B→ρB\to ρ semileptonic decays and ∣Vub∣|V_{ub}|

preprint2014arXivOpen access

Abstract

We reevaluate the B→ρ l+νlB\toρ\,l^+ν_l decay width as a full B→ππ l+νlB\toππ\,l^+ν_l four-particle decay, in which the two final pions are produced via an intermediate ρρ meson. The decay width can be written as a convolution of the B→ρ l+νlB\toρ\,l^+ν_l decay width, for an off-shell ρρ, with the ρ→ππρ\toππ line shape. This allows to fully incorporate the effects of the finite ρρ meson width. As shown, consideration of the ρρ meson width effects increase the ∣Vub∣|V_{ub}| value by some 8%, rendering it in better agreement with the determination based in the B→πB\toπ decay. We take the q2q^2 dependence of the B→ρB\to ρ semileptonic form factors from a dispersive Omnès representation. The Omnès subtraction constants and the overall normalization parameter ∣Vub∣|V_{ub}| are fitted to light cone sum rules and lattice QCD theoretical form-factor calculations, in the low and high q2q^2 regions respectively, together to the CLEO, BaBar and Belle experimental partial branching fraction distributions. The extracted value from this global fit is ∣Vub∣=(3.12±0.13)×10−3|V_{ub}|=(3.12\pm 0.13)\times 10^{-3}, in agreement with the average B→πB\to π exclusive value ∣Vub∣=(3.23±0.31)×10−3|V_{ub}|=(3.23\pm 0.31)\times 10^{-3} quoted by the Particle Data Group. The extracted value increases to ∣Vub∣=(3.51±0.16)×10−3|V_{ub}|=(3.51\pm 0.16)\times 10^{-3} if only the most recent Belle Collaboration data is used. This latter value is in agreement with different theoretical determinations based in the B→πB\toπ semileptonic decay and the values obtained by the CKMfitter and UTfit groups. In any case a clear tension with the ∣Vub∣|V_{ub}| value extracted from inclusive semileptonic b→ub\to u decays still persists.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.