Study of B → πlν and B → ρlν decays and determination of |V_(ub)|
Abstract
We present an analysis of exclusive charmless semileptonic B-meson decays based on 377 × 10^6 BB̅ pairs recorded with the BABAR detector at the Υ(4S) resonance. We select four event samples corresponding to the decay modes B^0 → π^-ℓ^+ν, B^+ → π^0ℓ^+ν, B^0 → ρ^-ℓ^+ν, and B^+ → ρ^0ℓ^+ν and find the measured branching fractions to be consistent with isospin symmetry. Assuming isospin symmetry, we combine the two B → πℓν samples, and similarly the two B → ρℓν samples, and measure the branching fractions B(B^0→π^-ℓ^+ν)=(1.41 ± 0.05 ± 0.07) × 10^(-4) and B(B^0 → ρ^-ℓ^+ν)=(1.75 ± 0.15 ± 0.27) × 10^(-4), where the errors are statistical and systematic. We compare the measured distribution in q^2, the momentum transfer squared, with predictions for the form factors from QCD calculations and determine the Cabibbo-Kobayashi-Maskawa matrix element |V_(ub)|. Based on the measured partial branching fraction for B → πℓν in the range q^2 < 12 GeV^2 and the most recent QCD light-cone sum-rule calculations, we obtain |V_(ub)|=(3.78 ± 0.13^(+0.55)_(-0.40)) × 10^(-3), where the errors refer to the experimental and theoretical uncertainties. From a simultaneous fit to the data over the full q^2 range and the FNAL/MILC lattice QCD results, we obtain |V_(ub)|=(2.95 ± 0.31) × 10^(-3) from B → πℓν, where the error is the combined experimental and theoretical uncertainty.
Additional Information
© 2011 American Physical Society. Received 18 May 2010; published 7 February 2011. We would like to thank A. Khodjamirian, A. Kronfeld, P. Mackenzie, T. Mannel, J. Shigemitsu, and R. Van de Water for their help with theoretical form-factor calculations. We are grateful for the extraordinary contributions of our PEP-II colleagues in achieving the excellent luminosity and machine conditions that have made this work possible. The success of this project also relies critically on the expertise and dedication of the computing organizations that support BABAR. The collaborating institutions wish to thank SLAC for its support and the kind hospitality extended to them. This work is supported by the US Department of Energy and National Science Foundation, the Natural Sciences and Engineering Research Council (Canada), the Commissariat à l'Energie Atomique and Institut National de Physique Nucléaire et de Physique des Particules (France), the Bundesministerium für Bildung und Forschung and Deutsche Forschungsgemeinschaft (Germany), the Istituto Nazionale di Fisica Nucleare (Italy), the Foundation for Fundamental Research on Matter (The Netherlands), the Research Council of Norway, the Ministry of Education and Science of the Russian Federation, Ministerio de Ciencia e Innovación (Spain), and the Science and Technology Facilities Council (United Kingdom). Individuals have received support from the Marie-Curie IEF program (European Union), the A. P. Sloan Foundation (USA), and the Binational Science Foundation (USA-Israel).Attached Files
Published - Sanchez2011p13157Phys_Rev_D.pdf
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Additional details
- Eprint ID
- 23106
- Resolver ID
- CaltechAUTHORS:20110325-091112297
- Stanford Linear Accelerator Center (SLAC)
- Department of Energy (DOE)
- NSF
- Commissariat à l'Energie Atomique (CEA)/Institut National de Physique Nucleaire et de Physique des Particules (CNRS) (France)
- Bundesministerium fur Bildung und Forschung (BMBF) (Germany)
- Istituto Nazionale di Fisica Nucleare (INFN) (Italy)
- Foundation for Fundamental Research on Matter (FOM) (The Netherlands)
- Research Council of Norway
- Ministry of Education and Science of the Russian Federation (MES) (Russia)
- Ministerio de Ciencia e Innovación (MCINN) (Spain)
- Science and Technology Facilities Council (STFC) (UK)
- European Union (EU)
- A. P. Sloan Foundation
- Binational Science Foundation (USA-Israel)
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2011-03-28Created from EPrint's datestamp field
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2021-11-09Created from EPrint's last_modified field