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Spin asymmetry for the 16O( γ ,πp) reaction in the Δ(1232) regionwithin an effective Lagrangian approach

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摘要

The spin asymmetry of the photon in the exclusive A( γ ,πN)A 1 reaction is computed employing arecently developed fully relativistic model based on elementary pion production amplitudes that includea consistent treatment of the spin-3/2 nucleon resonances. We compare the results of this model to theonly available data on Oxygen K. Hicks, et al., Phys. Rev. C 61 (2000) 054609 and find that, contraryto other models, the predicted spin asymmetry compares well to the available experimental data in theΔ(1232) region. Our results indicate that no major medium modifications in the Δ(1232) properties areneeded in order to describe the measured spin asymmetries.
机译:独有 A( γ ,πN)A 1 反应中光子的自旋不对称性是采用最近开发的基于基本介子产生振幅的完全相对论模型计算的,该模型包括对自旋 3/2 核子共振的一致处理。我们将该模型的结果与氧气上唯一可用的数据进行比较 [K. Hicks, et al., Phys. Rev. C 61 (2000) 054609] 并发现,与其他模型相反,预测的自旋不对称性与 Δ(1232) 区域的可用实验数据相比很好。我们的结果表明,为了描述测量的自旋不对称性,不需要对Δ(1232)性质进行重大的介质修改。

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