Non-Gaussianity in the squeezed three-point correlation from the relativistic effects
DOI10.1088/1475-7516/2022/08/050OpenAlexW4292774547MaRDI QIDQ5101160
Jaiyul Yoo, Nastassia Grimm, Ermis Mitsou
Publication date: 2 September 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2204.03002
Measures of association (correlation, canonical correlation, etc.) (62H20) Point estimation (62F10) Relativistic cosmology (83F05) Dilations, extensions, compressions of linear operators (47A20) Perturbations in context of PDEs (35B20) Galactic and stellar structure (85A15) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15) Set functions and measures and integrals in infinite-dimensional spaces (Wiener measure, Gaussian measure, etc.) (28C20) Cluster sets, prime ends, boundary behavior (30D40)
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Cites Work
- Unnamed Item
- Large-scale structure of the universe and cosmological perturbation theory
- Large-scale galaxy bias
- The spatial gauge-dependence of single-field inflationary bispectra
- Relativistic effects and primordial non-Gaussianity in the matter density fluctuation
- Symmetries and consistency relations in the large scale structure of the universe
- Republication of: Perturbations of a cosmological model and angular variations of the microwave background. Edited and with commentary by George Ellis and with notes on Sachs-Wolfe integration by Jürgen Ehlers. With brief autobiographies by Sachs and Wolfe.
- Relativistic effect in galaxy clustering
- General relativistic corrections and non-Gaussianity in large-scale structure
- Can the acceleration of our universe be explained by the effects of inhomogeneities?
- Galaxy bias and gauges at second order in general relativity
- Observables and gauge invariance in the theory of nonlinear spacetime perturbations
- Tetrad Formalism for Exact Cosmological Observables
- Gauge-transformation properties of cosmological observables and its application to the light-cone average
- Imprints of local lightcone \ projection effects on the galaxy bispectrum. Part II
- Gauge-invariant formalism of cosmological weak lensing
- Galaxy two-point correlation function in general relativity
- How Gaussian can our Universe be?
- Non-Gaussianities due to relativistic corrections to the observed galaxy bispectrum
- A general relativistic signature in the galaxy bispectrum: the local effects of observing on the lightcone
- Resilience of long modes in cosmological observables
- Local primordial non-Gaussianity in the relativistic galaxy bispectrum
- Galaxy power spectrum in general relativity
- Second-order gauge-invariant formalism for the cosmological observables: complete verification of their gauge-invariance
- Large gauge transformations, local coordinates and cosmological observables
- Cosmological information contents on the light-cone
- The galaxy bias at second order in general relativity with non-Gaussian initial conditions
- An EFT description of galaxy intrinsic alignments
- Inflationary soft theorems revisited: a generalized consistency relation
- A rigorous EFT-based forward model for large-scale structure
- General relativistic effects in the galaxy bias at second order
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