Responses in large-scale structure

DOI10.1088/1475-7516/2017/06/053OpenAlexW2601683864MaRDI QIDQ5024225

Fabian Schmidt, Alexandre Barreira

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/1703.09212

zbMATH Keywords

power spectrumcosmological parameters from LSSdark energy experiments

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (6)

Cosmological angular trispectra and non-Gaussian covariance ⋮ Large-scale galaxy bias ⋮ Local Primordial Non-Gaussianities and super-sample variance ⋮ The squeezed matter bispectrum covariance with responses ⋮ Complete super-sample lensing covariance in the response approach ⋮ Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias

Uses Software

• CAMB

Cites Work

• The effective field theorist's approach to gravitational dynamics
• Halo models of large scale structure
• Consequences of symmetries and consistency relations in the large-scale structure of the universe for non-local bias and modified gravity
• Large-scale structure of the universe and cosmological perturbation theory
• The effective field theory of cosmological large scale structures
• Symmetries and consistency relations in the large scale structure of the universe
• Equal-time consistency relations in the large-scale structure of the universe

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