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General relativity and relativistic astrophysics

机译:广义相对论和相对论天体物理学

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Einstein established the theory of general relativity and the corresponding field equation in 1915 and its vacuum solutions were obtained by Schwarzschild and Kerr for, respectively, static and rotating black holes, in 1916 and 1963, respectively. They are, however, still playing an indispensable role, even after 100 years of their original discovery, to explain high energy astrophysical phenomena. Application of the solutions of Einstein's equation to resolve astrophysical phenomena has formed an important branch, namely relativistic astrophysics. I devote this article to enlightening some of the current astrophysical problems based on general relativity. However, there seem to be some issues with regard to explaining certain astrophysical phenomena based on Einstein's theory alone. I show that Einstein's theory and its modified form, both are necessary to explain modern astrophysical processes, in particular, those related to compact objects.
机译:爱因斯坦在1915年建立了广义相对论和相应的场方程,其真空解由Schwarzschild和Kerr分别于1916年和1963年获得,用于静态和旋转黑洞。然而,即使在最初发现100年后,它们仍然发挥着不可或缺的作用,以解释高能天体物理学现象。爱因斯坦方程组解决天体物理现象的应用已经形成了一个重要的分支,即相对论天体物理学。我将这篇文章专门介绍基于广义相对论的当前一些天体物理学问题。但是,仅基于爱因斯坦的理论来解释某些天体物理学现象似乎存在一些问题。我证明,爱因斯坦的理论及其修改形式对于解释现代天体物理学过程,特别是与紧凑物体有关的过程都是必要的。

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