外太空气体云在冷却的同时自发引力收缩的可能性

A. Belyaev
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引用次数: 1

摘要

外层空间的气体云总是由于电磁辐射而损失能量,即是非孤立的热力学系统。在一定条件下,气体云的能量损失会导致色散过程被自发引力压缩过程所取代。在这些自发压缩起始过程的条件下,云被压缩所释放的引力能将对应于它所经历的电磁辐射损失。此外,在焓不变的情况下,云会随着内能的减少而缩小。因此,外层空间气体云的自发引力压缩过程将伴随着气体云温度的降低。这种压缩气体云并同时冷却的机制,在宇宙演化的某个阶段,可以控制隐藏星系质量形成的可能过程之一。
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The Possibility of Spontaneous Gravitational Contraction of a Gas Cloud in Outer Space with Simultaneous Cooling of the Cloud
Gas clouds in outer space always lose energy due to electromagnetic radiation, i.e., are non-isolated thermodynamic systems. Under certain conditions, the energy loss of the gas cloud can lead to replacement of the process of dispersion by the process of spontaneous gravitational compression. Under these conditions of the initiation process of spontaneous compression, the gravitational energy released by the compression of the cloud will correspond to losses due to electromagnetic radiation it experiences. Furthermore, the cloud will shrink with a decrease in internal energy with constant enthalpy. As a result, the process of spontaneous gravitational compression of a gas cloud in outer space will be accompanied by a decrease in the temperature of the cloud. This mechanism of compression of a gas cloud with simultaneous cooling could, at a certain stage of the evolution of the universe, govern one of the possible processes of formation of a hidden mass of galaxies.
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