2016
DOI: 10.1007/jhep08(2016)098
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B →Vℓ+ℓ− in the Standard Model from light-cone sum rules

Abstract: We present B q → ρ, B q → ω, B q → K * , B s → K * and B s → φ form factors from light-cone sum rules (LCSR) at O(α s ) for twist-2 and 3 and O(α 0 s ) for twist-4 with updated hadronic input parameters. Three asymptotic light-cone distribution amplitudes of twist-4 (and 5) are determined, necessary for the form factors to obey the equations of motion. It is argued that the latter constrain the uncertainty of tensor-to-vector form factor ratios thereby improving the prediction of zeros of helicity amplitudes o… Show more

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Cited by 524 publications
(843 citation statements)
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“…If the experimental result is reconfirmed with future measurements, flavour violating NP contributions would be the most probable explanation. Interestingly, this 2.6σ deviation can also be explained with a similar NP contribution to C 9 like the anomalies in the angular observables [15,18,[23][24][25][26][27][28]. Thus, a confirmation of the deviation in R K would also indirectly confirm the NP interpretation of the anomalies in the angular observables.…”
Section: Jhep07(2017)025mentioning
confidence: 69%
See 3 more Smart Citations
“…If the experimental result is reconfirmed with future measurements, flavour violating NP contributions would be the most probable explanation. Interestingly, this 2.6σ deviation can also be explained with a similar NP contribution to C 9 like the anomalies in the angular observables [15,18,[23][24][25][26][27][28]. Thus, a confirmation of the deviation in R K would also indirectly confirm the NP interpretation of the anomalies in the angular observables.…”
Section: Jhep07(2017)025mentioning
confidence: 69%
“…There are also slight theoretical differences, where we have employed the updated LCSR form factor calculations of ref. [27]. In addition, for the experimental results on BR(B → K * µ + µ − ) we have used the updated LHCb measurement [44] and we do not include BR(B → K * γ) which has been considered by ref.…”
Section: Fit Results For Hadronic Power Correctionsmentioning
confidence: 99%
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“…where f ρ = 0.209 GeV and A 0 (m 2 π ) A 0 (0) = 0.36 ± 0.04 [26,27]. A similar procedure can be applied to the I = 0 channel, assuming dominance of a scalar resonance, B → S 0 → ππ.…”
Section: Jhep10(2017)117mentioning
confidence: 99%