Modeling the marked spectrum of matter and biased tracers in real- and redshift-space

DOI10.1088/1475-7516/2021/03/038zbMath1484.85023arXiv2010.05914OpenAlexW3139464630MaRDI QIDQ5026003

Elena Massara, Oliver H. E. Philcox, Alejandro Aviles

Publication date: 7 February 2022

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

Full work available at URL: https://arxiv.org/abs/2010.05914

zbMATH Keywords

power spectrumcosmological perturbation theorygalaxy surveyscosmological parameters from LSS

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Diffraction, scattering (78A45) Many-body theory; quantum Hall effect (81V70) Gravitational energy and conservation laws; groups of motions (83C40) Perturbations in context of PDEs (35B20) Weak interaction in quantum theory (81V15) Galactic and stellar structure (85A15) Effective quantum field theories (81T12)

Related Items (2)

Fast computation of non-linear power spectrum in cosmologies with massive neutrinos ⋮ Redshift space power spectrum beyond Einstein-de Sitter kernels

Uses Software

• DLMF
• Quijote

Cites Work

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• On loops in inflation
• Large-scale structure of the universe and cosmological perturbation theory
• The effective field theory of cosmological large scale structures
• NIST digital library of mathematical functions
• Spatial distribution of galactic halos and their merger histories
• On Correlations of Marked Point Processes
• Cosmological perturbation theory using the FFTLog: formalism and connection to QFT loop integrals
• Matter trispectrum: theoretical modelling and comparison to N-body simulations
• The EFT likelihood for large-scale structure in redshift space
• Unbiased cosmology inference from biased tracers using the EFT likelihood
• Marked correlation functions in perturbation theory
• The EFT likelihood for large-scale structure
• A Lagrangian perturbation theory in the presence of massive neutrinos

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