Dark energy and modified gravity in the Effective Field Theory of Large-Scale Structure
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Publication:5022297
DOI10.1088/1475-7516/2018/04/005OpenAlexW3104093341WikidataQ130036415 ScholiaQ130036415MaRDI QIDQ5022297
Giulia Cusin, Matthew Lewandowski, Filippo Vernizzi
Publication date: 18 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1712.02783
Related Items (10)
Evolution of dark matter velocity dispersion ⋮ The large scale structure bootstrap: perturbation theory and bias expansion from symmetries ⋮ Baryonic effects in the Effective Field Theory of Large-Scale Structure and an analytic recipe for lensing in CMB-S4 ⋮ k-evolution: a relativistic N-body code for clustering dark energy ⋮ Violation of the consistency relations for large-scale structure with dark energy ⋮ Constraints on modified gravity from the BOSS galaxy survey ⋮ Hi-COLA: fast, approximate simulations of structure formation in Horndeski gravity ⋮ 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 ⋮ Gravitational wave decay into dark energy
Uses Software
Cites Work
- Starting the universe: stable violation of the null energy condition and non-standard cosmologies
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- The matter power spectrum in redshift space using effective field theory
- Weakening gravity on redshift-survey scales with kinetic matter mixing
- An effective description of dark matter and dark energy in the mildly non-linear regime
- A unifying description of dark energy
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