330 K
12 pp.
 
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TitleReport of the Working Group on CP Violation and Rare Decays
Author(s)Cronin, J. W.; Deshpande, N. G.; Kane, G. L.; Luth, V. C.; Odian, A. C.; Machacek, M. E.; Paige, F.; Schmidt, M. P.; Slaughter, J.; Trilling, G. H.
Publication DateOctober 1984
Report NumberLBL-18402
Unique IdentifierACC0351
Other NumbersCONF-8406198-23; Legacy ID: DE85003470; OSTI ID: 6124405
Research OrgDepartment of Physics, University of Chicago, Chicago, IL (USA); Department of Physics, University of Oregon, Eugene, OR (USA); Department of Physics, University of Michigan, Ann Arbor, MI (USA); Stanford Linear Accelerator Center (SLAC), CA (USA); Department of Physics, Northeastern University, Boston, MA (USA); Brookhaven National Laboratory (BNL), Upton, NY (USA)
Contract NoAC03-76SF00098
Sponsoring OrgOffice of Energy Research (ER), U.S. Department of Energy (DOE)
Other InformationDesign and Utilization of the Superconducting Super Collider Summer Study, Snowmass, CO, USA, 23 June - 13 July 1984
Subject72 Physics of Elementary Particles and Fields; B Mesons; Particle Decay; CP Invariance; Final-state Interactions; Bosons; Decay; Elementary Particles; Hadrons; Interactions; Invariance Principles; Mesons
Related Web PagesJames Cronin, CP Violation, and the Pierre Auger Observatory
AbstractIt has been pointed out that, with its high energy and luminosity, the SSC may provide the best or only way in which CP violation in heavy meson decays or the rare decay modes of such mesons can be observed. The major problem in the exploitation of the high rates of heavy quark production is the identification of interesting decays in the midst of a large background of more conventional processes. There have been some optimistic reports on the feasibility of such experiments, but relatively little quantitative backup has been provided. In the present report, we concentrate exclusively on B-meson decays. As is the case for K mesons, but not for charm or top decays, the favored modes are suppressed by the smallness of Cabibbo-Kobayashi-Maskawa angles, and therefore rare modes are relatively more frequent and potentially easier to observe.
330 K
12 pp.
 
View Document 
  


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