Abstract
Abstract
We have extracted the ratio |Vub|/|Vcb| from a combined study of the available inputs on $$ \overline{B}\to \left(\pi, \rho, \omega \right){\ell}^{-}{\overline{\nu}}_{\ell } $$
B
¯
→
π
ρ
ω
ℓ
−
ν
¯
ℓ
and $$ \overline{B}\left({\overline{B}}_s\right)\to \left({D}^{\left(\ast \right)},{D}_s^{\left(\ast \right)}\right){\ell}^{-}{\overline{\nu}}_{\ell }\ \left(\ell =\mu\ \textrm{or}\ e\right) $$
B
¯
B
¯
s
→
D
∗
D
s
∗
ℓ
−
ν
¯
ℓ
ℓ
=
μ
or
e
decays. We have done our analysis with and without the inclusion of the available experimental results on the branching fraction $$ \mathcal{BR}\left({\overline{B}}_s\to {K}^{+}{\mu}^{-}{\overline{\nu}}_{\mu}\right) $$
BR
B
¯
s
→
K
+
μ
−
ν
¯
μ
or the ratio of the rates $$ \Gamma \left({\overline{B}}_s\to {K}^{+}{\ell}^{-}{\overline{\nu}}_{\ell}\right)/\Gamma \left({\overline{B}}_s\to {D}_s^{+}{\ell}^{-}{\overline{\nu}}_{\ell}\right) $$
Γ
B
¯
s
→
K
+
ℓ
−
ν
¯
ℓ
/
Γ
B
¯
s
→
D
s
+
ℓ
−
ν
¯
ℓ
. We have used all the available experimental data on the branching fractions in different q2-bins, the available theory inputs on the form factors from lattice and the light cone sum rule (LCSR) approach; analysed the data in different possible scenarios and presented the results. From a combined analysis of all the b → cℓ−νℓ exclusive decays, we have obtained |Vcb| = (40.5 ± 0.6) × 10−3 and from all the b → uℓ−νℓ modes, we obtain |Vub| = (3.46 ± 0.12) × 10−3 which changes to |Vub| = (3.51 ± 0.13) × 10−3 after dropping $$ \mathcal{BR}\left({\overline{B}}_s\to {K}^{+}{\mu}^{-}{\overline{\nu}}_{\mu}\right) $$
BR
B
¯
s
→
K
+
μ
−
ν
¯
μ
. We hence report the values of the ratio |Vub|/|Vcb| = 0.085 ± 0.003 and 0.087 ± 0.003 with and without the input from $$ {\overline{B}}_s\to {K}^{+}{\mu}^{-}{\overline{\nu}}_{\mu } $$
B
¯
s
→
K
+
μ
−
ν
¯
μ
modes, respectively. We have also predicted the ratio $$ \Gamma \left({\overline{B}}_s\to {K}^{+}{\ell}^{-}{\overline{\nu}}_{\ell}\right)/\Gamma \left({\overline{B}}_s\to {D}_s^{+}{\ell}^{-}{\overline{\nu}}_{\ell}\right) $$
Γ
B
¯
s
→
K
+
ℓ
−
ν
¯
ℓ
/
Γ
B
¯
s
→
D
s
+
ℓ
−
ν
¯
ℓ
using the fit results. In addition, we provide the predictions of $$ \mathcal{BR}\left({\overline{B}}_s\to {K}^{+}{\mu}^{-}{\overline{\nu}}_{\mu}\right) $$
BR
B
¯
s
→
K
+
μ
−
ν
¯
μ
and $$ \mathcal{BR}\left(\overline{B}\to \left(\rho, \omega \right){\ell}^{-}{\overline{\nu}}_{\ell}\right) $$
BR
B
¯
→
ρ
ω
ℓ
−
ν
¯
ℓ
in the Standard Model (SM) in small q2-bins.
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
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