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Neutrino-induced neutral-current reaction cross sections for r-process nuclei

机译:中微子诱导的r过程核的中性电流反应截面

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Neutrino-induced reactions play an important role during and after the r-process, if the latter occurs in an environment with extreme neutrino fluxes such as the neutrino-driven wind model or neutron star mergers. Recently we have evaluated the charged-current neutrino-nucleus cross sections relevant for r-process simulations. We extend our approach here to the neutral-current cross sections. Our tabulation considers neutron-rich nuclei with neutron numbers N = 41-135 and charge numbers Z = 21-82 and lists total as well as partial neutron spallation cross sections. The calculations have been performed within the random phase approximation considering multipole transitions with J less than or equal to 3 and both parities. The supernova neutrino spectrum is described by a Fermi-Dirac distribution with various temperature parameters between T = 2.8 MeV and T = 10 MeV and with the degeneracy parameters alpha = 0 and alpha = 3. (C) 2002 Elsevier Science (USA). [References: 13]
机译:如果r过程在中微子通量极高的环境(例如中微子驱动的风模型或中子星合并)中发生,则中微子诱导的反应在r过程中和过程中起着重要作用。最近,我们评估了与r过程模拟相关的带电电流中微子核的横截面。在这里,我们将方法扩展到中性线横截面。我们的列表考虑了中子数为N = 41-135,电荷数为Z = 21-82的富中子核,并列出了全部以及部分中子散裂截面。考虑到J小于或等于3的多极跃迁以及两个奇偶校验,已经在随机相位近似内执行了计算。超新星中微子光谱由费米-狄拉克分布描述,费米-狄拉克分布的各种温度参数在T = 2.8 MeV和T = 10 MeV之间,简并性参数alpha = 0和alpha =3。(C)2002 Elsevier Science(美国)。 [参考:13]

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