Observation of D0−Dˉ0D^0-\bar{D}^0 Mixing in e+e−e^+e^- Collisions

preprint2014arXivOpen access
B. R. KoE. WonI. AdachiH. AiharaK. ArinsteinD. M. AsnerV. AulchenkoT. AushevA. BalaV. BhardwajB. BhuyanA. BobrovA. BondarA. BozekM. BračkoT. E. BrowderD. ČervenkovA. ChenB. G. CheonK. ChilikinR. ChistovI. -S. ChoK. ChoV. ChobanovaS. -K. ChoiY. ChoiD. CinabroJ. DalsenoM. DanilovZ. DoležalZ. DrásalD. DuttaK. DuttaS. EidelmanD. EpifanovH. FarhatJ. E. FastT. FerberV. GaurS. GangulyA. GarmashR. GillardR. GlattauerY. M. GohB. GolobJ. HabaT. HaraH. HayashiiX. H. HeT. HiguchiY. HoshiW. -S. HouH. J. HyunT. IijimaA. IshikawaR. ItohY. IwasakiT. IwashitaI. JaegleT. JuliusT. KawasakiC. KieslingD. Y. KimJ. B. KimJ. H. KimM. J. KimY. J. KimJ. KlucarP. KodyšS. KorparP. KrižanP. KrokovnyT. KuhrT. KumitaA. KuzminY. -J. KwonJ. S. LangeS. -H. LeeJ. LiY. LiJ. LibbyC. LiuZ. Q. LiuP. LukinD. MatvienkoK. MiyabayashiH. MiyataG. B. MohantyA. MollR. MussaY. NagasakaE. NakanoM. NakaoZ. NatkaniecM. NayakE. NedelkovskaN. K. NisarO. NitohS. OgawaS. OkunoG. PakhlovaC. W. ParkH. K. ParkT. K. PedlarT. PengM. PetričL. E. PiilonenM. RitterM. RöhrkenA. RostomyanS. RyuH. SahooY. SakaiL. SanteljT. SanukiV. SavinovO. SchneiderG. SchnellC. SchwandaA. J. SchwartzR. SeidlO. SeonM. E. SeviorM. ShapkinC. P. ShenT. -A. ShibataJ. -G. ShiuB. ShwartzA. SibidanovF. SimonJ. B. SinghY. -S. SohnA. SokolovS. StaničM. StaričM. StederT. SumiyoshiU. TamponiG. TatishviliY. TeramotoK. TrabelsiM. UchidaS. UeharaT. UglovY. UnnoS. UnoP. UrquijoY. UsovS. E. VahsenC. Van HulseP. VanhoeferG. VarnerA. VinokurovaV. VorobyevM. N. WagnerC. H. WangM. -Z. WangP. WangY. WatanabeH. YamamotoY. YamashitaS. YashchenkoY. YookC. C. ZhangZ. P. ZhangV. ZhilichA. Zupanc

Abstract

We observe D0−Dˉ0D^0-\bar{D}^0 mixing in the decay D0→K+π−D^0\rightarrow K^+π^- using a data sample of integrated luminosity 976 fb−1^{-1} collected with the Belle detector at the KEKB e+e−e^+e^- asymmetric-energy collider. We measure the mixing parameters x′2=(0.09±0.22)×10−3{x'}^2 = (0.09\pm0.22)\times 10^{-3} and y′=(4.6±3.4)×10−3y' = (4.6\pm3.4)\times 10^{-3} and the ratio of doubly Cabibbo-suppressed to Cabibbo-favored decay rates RD=(3.53±0.13)×10−3R_D = (3.53\pm0.13)\times 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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