Perturbations of cosmological redshift drift

被引:2
|
作者
Bessa, Pedro [1 ,2 ,3 ]
Durrer, Ruth [1 ,2 ]
Stock, Dennis [1 ,2 ]
机构
[1] Univ Geneva, Dept Phys Theor, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland
[2] Univ Geneva, Ctr Astroparticle Phys, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland
[3] Univ Fed Espirito Santo, PPGCosmo UFES, BR-29075910 Vitoria, Brazil
基金
瑞士国家科学基金会;
关键词
Cosmological perturbation theory in GR and beyond; power spectrum; dark energy theory;
D O I
10.1088/1475-7516/2023/11/093
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we calculate the linear perturbations of the cosmological redshift drift. We show explicitly that our expressions are gauge-invariant and compute the power spectrum of the redshift drift perturbations and its correlations with galaxy number counts within linear perturbation theory. Our findings show that the perturbations are small, and that the peculiar velocity and acceleration terms are dominating and cannot be neglected when modeling the full perturbative expression for the redshift drift. We also find that the cross-correlations with galaxy number count fluctuations might increase the detectability of the effect and can help to separate the perturbative effects from the background cosmological redshift drift signal.
引用
收藏
页数:22
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