Observation Of D-0-(D)Over-Bar(0) Mixing In E(+) E(-) Collisions

B R Ko,E Won,I Adachi,H Aihara,K Arinstein,D M Asner,V Aulchenko,T Aushev,A Bala,V Bhardwaj,B Bhuyan,A Bobrov,A Bondar,A Bozek,M Bracko,T E Browder,D Cervenkov,A Chen,B G Cheon,K Chilikin,R Chistov,I S Cho,K Cho,V Chobanova,S K Choi,Yoojoo Choi,D Cinabro,J Dalseno,M Danilov,Z Dolezal,Z Drasal,D Dutta,K Dutta,S Eidelman,D Epifanov,H Farhat, J Fast,T Ferber,V K Gaur,S Ganguly,A Garmash,R Gillard, R Glattauer,Y M Goh,B Golob,J Haba,T Hara, H Hayashii,X H He,Toshiro Higuchi,Y Hoshi,W S Hou, H J Hyun,T Iijima, A Ishikawa,R Itoh,Y Iwasaki,Tomomi Iwashita,I Jaegle,T Julius,Tomonori Kawasaki,C Kiesling,D Y Kim, J H Kim,Min Ju Kim,Y J Kim,J Klucar,P Kodys,S Korpar,P Krizan,P Krokovny,T Kuhr,T Kumita,A Kuzmin,Y J Kwon, J S Lange,Sung Haeng Lee,J Li,Youji Li,J Libby,Chiayih Liu,Z Q Liu,P Lukin,D Matvienko,K Miyabayashi,H Miyata,G B Mohanty,A Moll,R Mussa,Y Nagasaka,E Nakano,Masashi Nakao,Z Natkaniec,M Nayak,E Nedelkovska,N K Nisar,O Nitoh,Satoshi Ogawa,S Okuno,G Pakhlova,C W Park,H K Park,T K Pedlar,Tao Peng, M Petric,L E Piilonen,M Ritter, M Roehrken, A Rostomyan,S Ryu,H Sahoo,Yuko Sakai, L Santelj,T Sanuki, V Savinov,O Schneider,G Schnell,C Schwanda,A J Schwartz,R Seidl,O Seon,M E Sevior,M Shapkin, C P Shen,T A Shibata,J G Shiu,B Shwartz,A Sibidanov,F Simon, J B Singh, Y S Sohn,A Sokolov, S Stanic, M Staric, M Steder,T Sumiyoshi,U Tamponi,G Tatishvili,Y Teramoto,K Trabelsi,M Uchida,S Uehara,T Uglov, Y Unno,S Uno, P Urquijo,Y Usov, S Vahsen,C Van Hulse,P Vanhoefer, G Varner,A Vinokurova,V Vorobyev,M N Wagner,C H Wang,M Z Wang,Pan Wang,Y Watanabe,Hidefumi Yamamoto,Y Yamashita, S Yashchenko, Y Yook,C C Zhang, Z P Zhang,V Zhilich, A Zupanc

Physical review letters(2014)

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摘要
We observe D-0-(D) over bar (0) mixing in the decay D-0 -> K+ pi(-) using a data sample of integrated luminosity 976 fb(-1) collected with the Belle detector at the KEKB e(+) e(-) asymmetric-energy collider. We measure the mixing parameters x'(2) = (0.09 +/- 0.22) x 10(-3) and y' = (4.6 +/- 3.4) x 10(-3) and the ratio of doubly Cabibbo-suppressed to Cabibbo-favored decay rates R-D = (3.53 +/- 0.13) x 10(-3) where the uncertainties are statistical and systematic combined. Our measurement excludes the no-mixing hypothesis at the 5.1 standard deviation level.
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