Abstract:The amplitudes for decays of the typehave relatively small factorizable contributions through the annihilation mechanism. The dominant contributions to the decay amplitudes arise from chiral loop contributions and tree level amplitudes which can be obtained in terms of soft gluon emissions forming a gluon condensate. We predict that the branching ratios for the processesB. We obtain branching ratios for two D * 's in the final state of order two times bigger.
“…As the slope of the IW function is steeper than the one used in, say, Ref. [18], the partial amplitudes for B → DD depending on the IW function, might be overestimated there. This will then have consequences for the size of the overall amplitude.…”
Section: Resultsmentioning
confidence: 81%
“…Some versions of quark models [3,4,7] gave a slope ξ ′ (1) ≃ −0.4 to −0.3, which is not in agreement with general theoretical expectations expressed in Bjorken [12] and Uraltsev [13] sum rules which together imply −ξ ′ (1) ≥ 3/4. Also, a combined fit [14] to results of experimental measurements of B → D * lν decays gives −ξ ′ (1) = 1.16 ± 0.05, and, although dispersion of experimental results is large leading to a small confidence level of this fit (≈ 1%), it seems reasonable to assume that absolute value of the slope cannot be significantly smaller than 1. In this paper we propose a modified version of the model in [7], which has a particular feature of explicit inclusion of the gluon condensate effects, enabling consistent estimation of non-factorizable amplitudes [15,16,17,18,19], and we demonstrate that this model gives a satisfactory description of the IW function slope.…”
We consider the Isgur-Wise function ξ(ω) within a new modified version of a heavy-light chiral quark model. While early versions of such models gave too small absolute value of the slope, namely ξ ′ (1) ≃ −0.4 to −0.3, we show how extended version(s) may lead to values around −1, in better agreement with recent measurements. This is obtained by introducing a new mass parameter in the heavy quark propagator.We also shortly comment on the consequences for the decay modes B → DD.
“…As the slope of the IW function is steeper than the one used in, say, Ref. [18], the partial amplitudes for B → DD depending on the IW function, might be overestimated there. This will then have consequences for the size of the overall amplitude.…”
Section: Resultsmentioning
confidence: 81%
“…Some versions of quark models [3,4,7] gave a slope ξ ′ (1) ≃ −0.4 to −0.3, which is not in agreement with general theoretical expectations expressed in Bjorken [12] and Uraltsev [13] sum rules which together imply −ξ ′ (1) ≥ 3/4. Also, a combined fit [14] to results of experimental measurements of B → D * lν decays gives −ξ ′ (1) = 1.16 ± 0.05, and, although dispersion of experimental results is large leading to a small confidence level of this fit (≈ 1%), it seems reasonable to assume that absolute value of the slope cannot be significantly smaller than 1. In this paper we propose a modified version of the model in [7], which has a particular feature of explicit inclusion of the gluon condensate effects, enabling consistent estimation of non-factorizable amplitudes [15,16,17,18,19], and we demonstrate that this model gives a satisfactory description of the IW function slope.…”
We consider the Isgur-Wise function ξ(ω) within a new modified version of a heavy-light chiral quark model. While early versions of such models gave too small absolute value of the slope, namely ξ ′ (1) ≃ −0.4 to −0.3, we show how extended version(s) may lead to values around −1, in better agreement with recent measurements. This is obtained by introducing a new mass parameter in the heavy quark propagator.We also shortly comment on the consequences for the decay modes B → DD.
“…The LEET form factors ζ and ζ ⊥ , together with data for the D → π and D → ρ transitions, will determine the coupling constants G A and G V , which may be used in the calculation of nonfactorizable (color suppressed) nonleptonic D-meson decays, in the same manner as has previously been done for K → ππ [39,51], D → K 0K0 [52], B → DD [53,54], B → Dπ [40], and B → π 0 π 0 [41]. Then nonleptonic decay amplitudes can be written in terms of the LEET form factors ζ i , both for the factorized and the color-suppressed cases.…”
We study transition form factors for decays of D mesons. That is, we consider matrix elements of the weak left-handed quark current for the transitions D → P and D → V, where P and, V are light pseudoscalar or vector mesons, respectively. Our motivation to perform the present study of these form factors is future calculations of nonleptonic decay amplitudes. We consider the transition form factors within a class of chiral quark models. Especially, we study how the large energy effective theory limit works for D-meson decays. In this paper, we extend previous work on the case B → π to the case D → P ¼ π, K. Further, we extend our previous model based on the large energy effective theory to the entirely new case D → V ¼ ρ; K Ã ; … To determine some of the parameters in our model, we use existing data and results based on some other methods like lattice calculations, light-cone sum rules, and heavy-light chiral perturbation theory. We also obtain some new predictions for relations between form factors.
“…The LEET form factors ζ and ζ ⊥ , together with data for the D → π and D → ρ transitions, will determine the coupling constants G A and G V , which may be used in the calculation of nonfactorizable (color suppressed) nonleptonic D-meson decays, in the same manner as has previously been done for K → ππ [39,51], D → K 0K0 [52], B → DD [53,54], B → Dπ [40], and B → π 0 π 0 [41]. Then nonleptonic decay amplitudes can be written in terms of the LEET form factors ζ i , both for the factorized and the color-suppressed cases.…”
I would like to thank my advisor Jan Olav Eeg for his guidance, patience and motivation during these years. I also thank the professors Farid Ould-Saada, Carsten Lutken and Are Raklev who were my teachers. Thanks also to my office mate Sergey and my fellow students Marianne, Marius and the members of the theory group for their support both technical and social. I would also like to thank my PhD committee. My children Thomas and Andreas and my husband Roar were patient with my late working hours, weekend work, and with some truncated vacations. Roar also helped with proof reading, providing useful writing advice, and did the usual house and family work when I was occupied with equations and calculations. I would also like to thank Bjørg and Asgeir who supported the project fully as well, which was also very important to me.
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