode we obtain Γ = (83.2±1.5±2.6) keV and Δm0 = (145426.6±0.5±1.9) keV. [corrected] The combined measurements yield Γ = (83.3±1.2±1.4) keV and Δm0 = (145425.9±0.4±1.7) keV; the width is a factor of approximately 12 times more precise than the previous value, while the mass difference is a factor of approximately 6 times more precise.Entities:
Year: 2013 PMID： 24074072 DOI： 10.1103/PhysRevLett.111.111801
Source DB: PubMed Journal: Phys Rev Lett ISSN： 0031-9007 Impact factor: 9.161