论文标题
透明的低密度恒星等离子体在非常大的质量和深色光环的非常大的体积上延伸
Transparent low-density stellar plasma extending over very large volumes with large masses and Dark Haloes
论文作者
论文摘要
具有玻尔兹曼统计的自由电子模型，用于球形低密度等离子体（科学报告9.20384，2019），通过数值计算进一步开发，渐近关系获得了电子，质量密度和此类等离子体潜力的密度。溶液的开发是纯数X与距离恒星等离子体中心（Galaxy Center）的距离成正比的函数，其系数极小，因此这些溶液本质上是大天文距离和质量的函数。目前的等离子体分为一个中央部分和很长的尾部，其中大部分等离子体都包含在长恒星等离子体尾巴中。本模型专门用于完全离子化的氢血浆，其中在低密度恒星等离子体中可以忽略光谱线的发射和吸收。结果表明，当前的低密度血浆可能代表深色光环，渗透并包围紧凑的银河恒星。在大多数EM频谱中，发现这种血浆是透明的。
The free electron model with Boltzmann statistics for spherical low-density plasmas (Scientific Reports 9. 20384, 2019) is developed further by numerical calculations with asymptotic relations obtaining the density of electrons, mass densities and the potentials of such plasmas. Solutions are developed as function of a pure number x proportional to the distance from the stellar plasma center (galaxy center) with extremely small coefficient so that these solutions are essentially functions of large astronomical distances and masses. The present plasma is divided into a central part and very long tail where most of the large mass of this plasma is included in the long stellar plasma tail. The present model is specialized to completely ionized Hydrogen plasma where emission and absorption of spectral lines can be neglected in the low density stellar plasma. It is shown that the present low-density plasma might represent dark halo which permeates and surrounds the compact galactic stars. Such plasma is found to be transparent in most of the EM spectrum.
