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The perturbation of gravitational waves in plasma in the FRW space-time

机译:FRW时空中等离子体引力波的扰动

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In this paper we study the perturbation of gravitational waves in plasma, using the relativistic hydro-magnetic equation in the so-called Cowling approximation considering a Friedman-Robertson-Walker (FRW) cosmological model. It has been assumed the gravitational field and the weak magnetic field do not break the homogeneity and isotropy of the considered FRW space time. Applying the formalism proposed for Zel'dovich and Novikov (The structure and evolution of the universe, Volume II, 1983), Brandenburg et al. (Phys. Rev. D 54: 1291, 1996) and Weinberg (Gravitation and Cosmology, 1972). We verify that density fluctuation may be obtained.
机译:在本文中,我们在考虑了弗里德曼-罗伯逊-沃克(FRW)宇宙学模型的所谓考林近似中,使用相对论性水磁方程,研究了等离子体中的引力波扰动。假设重力场和弱磁场不会破坏所考虑的FRW时空的均匀性和各向同性。布兰登堡(Brandenburg)等人应用了为泽尔多维奇(Zel'dovich)和诺维科夫(Novikov)提出的形式主义(宇宙的结构和演化,第二卷,1983年)。 (Phys。Rev. D 54:1291,1996)和Weinberg(Gravitation and Cosmology,1972)。我们验证可以得到密度波动。

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