Estimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$

The interference between Cabibbo-favoured and Cabibbo-suppressed $B\to D\pi$ decay amplitudes provides sensitivity to the CKM angle $\gamma$. The relative size of the interfering amplitudes is an important ingredient in the determination of $\gamma$. Using branching fractions from various $B\to Dh$...

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Detalles Bibliográficos
Autores principales: Kenzie, Matthew, Martinelli, Maurizio, Tuning, Niels
Lenguaje:eng
Publicado: 2016
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.94.054021
http://cds.cern.ch/record/2195565
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author Kenzie, Matthew
Martinelli, Maurizio
Tuning, Niels
author_facet Kenzie, Matthew
Martinelli, Maurizio
Tuning, Niels
author_sort Kenzie, Matthew
collection CERN
description The interference between Cabibbo-favoured and Cabibbo-suppressed $B\to D\pi$ decay amplitudes provides sensitivity to the CKM angle $\gamma$. The relative size of the interfering amplitudes is an important ingredient in the determination of $\gamma$. Using branching fractions from various $B\to Dh$ decays, and the measured value for $r_{B}^{DK}$, the magnitude of the amplitude ratio of $B^+\to D^0\pi^+$ and $B^+\to \bar{D}^0\pi^+$ decays is estimated to be $r_{B}^{D\pi} = 0.0053 \pm 0.0007$.
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spelling cern-21955652023-03-14T17:26:24Zdoi:10.1103/PhysRevD.94.054021http://cds.cern.ch/record/2195565engKenzie, MatthewMartinelli, MaurizioTuning, NielsEstimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$Particle Physics - PhenomenologyThe interference between Cabibbo-favoured and Cabibbo-suppressed $B\to D\pi$ decay amplitudes provides sensitivity to the CKM angle $\gamma$. The relative size of the interfering amplitudes is an important ingredient in the determination of $\gamma$. Using branching fractions from various $B\to Dh$ decays, and the measured value for $r_{B}^{DK}$, the magnitude of the amplitude ratio of $B^+\to D^0\pi^+$ and $B^+\to \bar{D}^0\pi^+$ decays is estimated to be $r_{B}^{D\pi} = 0.0053 \pm 0.0007$.The interference between Cabibbo-favored and Cabibbo-suppressed B→Dπ decay amplitudes provides sensitivity to the CKM angle γ. The relative size of the interfering amplitudes is an important ingredient in the determination of γ. Using branching fractions from various B→Dh decays, and the measured value for rBDK, the magnitude of the amplitude ratio of B+→D0π+ and B+→D¯0π+ decays is estimated to be rBDπ=0.0053±0.0007.The interference between Cabibbo-favoured and Cabibbo-suppressed $B\to D\pi$ decay amplitudes provides sensitivity to the CKM angle $\gamma$. The relative size of the interfering amplitudes is an important ingredient in the determination of $\gamma$. Using branching fractions from various $B\to Dh$ decays, and the measured value for $r_{B}^{DK}$, the magnitude of the amplitude ratio of $B^+\to D^0\pi^+$ and $B^+\to \bar{D}^0\pi^+$ decays is estimated to be $r_{B}^{D\pi} = 0.0053 \pm 0.0007$.arXiv:1606.09129oai:cds.cern.ch:21955652016-06-29
spellingShingle Particle Physics - Phenomenology
Kenzie, Matthew
Martinelli, Maurizio
Tuning, Niels
Estimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$
title Estimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$
title_full Estimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$
title_fullStr Estimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$
title_full_unstemmed Estimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$
title_short Estimating $r_{B}^{D\pi}$ as input to the determination of CKM angle $\gamma$
title_sort estimating $r_{b}^{d\pi}$ as input to the determination of ckm angle $\gamma$
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.94.054021
http://cds.cern.ch/record/2195565
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AT martinellimaurizio estimatingrbdpiasinputtothedeterminationofckmanglegamma
AT tuningniels estimatingrbdpiasinputtothedeterminationofckmanglegamma

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