论文标题
圆环形磁虫洞可能形成环星系
Possible formation of ring galaxies by torus-shaped magnetic wormholes
论文作者
论文摘要
我们提出了这样的假设，即某些环星系是由遗物磁环形形成的虫洞形成的。在虫洞重组磁场之前的原始血浆中，能量小于阈值能量。它们是麦克斯韦的恶魔从最近的（地平线大小）区域收集重子，从而形成了与虫洞喉咙相同的圆环状形状的大块物质。这样的团块可以用作形成环星系和具有环形形式的较小物体的种子。在重组后，圆环状的团块可能会腐烂并合并。与星系不同，此类物体在光环中可能包含更少甚至没有暗物质。但是，此类物体最严格的特征是存在大型的环形磁场。我们表明，磁场有阈值，这些磁场为这种原始马克西群中的巴属团块的上和下边界值提供了阈值。
We present the hypothesis that some of ring galaxies were formed by relic magnetic torus - shaped wormholes. In the primordial plasma before the recombination magnetic fields of wormholes trap baryons whose energy is smaller than a threshold energy. They work as the Maxwell's demons collecting baryons from the nearest (horizon size) region and thus forming clumps of baryonic matter which have the same torus-like shapes as wormhole throats. Such clumps may serve as seeds for the formation of ring galaxies and smaller objects having the ring form. Upon the recombination torus-like clumps may decay and merge. Unlike galaxies, such objects may contain less or even no dark matter in halos. However the most stringent feature of such objects is the presence of a large - scale toroidal magnetic field. We show that there are threshold values of magnetic fields which give the upper and lower boundary values for the baryon clumps in such protogalaxies.
