Abstract:It is pointed out that decays of the type B → DD have no factorizable contributions, unless at least one of the charmed mesons in the final state is a vector meson. The dominant contributions to the decay amplitudes arise from chiral loop contributions and tree level amplitudes generated by soft gluon emissions forming a gluon condensate. We predict that the branching ratios for the processesB 0 → s are all of order (3 − 4) × 10 −4 , whileB 0 → D + * s D − * s has a branching ratio 5 to 10 times bigger. We emp… Show more
“…[34] (albeit the real part of the ratio has the opposite sign), but smaller than the result in Ref. [50]. On the other hand the measured values for the branching ratios of the annihilation-dominated modes seem consistently larger than the estimates in Ref.…”
Section: E Branching Ratios and Su(3) Breakingcontrasting
An extensive model-independent analysis of B → DD decays is carried out employing SU(3) flavour symmetry, including symmetry-breaking corrections. Several theoretically clean observables are identified which allow for testing the Standard Model. These include the known time-dependent CP asymmetries, the penguin pollution of which can be controlled in this framework, but notably also quasi-isospin relations which are experimentally well accessible and unaffected by symmetrybreaking corrections. Theoretical assumptions can be kept to a minimum and controlled by additional sum rules. Available data are used in global fits to predict the branching ratio for thes decay as well as several CP asymmetries which have not been measured so far, and future prospects are analyzed.
“…[34] (albeit the real part of the ratio has the opposite sign), but smaller than the result in Ref. [50]. On the other hand the measured values for the branching ratios of the annihilation-dominated modes seem consistently larger than the estimates in Ref.…”
Section: E Branching Ratios and Su(3) Breakingcontrasting
An extensive model-independent analysis of B → DD decays is carried out employing SU(3) flavour symmetry, including symmetry-breaking corrections. Several theoretically clean observables are identified which allow for testing the Standard Model. These include the known time-dependent CP asymmetries, the penguin pollution of which can be controlled in this framework, but notably also quasi-isospin relations which are experimentally well accessible and unaffected by symmetrybreaking corrections. Theoretical assumptions can be kept to a minimum and controlled by additional sum rules. Available data are used in global fits to predict the branching ratio for thes decay as well as several CP asymmetries which have not been measured so far, and future prospects are analyzed.
“…Using B(B 0 → D − s π + ) from [2] we obtain This value represents the first existing limit on this decay mode and reaches the sensitivity to test the prediction of [3].…”
“…These counterterms are not considered here (or in [3,4]) and has to be be considered together with the constant (non-logarithmic) chiral loop terms which we also have dropped in this analysis. The inclusion of counterterms and constant chiral loops terms will be discussed elsewhere.…”
Section: Heavy Light Chiral Perturbation Theorymentioning
confidence: 99%
“…In our approach [3,4], the non-factorizable contributions are coming from chiral loops and from tree level amplitudes generated by soft gluon emision forming a gluon condensate. The gluon condensate contributions can be calculated within a recently developed Heavy Light Chiral Quark Model (HLχQM) [5].…”
Abstract.We point out that the amplitudes for the decaysIf one or two of the D-mesons in the final state are vectors (i.e D * 's) there are relatively small factorizable contributions through the annihilation mechanism. The dominant contributions to the decay amplitudes arise from chiral loop contributions and 1/N c suppressed tree level. We predict that the branching ratios for the processesBare of order (4 − 7) × 10 −3 . If both D-mesons in the final state are D * 's, we obtain branching ratios of order two times bigger.
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