Baryonic effects in the Effective Field Theory of Large-Scale Structure and an analytic recipe for lensing in CMB-S4

DOI10.1088/1475-7516/2021/10/074zbMath1487.85011arXiv2010.02929OpenAlexW3209929798MaRDI QIDQ5061945

Raphael Sgier, Matthew Lewandowski, David Sekera, Leonardo Senatore, Diogo P. L. Bragança

Publication date: 14 March 2022

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

Full work available at URL: https://arxiv.org/abs/2010.02929

zbMATH Keywords

power spectrumgalaxy clusteringcosmological parameters from LSSbaryon acoustic oscillations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Nuclear physics (81V35) Diffraction, scattering (78A45) Spectrum, resolvent (47A10) Quantum field theory on curved space or space-time backgrounds (81T20) Hydro- and aero-acoustics (76Q05) Electromagnetic fields in general relativity and gravitational theory (83C50) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Perturbations in context of PDEs (35B20) Galactic and stellar structure (85A15) Cluster algebras (13F60) Liquid-liquid two component flows (76T06) Dark matter and dark energy (83C56) Effective quantum field theories (81T12)

Related Items (1)

Efficiently evaluating loop integrals in the EFTofLSS using QFT integrals with massive propagators

Uses Software

• EuclidEmulator

Cites Work

• On loops in inflation
• Large-scale structure of the universe and cosmological perturbation theory
• The effective field theory of cosmological large scale structures
• Dissipative effects in the effective field theory of inflation
• Symmetries and consistency relations in the large scale structure of the universe
• Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
• The matter power spectrum in redshift space using effective field theory
• Dark energy and modified gravity in the Effective Field Theory of Large-Scale Structure
• An effective description of dark matter and dark energy in the mildly non-linear regime
• Very massive tracers and higher derivative biases
• Violation of the consistency relations for large-scale structure with dark energy
• A unifying description of dark energy

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