The Galaxy Power Spectrum and Bispectrum in Redshift Space
arXiv:1806.04015 · doi:10.1088/1475-7516/2018/12/035
Abstract
We present the complete expression for the next-to-leading (1-loop) order galaxy power spectrum and the leading-order galaxy bispectrum in redshift space in the general bias expansion, or equivalently the effective field theory of biased tracers. We consistently include all line-of-sight dependent selection effects. These are degenerate with many, but not all, of the redshift-space distortion contributions, and have not been consistently derived before. Moreover, we show that, in the framework of effective field theory, a consistent bias expansion in redshift space must include these selection contributions. Physical arguments about the tracer sample considered and its observational selection have to be used to justify neglecting the selection contributions. In summary, the next-to-leading order galaxy power spectrum and leading-order galaxy bispectrum in the general bias expansion are described by 22 parameters, which reduces to 11 parameters if selection effects can be neglected. All contributions to the power spectrum can be written in terms of 28 independent loop integrals.
61 pages, 2 figures. The version published in JCAP, except that the supplementary material pointing to GitHub
References in corpus (18)
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- A test of the nature of cosmic acceleration using galaxy redshift distortions
- The Effective Field Theory of Cosmological Large Scale Structures
- Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
- New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
- Gravity and Large-Scale Non-local Bias
- Testing cosmological structure formation using redshift-space distortions
- The IR-resummed Effective Field Theory of Large Scale Structures
- Infrared Resummation for Biased Tracers in Redshift Space
- Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
- Baryon acoustic signature in the clustering of density maxima
- On the IR-Resummation in the EFTofLSS
- An analytic model for the bispectrum of galaxies in redshift space
- Modeling the three-point correlation function
- FFT-PT: Reducing the two-loop large-scale structure power spectrum to low-dimensional radial integrals
- The impact of Lyman- radiative transfer on large-scale clustering in the Illustris simulation
- A Radial Measurement of the Galaxy Tidal Alignment Magnitude with BOSS Data
- Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
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