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Impact of medium modifications of the nucleon weak and electromagnetic form factors on the neutrino mean free path in dense matter

机译:中核弱和电磁形状因子对致密物质中的核心弱和电磁形状因素的影响

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摘要

Impact of the in-medium modified nucleon weak and electromagnetic form factors on the neutrino mean free path in dense matter is studied by considering both the weak and electromagnetic interactions of neutrinos with the constituents of the matter. A relativistic mean field model and the quark-meson coupling model are respectively adopted for the in-medium effective nucleon mass and nucleon form factors. We find that the cross sections of neutrino scattering in cold nuclear medium decrease when the in-medium modifications of the nucleon weak and electromagnetic form factors are taken into account. This reduction results in the enhancement of the neutrino mean free path, in particular at the baryon density of around a few times of the normal nuclear matter density. The enhancement of the neutrino mean free path is estimated to be about 10%-40% compared with the values obtained without the medium modifications of the nucleon form factors, and the enhancement is expected to accelerate the cooling of neutron stars.
机译:通过考虑Neutrinos与物质成分的弱和电磁相互作用,研究了中介质改性核仁弱和电磁形状因子的影响。相对论平均场模型和夸克 - 中思偶联模型分别用于中型有效核聚核群和核仁形态因子。我们发现,当考虑核核心弱和电磁形式因子的中式修饰时,冷核介质中的中微子散射的横截面降低。这种降低导致增强中微子均值的自由路径,特别是在正常核物质密度的大约几次的重孔密度下。与没有核子形式因子的培养基修饰的无需介质修饰,估计中微子均值平均值的增强约为10%-40%,并且预期增强将加速中子恒星的冷却。

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