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Spin Dependence of Deep Inelastic Diffraction

High Energy Physics - Phenomenology · Submitted 1 Jun 1999

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim A first numerical estimate indicates that the perturbative contribution to the spin asymmetry is substantially larger than the nonperturbative one.

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arXiv IDhep-ph/9906204 (version 1)
Pith ID6RL2E5XO, Pith's permanent record of this paper and its review
CitationJ.Bartels (Hamburg), M.G.Ryskin (St. Petersburg, Pnpi), T.Gehrmann (Karlsruhe, TTP). "Spin Dependence of Deep Inelastic Diffraction." arXiv:hep-ph/9906204 (1999). https://pith.science/paper/6RL2E5XO
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.50 · human participants 0.01 · controlled comparison 0.06 · randomized assignment 0.01 · states quantitative result 0.14 · compares with prior results 0.34 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

Using a perturbative model for diffractive interactions, we derive an expression for the polarized diffractive structure function $g_1^D$ in the high energy limit. This structure function is given by the interference of diffractive amplitudes with polarized and unpolarized exchanges. For the polarized exchange we consider both two-gluon and quark-antiquark amplitudes. The polarized diffractive amplitude receives sizable contributions from non-strongly ordered regions in phase space, resulting in a double logarithmic enhancement at small $x$. The resummation of these double logarithmic terms is outlined. We also discuss the transition from our perturbative expression to the nonperturbative region. A first numerical estimate indicates that the perturbative contribution to the spin asymmetry is substantially larger than the nonperturbative one.

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What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Using a perturbative model for diffractive interactions, we derive an expression for the polarized diffractive structure function $g_1^D$ in the high energy limit. contribution 0.78 0.96 0.08 asserted 1.00
s1 This structure function is given by the interference of diffractive amplitudes with polarized and unpolarized exchanges. result 0.62 0.64 0.06 asserted 1.00
s2 For the polarized exchange we consider both two-gluon and quark-antiquark amplitudes. method 0.84 0.72 0.03 asserted 0.90
s3 The polarized diffractive amplitude receives sizable contributions from non-strongly ordered regions in phase space, resulting in a double logarithmic enhancement at small $x$. result 1.00 0.89 0.21 asserted 1.00
s4 The resummation of these double logarithmic terms is outlined. method 0.78 0.83 0.05 asserted 0.77
s5 We also discuss the transition from our perturbative expression to the nonperturbative region. contribution 0.88 0.79 0.04 asserted 0.68
s6 A first numerical estimate indicates that the perturbative contribution to the spin asymmetry is substantially larger than the nonperturbative one. result 1.00 0.91 0.61 hedged possibility 0.99

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The paper
Original abstract

Using a perturbative model for diffractive interactions, we derive an expression for the polarized diffractive structure function $g_1^D$ in the high energy limit. This structure function is given by the interference of diffractive amplitudes with polarized and unpolarized exchanges. For the polarized exchange we consider both two-gluon and quark-antiquark amplitudes. The polarized diffractive amplitude receives sizable contributions from non-strongly ordered regions in phase space, resulting in a double logarithmic enhancement at small $x$. The resummation of these double logarithmic terms is outlined. We also discuss the transition from our perturbative expression to the nonperturbative region. A first numerical estimate indicates that the perturbative contribution to the spin asymmetry is substantially larger than the nonperturbative one.

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