Observation ofB¯0→DsJ*(2317)+K−Decay

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ID: 269395
2005
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Abstract
The decays B¯0→DsJ+K− and B¯0→DsJ−π+ are studied for the first time. A significant signal is observed in the B¯0→DsJ*(2317)+K− decay channel with B(B¯0→DsJ*(2317)+K−)×B(DsJ*(2317)+→Ds+π0)=(5.3−1.3+1.5±0.7±1.4)×10−5. No signals are observed in the B¯0→DsJ*(2317)−π+, B¯0→DsJ(2460)+K−, and B¯0→DsJ(2460)−π+ decay modes, and upper limits are obtained. The analysis is based on a data set of 140 fb−1 collected by the Belle experiment at the asymmetric e+e− collider KEKB.
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Authors A. Drutskoy,K. Abe,I. Adachi,H. Aihara,M. Akatsu,Y. Asano,T. Aushev,S. Bahinipati,A. M. Bakich,A. Bay,I. Bedny,U. Bitenc,I. Bizjak,S. Blyth,A. Bondar,A. Bozek,M. Bračko,J. Brodzicka,T. E. Browder,Pao-Ti Chang,Y. Chao,A. Chen,Kai-Feng Chen,W. T. Chen,B. G. Cheon,R. Chistov,S.-K. Choi,Y. Choi,A. Chuvikov,S. Cole,J. Dalseno,M. Danilov,M. Dash,S. Eidelman,V. Eiges,Y. Enari,F. Fang,S. Fratina,N. Gabyshev,T. Gershon,A. Go,G. Gokhroo,B. Golob,K. Hayasaka,H. Hayashii,M. Hazumi,T. Higuchi,L. Hinz,T. Hokuue,Y. Hoshi,S. Hou,W.-S. Hou,A. Imoto,K. Inami,Akimasa Ishikawa,Masako Iwasaki,J. H. Kang,P. Kapusta,N. Katayama,H. Kawai,T. Kawasaki,H. R. Khan,H. Kichimi,H. J. Kim,J. H. Kim,S. K. Kim,K. Kinoshita,Patrick Koppenburg,Peter Križan,Pavel Krokovny,R. Kulasiri,C. C. Kuo,A. Kuzmin,Y.-J. Kwon,J. S. Lange,S. H. Lee,Tadeusz Lesiak,J. Li,S.-W. Lin,D. Liventsev,J. Macnaughton,G. Majumder,F. Mandl,T. Matsumoto,A. Matyja,Y. Mikami,W. Mitaroff,H. Miyata,R. Mizuk,D. Mohapatra,T. Mori,T. Nagamine,Y. Nagasaka,E. Nakano,M. Nakao,H. Nakazawa,Z. Natkaniec,Shohei Nishida,O. Nitoh,S. Ogawa,T. Ohshima,T. Okabe,S. L. Olsen,W. Ostrowicz,H. Ozaki,Pavel Pakhlov,H. Palka,C. W. Park,H. Park,N. Parslow,R. Pestotnik,L. E. Piilonen,M. Rozanska,H. Sagawa,Y. Sakai,N. Sato,T. Schietinger,O. Schneider,P. Schönmeier,J. Schümann,A. J. Schwartz,S. Semenov,K. Senyo,R. Seuster,H. Shibuya,A. Somov,N. Soni,R. Stamen,S. Stanic,M. Starič,K. Sumisawa,T. Sumiyoshi,S. Y. Suzuki,O. Tajima,F. Takasaki,K. Tamai,N. Tamura,M. Tanaka,Y. Teramoto,X. C. Tian,T. Tsukamoto,S. Uehara,T. Uglov,K. Ueno,S. Uno,S. Villa,C. C. Wang,M.-Z. Wang,M. Watanabe,B. D. Yabsley,A. Yamaguchi,Y. Yamashita,M. Yamauchi,J. Ying,C. C. Zhang,L. M. Zhang,Z. P. Zhang,V. Zhilich,D. Zontar,Y. Iwasaki;A. Drutskoy;K. Abe;I. Adachi;H. Aihara;M. Akatsu;Y. Asano;T. Aushev;S. Bahinipati;A. M. Bakich;A. Bay;I. Bedny;U. Bitenc;I. Bizjak;S. Blyth;A. Bondar;A. Bozek;M. Bračko;J. Brodzicka;T. E. Browder;Pao-Ti Chang;Y. Chao;A. Chen;Kai-Feng Chen;W. T. Chen;B. G. Cheon;R. Chistov;S.-K. Choi;Y. Choi;A. Chuvikov;S. Cole;J. Dalseno;M. Danilov;M. Dash;S. Eidelman;V. Eiges;Y. Enari;F. Fang;S. Fratina;N. Gabyshev;T. Gershon;A. Go;G. Gokhroo;B. Golob;K. Hayasaka;H. Hayashii;M. Hazumi;T. Higuchi;L. Hinz;T. Hokuue;Y. Hoshi;S. Hou;W.-S. Hou;A. Imoto;K. Inami;Akimasa Ishikawa;Masako Iwasaki;J. H. Kang;P. Kapusta;N. Katayama;H. Kawai;T. Kawasaki;H. R. Khan;H. Kichimi;H. J. Kim;J. H. Kim;S. K. Kim;K. Kinoshita;Patrick Koppenburg;Peter Križan;Pavel Krokovny;R. Kulasiri;C. C. Kuo;A. Kuzmin;Y.-J. Kwon;J. S. Lange;S. H. Lee;Tadeusz Lesiak;J. Li;S.-W. Lin;D. Liventsev;J. Macnaughton;G. Majumder;F. Mandl;T. Matsumoto;A. Matyja;Y. Mikami;W. Mitaroff;H. Miyata;R. Mizuk;D. Mohapatra;T. Mori;T. Nagamine;Y. Nagasaka;E. Nakano;M. Nakao;H. Nakazawa;Z. Natkaniec;Shohei Nishida;O. Nitoh;S. Ogawa;T. Ohshima;T. Okabe;S. L. Olsen;W. Ostrowicz;H. Ozaki;Pavel Pakhlov;H. Palka;C. W. Park;H. Park;N. Parslow;R. Pestotnik;L. E. Piilonen;M. Rozanska;H. Sagawa;Y. Sakai;N. Sato;T. Schietinger;O. Schneider;P. Schönmeier;J. Schümann;A. J. Schwartz;S. Semenov;K. Senyo;R. Seuster;H. Shibuya;A. Somov;N. Soni;R. Stamen;S. Stanic;M. Starič;K. Sumisawa;T. Sumiyoshi;S. Y. Suzuki;O. Tajima;F. Takasaki;K. Tamai;N. Tamura;M. Tanaka;Y. Teramoto;X. C. Tian;T. Tsukamoto;S. Uehara;T. Uglov;K. Ueno;S. Uno;S. Villa;C. C. Wang;M.-Z. Wang;M. Watanabe;B. D. Yabsley;A. Yamaguchi;Y. Yamashita;M. Yamauchi;J. Ying;C. C. Zhang;L. M. Zhang;Z. P. Zhang;V. Zhilich;D. Zontar;Y. Iwasaki;
Journal physical review letters
Year 2005
DOI
10.1103/physrevlett.94.061802
URL
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