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首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >Relationship between Bondi-Sachs quantities and source of gravitational radiation in asymptotically de Sitter spacetime
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Relationship between Bondi-Sachs quantities and source of gravitational radiation in asymptotically de Sitter spacetime

机译:渐近德保姆时尚邦德 - 群集数量与重力辐射源的关系

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摘要

Gravitational radiation plays an important role in astrophysics. Based on the fact that our universe is expanding, the gravitational radiation when a positive cosmological constant is presented has been studied along with two different ways recently, one is the Bondi-Sachs (BS) framework in which the result is shown by BS quantities in the asymptotic null structure, the other is the perturbation approach in which the result is presented by the quadrupoles of source. Therefore, it is worth to interpret the quantities in asymptotic null structure in terms of the information of the source. In this paper, we investigate this problem and find the explicit expressions of BS quantities in terms of the quadrupoles of source in asymptotically de Sitter spacetime. We also estimate how far away the source is, the cosmological constant may affect the detection of the gravitational wave.
机译:引力辐射在天体物理学中起着重要作用。 基于我们的宇宙正在扩展的事实,在播出了正宇宙常数时的引力辐射最近已经研究了两种不同的方式,其中一个是Bondi-Sachs(BS)框架,其中通过BS量示出了结果 渐近空结构,另一个是源极的扰动方法,其中由源极弦介绍。 因此,在源的信息方面,值得解释渐近空结构中的数量。 在本文中,我们调查了这个问题,并在渐近的de Satter时空的源极Quadrupols方面找到了BS数量的明确表达。 我们还估计了源的远距离,宇宙常数可能会影响引力波的检测。

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