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Large Scale Structure in Redshift Space

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Abstract

The mapping of dark matter clustering from real space to redshift space introduces the anisotropic property to the measured density power spectrum in redshift space, known as the redshift space distortion effect. The mapping formula is intrinsically non-linear, which is complicated by the higher order polynomials due to indefinite cross correlations between the density and velocity fields, and the Finger–of–God effect due to the randomness of the peculiar velocity field. Whilst the full higher order polynomials remain unknown, the other systematics can be controlled consistently within the same order truncation in the expansion of the mapping formula, as shown in this paper. The systematic due to the unknown non–linear density and velocity fields is removed by separately measuring all terms in the expansion directly using simulations. The uncertainty caused by the velocity randomness is controlled by splitting the FoG term into two pieces, 1) the “one–point” FoG term being independent of the separation vector between two different points, and 2) the “correlated” FoG term appearing as an indefinite polynomials which is expanded in the same order as all other perturbative polynomials. We introduce the recent progress on understanding this mapping, and the application for the future analysis to reveal the nature of cosmic acceleration.

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  1. Korea Astronomy and Space Science Institute, Daejeon, 34055, Korea

    Yong-Seon Song

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  1. Yong-Seon Song
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Correspondence to Yong-Seon Song.

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Song, YS. Large Scale Structure in Redshift Space. J. Korean Phys. Soc. 73, 504–515 (2018). https://doi.org/10.3938/jkps.73.504

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