Rare and forbidden decay of charm mesons at CLEO-c and BES-III.pdf

Rare and forbidden decay of charm mesons at CLEO-c and BES-III.pdf

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Rare and forbidden decay of charm mesons at CLEO-c and BES-III

a r X i v : 0 7 0 7 .2 4 1 3 v 2 [ h e p - e x ] 2 0 J u l 2 0 0 7 Rare and forbidden decay of charm mesons at CLEO-c and BES-III Hai-Bo Li ?? Author Institute of High Energy Physics, P.O.Box 918, Beijing 100049, China E-mail: lihb@ This paper presents the results of searches for the flavor-changing neutral current, lepton-number- violating and lepton-flavor-violating processes in the charm mesons decays. Recent results from charged D mesons decays to final states with dielectrons from CLEO-c are reported. The prospects of the searches for the rare charm decays at BES-III are also discussed. KAON International Conference May 21-25 2007 Laboratori Nazionali di Frascati dell’INFN, Rome, Italy ? Speaker. ? For BES-III and CLEO-c Collaborations. c? Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Rare and forbidden decay of charm mesons at CLEO-c and BES-III Hai-Bo Li 1. Introduction Searches for rare-decay processes have played an important role in the development of the Standard Model (SM). The absence of flavor-changing neutral current (FCNC) in K decays im- plied the existence of charm quark, and the observations of B 0 ?B0 and Bs ?Bs mixings (FCNC processes) signaled the very large top-quark mass. The study of the FCNC has been focused on rare decays involving transitions such as s → dl+ l?, s → dν ν, b → sγ , and b → l+ l?. In contrast with the K and B FCNC processes, the D meson FCNC transitions are mediated by light down-quark sector, which implies an efficient Glashow-Iliopoulos-Maiani (IM) cancella- tion. In this case, D 0 mixing, as well as FCNC decays are expected to be very small in the SM short-distance contributions. Many extensions of the SM may enhance the mixing rate and FCNC processes in the short-distance of the D system by orders of magnitudes. Unfortunately, the new physics contributions are diluted by large long-distance contributions which are likel

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