伽玛射线暴的新和共同起源:一个发射辐射的星系种子分离

S. Nagao
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引用次数: 0

摘要

伽玛射线暴的机制尚不确定,而目前的候选,分别是短伽马暴和长伽马暴,是相当接受的。它们与一些观察到的事实相矛盾。本文用能量循环理论详细考察了一个能量循环分解为两个能量循环的过程。我们推导了分离星系种子的力和势能的方程。一个星系的种子垂直地分成两个种子。如果后退速度足够快,两颗种子就会垂直分离。如果还不够,它们就会被困在能量槽,从那里发生随后的平分离。势能的差部分以伽马射线辐射的形式散发出来。提出的过程很好地满足了grb的观测特征,这是标准宇宙学无法解释的。伽马射线暴是支持我们提出的星系演化模型的重要证据,该模型包括星系种子分离及其基础;能量循环理论。我们之前报道过的另一个关键证据是,该模型预测,在没有暗物质的任何径向距离上,星系的旋转速度都是恒定的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Novel and Common Origin of Gamma-ray Bursts: A Galactic Seed Separation with Emitting Radiations
The mechanism of the gamma-ray burst is uncertain while the current candidates, respectively, for short and long GRBs are rather accepted. They conflict with some observed facts. Here we examine in detail the process for an energy circulation to separate to two ones by the energy circulation theory. We derive the equations of the force and the potential energy for the separation of a galactic seed. A galactic seed divides to two seeds orthogonally. If the receding speed is high enough, two seeds separate away orthogonally. If not enough, they are trapped at the energy trough, from where a subsequent flat separation occurs. The difference in the potential energy is partly emitted as gamma-ray radiations. The proposed process nicely meets the observed features of the GRBs, which the standard cosmology cannot explain. The GRBs are an important evidence to support our proposed model of galactic evolution, which includes galactic seed separations, as well as its basis; the energy circulation theory. Another key evidence, which we reported previously, is that the model predicts a constant speed of a galaxy rotation at any radial distances without dark matter.
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