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Redshift space power spectrum beyond Einstein-de Sitter kernels
Journal of Cosmology and Astroparticle Physics ( IF 5.3 ) Pub Date : 2021-04-15 , DOI: 10.1088/1475-7516/2021/04/039
Alejandro Aviles 1, 2 , Georgios Valogiannis 3 , MarioA. Rodriguez-Meza 2 , JorgeL. Cervantes-Cota 2 , Baojiu Li 4 , Rachel Bean 5
Affiliation  

We develop a framework to compute the redshift space power spectrum (PS), with kernels beyond Einstein-de Sitter (EdS), that can be applied to a wide variety of generalized cosmologies. We build upon a formalism that was recently employed for standard cosmology in Chen, Vlah & White (2020), and utilize an expansion of the density-weighted velocity moment generating function that explicitly separates the magnitude of the k-modes and their angle to the line-of-sight direction dependencies. We compute the PS for matter and biased tracers to 1-loop Perturbation Theory (PT) and show that the expansion has a correct infrared and ultraviolet behavior, free of unwanted divergences. We also add Effective Field Theory (EFT) counterterms, necessary to account for small-scale contributions to PT, and employ an IR-resummation prescription to properly model the smearing of the BAO due to large scale bulk flows within Standard-PT. To demonstrate the applicability of our formalism, we apply it on the ΛCDM and the Hu-Sawicki f(R) models, and compare our numerical results against the elephant suite of N-body simulations, finding very good agreement up to k = 0.27 Mpc-1 h at z = 0.5 for the first three non-vanishing Legendre multipoles of the PS. To our knowledge, the model presented in this work is the most accurate theoretical EFT-PT for modified gravity to date, being the only one that accounts for beyond linear local biasing in redshift-space. Hence, we argue our RSD modeling is a promising tool to construct theoretical templates in order to test deviations from ΛCDM using real data obtained from the next stage of cosmological surveys such as DESI and LSST.



中文翻译:

超越 Einstein-de Sitter 核的红移空间功率谱

我们开发了一个框架来计算红移空间功率谱 (PS),其内核超出了 Einstein-de Sitter (EdS),可应用于各种广义宇宙学。我们以最近在 Chen, Vlah & White (2020) 中用于标准宇宙学的形式主义为基础,并利用密度加权速度矩生成函数的扩展,明确区分 k 模式的大小及其与视线方向依赖性。我们计算了物质的 PS 和偏置示踪剂到 1 环微扰理论 (PT),并表明膨胀具有正确的红外和紫外行为,没有不需要的发散。我们还添加了有效场论 (EFT) 反术语,这对于解释对 PT 的小规模贡献是必要的,并采用 IR 恢复处方来正确模拟由于 Standard-PT 内的大规模散装流导致的 BAO 拖尾。为了证明我们形式主义的适用性,我们将其应用于 ΛCDM 和 Hu-Sawicki f(R) 模型,并将我们的数值结果与 N 体模拟的大象套件进行比较,发现非常吻合对于 PS 的前三个非消失勒让德多极子,在z = 0.5 时k = 0.27 Mpc -1 h 。据我们所知,这项工作中提出的模型是迄今为止修正重力的最准确的理论 EFT-PT,是唯一一个能够解释红移空间中线性局部偏差之外的模型。因此,我们认为我们的 RSD 建模是构建理论模板的有前途的工具,以便使用从下一阶段的宇宙学调查(例如 DESI 和 LSST)获得的真实数据来测试与 ΛCDM 的偏差。

更新日期:2021-04-15
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