论文标题

从2H,3H和3HE中最低原子轨道吸收的触发吸收

Pion absorption from the lowest atomic orbital in 2H, 3H and 3He

论文作者

Golak, J., Urbanevych, V., Skibinski, R., Witala, H., Topolnicki, K., Baru, V., Filin, A. A., Epelbaum, E., Kamada, H., Nogga, A.

论文摘要

PI - + 2H-> n + n,pi - + 3h-> n + n + n,pi - + 3he-> n + d和pi- + 3he-> p + n + n捕获反应在完全纳入最终状态相互作用的情况下,研究了最低原子轨道的捕获反应。我们的结果是通过手性有效田间理论领先顺序的单核和两个核子过渡算子获得的。初始和最后的三核子状态是通过手性核子核子SMS电位计算的,高达N4LO+由一贯的正则性手性N2lo三核电势增强。我们发现,吸收率很大程度上取决于使用的核锥形吸收算子,其两体零件将速率降低了几个数量级。由两个核子产生的核子之间的最终状态相互作用也很重要,而三核子相互作用仅在pi- + 3he-> n + d反应中起着可见的作用。我们对PI- + 2H-> n + N过程的吸收率与Pionic Deuterium的Hadroonic地基态扩展的实验数据非常吻合。 3HE上的捕获率通常与误差线中的光谱数据一致,尽管我们的中心值被系统地低于数据。我们表明,对于三体破裂过程,对吸收率的主要贡献是由准无散射和最终状态相互作用运动构型产生的。

The pi- + 2H -> n + n, pi- + 3H -> n + n + n, pi- + 3He -> n + d and pi- + 3He -> p + n + n capture reactions from the lowest atomic orbitals are studied under full inclusion of final state interactions. Our results are obtained with the single-nucleon and two-nucleon transition operators derived at leading order in chiral effective field theory. The initial and final three-nucleon states are calculated with the chiral nucleon-nucleon SMS potential up to N4LO+ augmented by the consistently regularized chiral N2LO three-nucleon potential. We found that absorption rates depend strongly on the nuclear pion absorption operator used, and its two-body parts change the rates by a few orders of magnitude. The final state interactions between nucleons generated by the two-nucleon forces are also important, while the three-nucleon interaction plays a visible role only in the pi- + 3He -> n + d reaction. Our absorption rate for the pi- + 2H -> n + n process is in good agreement with the experimental data from the hadronic ground-state broadening in pionic deuterium. The capture rates on 3He are also generally consistent with the spectroscopic data within error bars, though our central values are found to be systematically below the data. We show that for the three-body breakup processes the dominant contributions to the absorption rates arise from the quasi-free scattering and final-state interaction kinematical configurations.

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