论文标题
一个新的引力黑洞
A new gravitational black-hole
论文作者
论文摘要
在最近的一篇论文中，我们分析了基于费米（弱）相互作用与重力之间的亲密关系的重力理论（STG）。我们提出了以下假设：物质对代表重力相互作用的度量的影响是有效的。这使我们认为引力是两个中性旋转场（G-Neutrinos）$ψ_g$和$ω_g$与各种物质和能量通过产生这种有效度量的相互作用的结果。换句话说，代表一般相对性框架中重力相互作用的通用度量是用与$ψ_g$和$ω_g$相关的弱电流构建的。在第一篇论文中，我们已经表明，当仅存在一个旋转器时，静态和球体对称构型的有效度量与GR的Schwarzschild几何形状相同。在本文中，我们更进一步，考虑到字段$ψ_g$具有自私的情况。静态和球形对称配置的解与前一个构型不同。这个新解决方案介绍了我们与Schwarzschild情况进行比较的另一个视野。
In a recent paper we have analyzed the Spinor Theory of Gravity (STG) which is based on the intimate relation between Fermi (weak) interaction and gravity. We presented the hypothesis that the effect of matter upon the metric that represents gravitational interaction in General Relativity is an effective one. This lead us to consider gravitation to be the result of the interaction of two neutral spinorial fields (G-neutrinos) $Ψ_g$ and $Ω_g$ with all kinds of matter and energy through the generation of such effective metric. In other words, the universal metric that represents gravitational interaction in the framework of General Relativity is constructed with the weak currents associated to $Ψ_g$ and $Ω_g$. In the first paper we have shown that when only one spinor exists, the effective metric of a static and spherically symmetric configuration is identical to the Schwarzschild geometry of GR. In the present paper we go one step further and consider the case in which the field $Ψ_g$ has a self-interaction. The solution of a static and spherically symmetric configuration is distinct from the previous one. This new solution presents another horizon that we compare with the case of Schwarzschild.
