纯爱因斯坦引力对宇宙学密度功率谱贡献的红外发散
Infrared divergence of pure Einstein gravity contributions to cosmological density power spectrum
摘要:
我们探讨了纯爱因斯坦引力对二阶密度功率谱的贡献。在小尺度下,我们发现爱因斯坦引力的贡献很小,可以忽略不计。这保证了牛顿引力足以处理重子声学振荡尺度。然而,在大尺度下,我们发现爱因斯坦引力对二阶功率谱的贡献主导了线性功率谱。因此,纯爱因斯坦引力贡献出现在三级微扰导致红外发散的功率谱。
英文摘要:
We probe the pure Einstein's gravity contributions to the second-order density power spectrum. In the small-scale, we discover that the Einstein's gravity contribution is negligibly small. This guarantees that Newton's gravity is sufficient to handle the baryon acoustic oscillation scale. In the large scale, however, we discover that the Einstein's gravity contribution to the second-order power spectrum dominates the linear-order power spectrum. Thus, pure Einstein gravity contribution appearing in the third-order perturbation leads to an infrared divergence in the power spectrum.
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