Photon energy spectrum in B $\to$ $X_S$ + $\gamma$ and comparison with data

Autor: Ali, Ahmed, Greub, C.
Jazyk: angličtina
Rok vydání: 1995
Předmět:
perturbation theory [quantum chromodynamics]
strangeness [final state]
interpretation of experiments: CLEO
effective Hamiltonian
final state [strangeness]
mass: spectator
B: radiative decay
(photon): energy spectrum
wave function [B]
CLEO [interpretation of experiments]
momentum [quark]
decay [inclusive reaction]
nonperturbative [model]
bottom
branching ratio [B]
radiative decay: B
energy spectrum: (photon)
inclusive reaction [decay]
ddc:530
B [radiative decay]
B: wave function
B: branching ratio
quantum chromodynamics: perturbation theory
spectator: mass
numerical calculations
radiative decay [B]
energy spectrum [(photon)]
mass [spectator]
CKM matrix matrix
quark: momentum
spectator [mass]
decay: inclusive reaction
inclusive reaction: decay
strangeness: final state
model: nonperturbative
(photon) [energy spectrum]
final state: strangeness
DOI: 10.3204/pubdb-2022-07330
Popis: 16 pp. (1995).
A comparison of the inclusive photon energy spectrum in the radiative decay B → XS + γ, measured recently by the CLEO Collaboration, with the standard model is presented, using a B-meson wave function model and improving earlier perturbative QCD-based computations of the same. The dependence of the photon energy spectrum on the non-perturbative model parameters, pF, the b-quark Fermi momentum in the B hadron, and mq, the spectator quark mass, is explicitly shown, allowing a comparison of these parameters with the ones obtained from the analysis of the lepton energy spectrum in semileptonic B decays. Taking into account present uncertainties, we estimate BR(B → Xs + γ) = (2.55 ± 1.28) × 10−4 in the standard model, assuming . Comparing this with the CLEO measurement BR(B → Xs + γ) = (2.32±0.67) × 10−4 implies , in agreement with the CKM unitarity.
Databáze: OpenAIRE