本文从理想流体、均匀密度模型解爱因斯坦场方程得到恒星的临界质量。
In this paper, the critical mass of stars is obtained by solving Einstein's field equations by means of the model of perfect fluid medium with uniform density.
本文给出了一个新的生成解定理和一个新的爱因斯坦·麦克·斯威场方程的严格解。
In this paper we have reached a new theorem on generation solutions and a new exact solution of Einstein-Maxwell Eguations.
本文给出了一个新的生成解定理和一个新的爱因斯坦·麦克·斯威场方程的严格解。
In this paper we have reached a new theorem on generation solutions and a new exact solution of Einstein-Maxwell Eguations.
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