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Title: Color suppressed contribution to B{sub d}{sup 0}{yields}{pi}0{pi}{sup 0}

Journal Article · · Physical Review. D, Particles Fields
;  [1]
  1. Department of Physics, University of Oslo, P.O.Box 1048 Blindern, N-0316 Oslo (Norway)

The decay modes of the type B{yields}{pi}{pi} are dynamically different. For the case B{sub d}{sup 0}{yields}{pi}{sup +}{pi}{sup -} there is a substantial factorized contribution which dominates. In contrast, the decay mode B{sub d}{sup 0}{yields}{pi}{sup 0}{pi}{sup 0} has a small factorized contribution, being proportional to a small Wilson coefficient combination. However, for the decay mode B{sub d}{sup 0}{yields}{pi}{sup 0}{pi}{sup 0} there is a sizeable nonfactorizable (color suppressed) contribution due to soft (long distance) interactions, which dominate the amplitude. We estimate the branching ratio for the mode B{sub d}{sup 0}{yields}{pi}{sup 0}{pi}{sup 0} in the heavy quark limit for the b quark. In order to estimate color suppressed contributions we treat the energetic light (u, d, s) quark within a variant of Large Energy Effective Theory combined with a recent extension of chiral quark models in terms of model- dependent gluon condensates. We find that our calculated color suppressed amplitude is suppressed by a factor of order {Lambda}{sub QCD}/m{sub b} with respect to the factorizable amplitude, as it should according to QCD-factorization. Further, for reasonable values of the constituent quark mass and the gluon condensate, the calculated nonfactorizable amplitude for B{sub d}{sup 0}{yields}{pi}{sup 0}{pi}{sup 0} can easily accommodate the experimental value. Unfortunately, the color suppressed amplitude is very sensitive to the values of these model-dependent parameters. Therefore fine-tuning is necessary in order to obtain an amplitude compatible with the experimental result for B{sub d}{sup 0}{yields}{pi}{sup 0}{pi}{sup 0}. A possible link to the triangle anomaly is discussed.

OSTI ID:
21578192
Journal Information:
Physical Review. D, Particles Fields, Vol. 83, Issue 5; Other Information: DOI: 10.1103/PhysRevD.83.054016; (c) 2011 American Institute of Physics; ISSN 0556-2821
Country of Publication:
United States
Language:
English