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Theory of Charmless Inclusive B Decays and the Extraction of V_{ub}

Bjorn O. Lange, Matthias Neubert, Gil Paz

TL;DR

The paper develops a unified, QCD-factorized framework that smoothly interpolates between the shape-function and OPE regimes for charmless inclusive B decays, enabling a precise extraction of |V_{ub}|. By parameterizing the leading shape function and constrained subleading inputs from the B -> X_s gamma photon spectrum, it reduces dominant theoretical uncertainties and provides a robust method to predict partial rates under diverse experimental cuts. It delivers explicit leading and subleading factorized expressions for both radiative and semileptonic decays, discusses Weak Annihilation control via kinematic cuts, and presents a comprehensive error analysis with practical guidance for event-generator implementations. The approach promises 5–10% precision on |V_{ub}| as experimental data on the shape function improves, with detailed predictions across multiple cuts and thorough treatment of perturbative and hadronic uncertainties.

Abstract

We present ``state-of-the-art'' theoretical expressions for the triple differential B->X_u l^- nu decay rate and for the B->X_s gamma photon spectrum, which incorporate all known contributions and smoothly interpolate between the ``shape-function region'' of large hadronic energy and small invariant mass, and the ``OPE region'' in which all hadronic kinematical variables scale with M_B. The differential rates are given in a form which has no explicit reference to the mass of the b quark, avoiding the associated uncertainties. Dependence on m_b enters indirectly through the properties of the leading shape function, which can be determined by fitting the B->X_s gamma photon spectrum. This eliminates the dominant theoretical uncertainties from predictions for B->X_u l^- nu decay distributions, allowing for a precise determination of |V_{ub}|. In the shape-function region, short-distance and long-distance contributions are factorized at next-to-leading order in renormalization-group improved perturbation theory. Higher-order power corrections include effects from subleading shape functions where they are known. When integrated over sufficiently large portions in phase space, our results reduce to standard OPE expressions up to yet unknown O(alpha_s^2) terms. Predictions are presented for partial B->X_u l^- nu decay rates with various experimental cuts. An elaborate error analysis is performed that contains all significant theoretical uncertainties, including weak annihilation effects. We suggest that the latter can be eliminated by imposing a cut on high lepton invariant mass.

Theory of Charmless Inclusive B Decays and the Extraction of V_{ub}

TL;DR

The paper develops a unified, QCD-factorized framework that smoothly interpolates between the shape-function and OPE regimes for charmless inclusive B decays, enabling a precise extraction of |V_{ub}|. By parameterizing the leading shape function and constrained subleading inputs from the B -> X_s gamma photon spectrum, it reduces dominant theoretical uncertainties and provides a robust method to predict partial rates under diverse experimental cuts. It delivers explicit leading and subleading factorized expressions for both radiative and semileptonic decays, discusses Weak Annihilation control via kinematic cuts, and presents a comprehensive error analysis with practical guidance for event-generator implementations. The approach promises 5–10% precision on |V_{ub}| as experimental data on the shape function improves, with detailed predictions across multiple cuts and thorough treatment of perturbative and hadronic uncertainties.

Abstract

We present ``state-of-the-art'' theoretical expressions for the triple differential B->X_u l^- nu decay rate and for the B->X_s gamma photon spectrum, which incorporate all known contributions and smoothly interpolate between the ``shape-function region'' of large hadronic energy and small invariant mass, and the ``OPE region'' in which all hadronic kinematical variables scale with M_B. The differential rates are given in a form which has no explicit reference to the mass of the b quark, avoiding the associated uncertainties. Dependence on m_b enters indirectly through the properties of the leading shape function, which can be determined by fitting the B->X_s gamma photon spectrum. This eliminates the dominant theoretical uncertainties from predictions for B->X_u l^- nu decay distributions, allowing for a precise determination of |V_{ub}|. In the shape-function region, short-distance and long-distance contributions are factorized at next-to-leading order in renormalization-group improved perturbation theory. Higher-order power corrections include effects from subleading shape functions where they are known. When integrated over sufficiently large portions in phase space, our results reduce to standard OPE expressions up to yet unknown O(alpha_s^2) terms. Predictions are presented for partial B->X_u l^- nu decay rates with various experimental cuts. An elaborate error analysis is performed that contains all significant theoretical uncertainties, including weak annihilation effects. We suggest that the latter can be eliminated by imposing a cut on high lepton invariant mass.

Paper Structure

This paper contains 29 sections, 84 equations, 4 figures, 7 tables.

Figures (4)

  • Figure 1: The hadronic phase space in $P_+$ and $P_-$. The light gray region contains background from $\bar{B}\to X_c\,l^-\bar{\nu}$ decays, while the dark gray region is only populated by $\bar{B}\to X_u\,l^-\bar{\nu}$ events. The line separating the two regions is the contour where $M_X^2=P_+ P_-=M_D^2$. Each point represents a $\bar{B}\to X_u\,l^-\bar{\nu}$ event in a Monte-Carlo simulation using the results of this paper. While the shape-function region of large $P_-$ and small $P_+$ is highly populated, there is not a single event with $P_+$ larger than 3 GeV out of the 1300 events generated.
  • Figure 2: Left: Different functional forms for the leading shape function. We show $F^{\rm (exp)}(\hat{\omega},\Lambda,2)$ (solid), $F^{\rm (gauss)}(\hat{\omega},\Lambda,2)$ (dotted), and $F^{\rm (hyp)}(\hat{\omega},\Lambda,2)$ (dash-dotted) as functions of the ratio $\hat{\omega}/\Lambda$. Right: The same functions with the parameters $\Lambda$ and $b$ tuned such that $m_b(\mu_*,\mu_*)=4.61$ GeV and $\mu_\pi^2(\mu_*,\mu_*) = 0.2$ GeV$^2$. See text for explanation.
  • Figure 3: Nine models for the subleading shape function $\hat{u}(\hat{\omega})$ obtained by adding or subtracting one of the four functions $h_n(\hat{\omega})$ to the default model in (\ref{['SSF:model1']}), shown as a thick line. See text for explanation.
  • Figure 4: Left: Theoretical prediction for the double differential decay rate. The light area represents a large decay rate. Black regions denote areas where the decay rate is close to zero. The dotted line is given by $P_+ P_- = M_D^2$, which means that charm background is located in the upper wedge. See text for further explanation. Right: The $P_+$ spectrum extended to large values of $P_+$. The thin solid line denotes the leading-power prediction, the dashed line depicts first-order power corrections, the dash-dotted line shows second-order power corrections, and the thick solid line is their sum.