论文标题
反物质球状簇的弧形通量
Anihelium flux from antimatter globular cluster
论文作者
论文摘要
宏观宇宙反物质物体是在强烈非杂种性的baryosynthesis模型中预测的。我们通过评估银河系宇宙射线中氦抗核的浮肿来检验银河系中的抗星状群的旧植物簇的假设。由于物质和反物质的象征性，我们假设反物质簇的方式与物质簇相似。来自反物质球状聚类的银河宇宙射线中antiparticle的能量密度估计。我们提出了一种方法，可以从银河系中的球状磁场中的银河磁场中膨胀抗核酸菌素传播。
Macroscopic cosmic antimatter objects are predicted in baryonasymmetrical Universe in the models of strongly nonhomogeneousbaryosynthesis. We test the hypothesis of the existence of an oldglobular cluster of anti-stars in the galactic halo by evaluating theflux of helium anti-nuclei in galactic cosmic rays. Due to the symme-try of matter and antimatter we assume that the antimatter clusterevolves in a similar way as a matter cluster. The energy density ofantiparticles in galactic cosmic rays from antimatter globular clusteris estimated. We propose a method for the propagation of a fluxof antinuclei in a galactic magnetic field from the globular cluster ofantistars in the Galaxy.
