1991
DOI: 10.1007/bf01549699
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Jet cone size dependence of inclusive cross-sections toO(? s 3 )

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Cited by 35 publications
(25 citation statements)
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“…Neglecting O(R 2 ) pieces, the evaluation and phase-space integration of the partonic cross sections can be performed analytically. This approximation has been shown [231,232,233,147] to account extremely well for jet observables up to cone sizes of about R ≈ 0.7 in related pp-scattering reactions by explicit comparison to calculations that take R fully into account. Figure 1.50 presents our results [234] for the expected NLO double-spin asymmetry A jet LL for single-inclusive jet photoproduction at √ S = 100 GeV for two different choices of proton helicity densities [24,25] and the two extreme sets of polarized photon densities introduced above.…”
Section: Barbara Jäger Marco Stratmannmentioning
confidence: 94%
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“…Neglecting O(R 2 ) pieces, the evaluation and phase-space integration of the partonic cross sections can be performed analytically. This approximation has been shown [231,232,233,147] to account extremely well for jet observables up to cone sizes of about R ≈ 0.7 in related pp-scattering reactions by explicit comparison to calculations that take R fully into account. Figure 1.50 presents our results [234] for the expected NLO double-spin asymmetry A jet LL for single-inclusive jet photoproduction at √ S = 100 GeV for two different choices of proton helicity densities [24,25] and the two extreme sets of polarized photon densities introduced above.…”
Section: Barbara Jäger Marco Stratmannmentioning
confidence: 94%
“…We work in the so-called "small-cone approximation" [227,228,229,230,231] which can be considered as an expansion of the jet cross section in terms of R of the form A log R + B + O(R 2 ). Neglecting O(R 2 ) pieces, the evaluation and phase-space integration of the partonic cross sections can be performed analytically.…”
Section: Barbara Jäger Marco Stratmannmentioning
confidence: 99%
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“…Figure 6 shows the variation of the cross section with cone size for E t =100 GeV jets from CDF compared with O(α 3 s ) predictions [66,67,68]. The data display the statistical errors only, but the ≈ 23 % systematic uncertainties are largely independent of R. Since there are only two back-to-back partons in the LO calculation, one can only predict such a variation beginning at NLO.…”
Section: Inclusive Jet Productionmentioning
confidence: 99%
“…The NLO corrections to conventional high p ⊥ jet production cross section were computed in [18], [19] and [20] for Tevatron energies. Later the code of [19] was used for calculating this cross section for RHIC and LHC energies in [21].…”
Section: Introductionmentioning
confidence: 99%