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宇宙诞生时的婴啼——来自暴胀的随机引力波背景

The infant cry of the universe——stochastic gravitational wave background from inflation

  • 摘要: 文章将介绍起源于宇宙极早期暴胀阶段的引力波。暴胀是宇宙热大爆炸开始之前的一段短暂的加速膨胀阶段,在暴胀期间,起源于量子扰动的曲率扰动和张量扰动都被拉伸到宏观尺度上。前者是大尺度结构和微波背景辐射各向异性的起源,后者则能形成原初引力波。在下一阶,曲率扰动的四极矩可以作为引力波源,特别是增强的曲率扰动同时能够形成大量原初黑洞和可观测的次级引力波,而后者是空间引力波探测的重要科学目标。

     

    Abstract: This article recounts the origin of gravitational waves from the very birth of the universe. Cosmic inflation is the short period of accelerated expansion prior to the onset of the hot Big Bang. Initially generated from quantum fluctuations, both curvature and tensor perturbations are stretched to cosmological scales; the former serve as the seeds of large-scale structures and the anisotropies of the cosmic microwave background, while the latter form primordial gravitational waves. At the next order, the quadrupole moment of the curvature perturbations can also act as a source of gravitational waves. In particular, enhanced curvature perturbations can simultaneously form abundant primordial black holes and observable secondary gravitational waves. The latter constitute one of the key scientific goals for space-based gravitational wave detectors.

     

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