夸克星
- 网络quark star
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简要地回顾了脉冲星、中子星和夸克星的研究历史;
Studies of pulsars , neutron stars , and quark stars are reviewed .
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文章估算了夸克星的质量极限和半径。
This article estimates the mass limit , degeneration and radius of quark stars .
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因质量的大小而形成脉冲星、中子星、夸克星,质量大到一定值的生成黑洞。
Pulsars , neutron stars and quark stars are then created based on their mass .
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脉冲星与夸克星
Pulsars and Quark Stars
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一般认为这些信号源就是夸克星或中子星,其中一些已经通过传统的方法观测到,称为脉冲星。
Such sources are believed to be either quark stars or neutron stars , and a subclass of these are already observed by conventional means as pulsars or X-ray emitting celestial objects .
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根据粒子物理理论和量子简并理论,本文认为自然界存在夸克星,这是恒星演化最后阶段形成的一类产物。
According to the particle physics theory and the quantum degeneration theory , this paper considers that quark stars are in existence in nature . They are the product of the last stage of the star 's evolutionary process .