Impact of bias and redshift-space modelling for the halo power spectrum: testing the effective field theory of large-scale structure

DOI10.1088/1475-7516/2020/07/011zbMath1492.85012arXiv1805.12394OpenAlexW3100147203MaRDI QIDQ5070264

Lucía Fonseca de la Bella, David Parkinson, David Seery, D. Regan

Publication date: 11 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1805.12394

zbMATH Keywords

power spectrumgalaxy clustersgalaxy clusteringredshift surveys

Mathematics Subject Classification ID

Classification and discrimination; cluster analysis (statistical aspects) (62H30) Bayesian inference (62F15) Trees (05C05) Diffraction, scattering (78A45) Spectrum, resolvent (47A10) Quantum field theory on curved space or space-time backgrounds (81T20) Electromagnetic fields in general relativity and gravitational theory (83C50) Perturbations in context of PDEs (35B20) Galactic and stellar structure (85A15) Symmetries and conservation laws in mechanics of particles and systems (70S10) Effective quantum field theories (81T12)

Related Items (6)

Interacting dark energy from redshift-space galaxy clustering ⋮ The EFT likelihood for large-scale structure ⋮ Consistent modeling of velocity statistics and redshift-space distortions in one-loop perturbation theory ⋮ Hybrid P_ℓ(k): general, unified, non-linear matter power spectrum in redshift space ⋮ The EFT likelihood for large-scale structure in redshift space ⋮ Redshift-space distortions in Lagrangian perturbation theory

Cites Work

• Unnamed Item
• Estimating the dimension of a model
• Large-scale structure of the universe and cosmological perturbation theory
• Large-scale galaxy bias
• The effective field theory of cosmological large scale structures
• Elementary exact evaluation of infinite integrals of the product of several spherical Bessel functions, power and exponential
• Infinite Integrals Involving Three Spherical Bessel Functions
• The matter power spectrum in redshift space using effective field theory
• Very massive tracers and higher derivative biases

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