General relativistic corrections and non-Gaussianity in large-scale structure

DOI10.1088/0264-9381/31/23/234005zbMath1306.83070arXiv1409.4738OpenAlexW2037848073WikidataQ60871948 ScholiaQ60871948MaRDI QIDQ2936167

Sabino Matarrese, Eleonora Villa, Licia Verde

Publication date: 5 January 2015

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1409.4738

zbMATH Keywords

relativistic correctionslensingcosmic microwave backgroundrelativistic cosmologyhigher-order cosmological perturbationsmatter clusteringprimary anisotropies

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of statistics to physics (62P35) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (6)

Galaxy power spectrum in general relativity ⋮ Large-scale galaxy bias ⋮ Relativistic second-order initial conditions for simulations of large-scale structure ⋮ Non-Gaussianity in the squeezed three-point correlation from the relativistic effects ⋮ Non-Gaussianities due to relativistic corrections to the observed galaxy bispectrum ⋮ Resilience of long modes in cosmological observables

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