2003
DOI: 10.1016/s0550-3213(02)01017-9
|View full text |Cite
|
Sign up to set email alerts
|

Photon distribution amplitudes in QCD

Abstract: Abstract:We develop a consistent technique for the calculation of real photon emission in hard exclusive processes, which is based on the background field formalism and allows a convenient separation of hard electromagnetic and soft hadronic components of the photon. The latter ones are related to matrix-elements of light-cone operators in the electromagnetic background field and can be parametrized in terms of photon distribution amplitudes. We construct a complete set of photon distribution amplitudes up to … Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

27
438
2
2

Year Published

2009
2009
2021
2021

Publication Types

Select...
4
3

Relationship

0
7

Authors

Journals

citations
Cited by 230 publications
(469 citation statements)
references
References 53 publications
27
438
2
2
Order By: Relevance
“…The collinear Wilson line with the convention of the covariant derivative To establish the hard-collinear factorization for the QCD amplitude (3.3), we further decompose the SCET operator O A,µ into the light-ray operators defining the photon DAs displayed in [16] …”
Section: 1mentioning
confidence: 99%
See 3 more Smart Citations
“…The collinear Wilson line with the convention of the covariant derivative To establish the hard-collinear factorization for the QCD amplitude (3.3), we further decompose the SCET operator O A,µ into the light-ray operators defining the photon DAs displayed in [16] …”
Section: 1mentioning
confidence: 99%
“…The second Gegenbauer moment of the leading-twist photon DA will be further taken as a 2 (µ 0 ) = 0.07 ± 0.07 as obtained in [16]. The magnetic susceptibility of the quark condensate χ(1 GeV) = (3.15 ± 0.3) GeV −2 computed from the QCD sum rule approach including the O(α s ) corrections [16] and the quark condensate density qq (1 GeV) = −(246 +28 −19 MeV) 3 determined by the GMOR relation [39] will be also employed for the numerical estimates in the following.…”
Section: Theory Inputsmentioning
confidence: 99%
See 2 more Smart Citations
“…The first four raws in Table 4 contain the results obtained applying sum rules in different contexts: analysing the of nucleon magnetic moments and Δ → Nγ radiative transitions [47], studying photon distribution amplitudes in QCD [50] or radiative heavy meson decays [51]. Method (renormalization point) c χ Sum rules (1 GeV) [47] 3.86 ± 0.11 Sum rules (0.5 GeV) [48] 2.56 Sum rules (1 GeV) [49] 1.98 ± 0.18 Sum rules (1 GeV) [50] 1.41 ± 0.13 Sum rules (1 GeV) [51] 1.28 ± 0.22 OPE + Pion Dominance (0.5 GeV) [52] 2 Instanton vacuum (1 GeV) [53] 1.12 ± 0.07 Zero mode of Dirac Op.…”
Section: Some Facts About χmentioning
confidence: 99%