论文标题
旋转旋转对第一代恒星崩溃成中子星而不是黑洞中的旋转效应，而不是黑洞
Spin-Torsion effect on collapsing of first generation stars into neutron stars rather than black holes in Einstein-Cartan-Sciama-Kibble theory
论文作者
论文摘要
在这个项目中，我们试图找到巨大的中子星体内部的非本地压力之间的相关性，这些星星抵抗了核心的重力塌陷和Quark场之间的自旋扭转耦合的效果和在非常高的核密度大得多。将暗能量注射到大型中子星（曼）的核心和这种黑暗能量对人类通过抗重力崩溃的额外抗性性质，这可能使中子恒星在未观察到的质量范围内存在于[216亿美元_ {\ odot}，5m _ {\ odot} {\ odot}] $。获得ECSK TOV方程会给人类环境介质的局部压力。此外，再次从拉格朗日（Lagrangian）获得了来自ECSK暗能量的负压，我们可以从中研究曼斯（Mans）核心和环境培养基的水力静态平衡。如果对于ECSK理论框架中的人群的未观察到的质量差距满足了平衡状态，这将暗示我们的模型预测天体物理学研究中人类的巨大质量范围。
In this project, we try to find the correlation between the non-local pressure inside the massive neutron stars resisting the gravitational collapse of the core and ECSK dark energy led by the effect of spin-torsion coupling between quark fields and the space-time at very high densities much larger than the nuclear density. The injection of dark energy into the core of massive neutron stars (MANs) and extra resistant nature of this dark energy to the collapse of MANs by the anti-gravity give the possibility of existence of neutron stars in the unobserved mass range of $[2.16M_{\odot},5M_{\odot}]$. Obtaining the ECSK TOV equation gives the local pressure of the ambient medium of MANs. Moreover, the negative pressure from the ECSK dark energy is obtained from the Lagrangian again, from which we are able to investigate the hydro-static equilibrium of the core and ambient medium of the MANs. If the equilibrium state is satisfied for the unobserved mass gap for the MANs in ECSK theory framework this will imply our model predicts this vast mass range of unobserved spectrum of the MANs in astrophysical studies.
