Search for the rare decay D0→γγD^0\toγγ at Belle

preprint2015arXivOpen access
Belle CollaborationN. K. NisarG. B. MohantyK. TrabelsiT. AzizA. AbdesselamI. AdachiH. AiharaD. M. AsnerV. AulchenkoT. AushevR. AyadV. BabuI. BadhreesS. BahinipatiE. BarberioP. BeheraV. BhardwajJ. BiswalA. BobrovA. BozekM. BračkoF. BreibeckT. E. BrowderD. ČervenkovV. ChekelianA. ChenB. G. CheonR. ChistovK. ChoV. ChobanovaY. ChoiD. CinabroJ. DalsenoN. DashZ. DoležalZ. DrásalA. DrutskoyD. DuttaS. EidelmanH. FarhatJ. E. FastB. G. FulsomV. GaurA. GarmashR. GillardY. M. GohP. GoldenzweigD. GreenwaldO. GrzymkowskaJ. HabaT. HaraK. HayasakaH. HayashiiX. H. HeW. -S. HouK. InamiA. IshikawaY. IwasakiW. W. JacobsI. JaegleH. B. JeonD. JoffeK. K. JooT. JuliusK. H. KangE. KatoT. KawasakiC. KieslingD. Y. KimH. J. KimK. T. KimM. J. KimS. H. KimK. KinoshitaP. KodyšS. KorparP. KrižanP. KrokovnyT. KuhrR. KumarT. KumitaA. KuzminY. -J. KwonI. S. LeeJ. S. LangeH. LiL. LiL. Li GioiJ. LibbyD. LiventsevP. LukinM. MasudaD. MatvienkoK. MiyabayashiH. MiyataR. MizukS. MohantyA. MollH. K. MoonT. MoriR. MussaE. NakanoM. NakaoT. NanutZ. NatkaniecM. NayakM. NiiyamaS. NishidaS. OgawaS. OkunoP. PakhlovG. PakhlovaB. PalC. W. ParkH. ParkS. PaulT. K. PedlarL. PesántezR. PestotnikM. PetričL. E. PiilonenK. PrasanthC. PulvermacherJ. RauchE. RibežlM. RitterA. RostomyanS. RyuH. SahooS. SandilyaT. SanukiY. SatoV. SavinovT. SchlüterO. SchneiderG. SchnellC. SchwandaA. J. SchwartzY. SeinoK. SenyoO. SeonI. S. SeongV. ShebalinT. -A. ShibataJ. -G. ShiuB. ShwartzF. SimonJ. B. SinghY. -S. SohnE. SolovievaS. StaničM. StaričJ. StypulaM. SumihamaT. SumiyoshiU. TamponiY. TeramotoM. UchidaT. UglovS. UnoP. UrquijoC. Van HulseP. VanhoeferG. VarnerK. E. VarvellA. VinokurovaA. VossenM. N. WagnerC. H. WangM. -Z. WangX. L. WangM. WatanabeY. WatanabeK. M. WilliamsE. WonJ. YeltonC. Z. YuanY. YusaZ. P. ZhangV. ZhilichV. ZhulanovA. Zupanc

Abstract

We search for the rare radiative decay D0→γγD^0\toγγ using a data sample with an integrated luminosity of 832fb−1832{\rm fb^{-1}} recorded by the Belle detector at the KEKB e+e−e^+e^- asymmetric-energy collider. We find no statistically significant signal and set an upper limit on the branching fraction of B(D0→γγ)<8.5×10−7{\cal B}(D^0\toγγ)<8.5\times10^{-7} at 90%90\% confidence level. This is the most restrictive limit on the decay channel to date.

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