2014
DOI: 10.1103/physrevd.89.094028
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Next-to-leading logarithmic QCD contribution of the electromagnetic dipole operator toB¯Xsγγwith a massive st

Abstract: We calculate the O(α s ) corrections to the double differential decay width dΓ 77 /(ds 1 ds 2 ) for the processB → X s γγ originating from diagrams involving the electromagnetic dipole operator O 7 . The kinematical variables s 1 and s 2 are defined as s i = (p b − q i ) 2 /m 2 b , where p b , q 1 , q 2 are the momenta of b-quark and two photons. We introduce a nonzero mass m s for the strange quark to regulate configurations where the gluon or one of the photons become collinear with the strange quark and ret… Show more

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Cited by 7 publications
(28 citation statements)
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“…the reviews [10,11] and references therein). On the other hand, the matrix elements sγγ|O i |b and sgγγ|O i |b , which in a NLL calculation are needed to order g 2 s and g s , respectively, are only partially known by now (see [16][17][18] for the details of the provided NLL contributions and [43] for a recent summary).…”
Section: Theoretical Framework and Kinematical Cutsmentioning
confidence: 99%
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“…the reviews [10,11] and references therein). On the other hand, the matrix elements sγγ|O i |b and sgγγ|O i |b , which in a NLL calculation are needed to order g 2 s and g s , respectively, are only partially known by now (see [16][17][18] for the details of the provided NLL contributions and [43] for a recent summary).…”
Section: Theoretical Framework and Kinematical Cutsmentioning
confidence: 99%
“…[10,11] for reviews). Regarding the B → X s γγ decay, the leading logarithmic (LL) prediction for the branching ratio was known since a long time [12][13][14][15], while the first attempts towards a NLL calculation were only made years later by us [16,17], in which the QCD corrections to the numerically dominant (O 7 , O 7 ) contribution were worked out in certain approximations which will be detailed in the next paragraph. In 2015, we also provided the contributions stemming from the self-interference of chromomagnetic dipole operator O 8 [18].…”
Section: Introductionmentioning
confidence: 99%
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“…In Refs. [89,90] useful parametrizations for the phasespace factors D<F(1 -n) have been given for n = 3,4, for the case where all final-state particles are massive. In our problem we only use the case n = 3 where only the neutralino is massive; this means that the general formula simplifies.…”
Section: Relevant Phase-space Formulasmentioning
confidence: 99%