宇宙弦存在下的原始引力波频谱

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
S. Azar Ag Ghaleh, A.M. Abbassi and M.H. Abbassi
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引用次数: 0

摘要

在本文中,我们考虑了一个沿 z 轴有长直宇宙弦的膨胀宇宙。我们证明宇宙弦效应可以被视为对 FRW 度量背景的扰动。通过对这个膨胀宇宙弦背景进行宇宙学扰动,我们导出了线性化的爱因斯坦场方程。我们证明,在前阶(忽略宇宙弦扰动与引力张量扰动的混合项),宇宙弦作为一个非均质项出现在张量扰动波方程的右侧。最后,通过寻找慢滚膨胀波方程的解析解,我们说明了它对原始引力波频谱的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spectrum of primordial gravitational waves in the presence of a cosmic string
In this paper we consider an inflating universe with long straight cosmic string along z-axis. We demonstrate that cosmic string's effect can be treated as a perturbation on the background of FRW metric. By performing cosmological perturbations on this inflating cosmic string background, we derived the linearized Einstein field equations. We show that at leading order (neglecting the mixing terms of cosmic string perturbations with gravitational tensor perturbations), the cosmic string appears as an inhomogeneous term on the right hand side of wave equation for tensor perturbations. Finally, by finding analytical solution of the wave equation for slow-roll inflation, we illustrate its impact on the spectrum of primordial gravitational waves.
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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