An effective description of dark matter and dark energy in the mildly non-linear regime
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Publication:5024301
DOI10.1088/1475-7516/2017/05/038OpenAlexW3101828977MaRDI QIDQ5024301
Azadeh Maleknejad, Matthew Lewandowski, Leonardo Senatore
Publication date: 28 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1611.07966
Related Items (10)
Evolution of dark matter velocity dispersion ⋮ Baryonic effects in the Effective Field Theory of Large-Scale Structure and an analytic recipe for lensing in CMB-S4 ⋮ An analytic implementation of the IR-resummation for the BAO peak ⋮ Violation of the consistency relations for large-scale structure with dark energy ⋮ Large-scale galaxy bias ⋮ Biased tracers in redshift space in the EFTofLSS with exact time dependence ⋮ Constraints on modified gravity from the BOSS galaxy survey ⋮ Efficiently evaluating loop integrals in the EFTofLSS using QFT integrals with massive propagators ⋮ Tree-level bispectrum in the effective field theory of large-scale structure extended to massive neutrinos ⋮ Dark energy and modified gravity in the Effective Field Theory of Large-Scale Structure
Uses Software
Cites Work
- Starting the universe: stable violation of the null energy condition and non-standard cosmologies
- The effective field theory of cosmological large scale structures
- Dissipative effects in the effective field theory of inflation
- Cosmological parameters from SDSS and WMAP
- A unifying description of dark energy
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- A Relativist's Toolkit
- General Relativity
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