Imprints of local lightcone projection effects on the galaxy bispectrum. Part III. Relativistic corrections from nonlinear dynamical evolution on large-scales
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Publication:5022254
DOI10.1088/1475-7516/2018/03/036OpenAlexW3098457229WikidataQ63390602 ScholiaQ63390602MaRDI QIDQ5022254
Roy Maartens, Chris Clarkson, Obinna Umeh, Sheean Jolicoeur
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/1711.01812
Related Items (9)
The galaxy bias at second order in general relativity with non-Gaussian initial conditions ⋮ General relativistic cosmological N-body simulations. Part I. Time integration ⋮ Multi-scale perturbation theory. Part I. Methodology and leading-order bispectrum corrections in the matter-dominated era ⋮ Multipoles of the relativistic galaxy bispectrum ⋮ Reduced phase space optics for general relativity: symplectic ray bundle transfer ⋮ Imprints of local lightcone projection effects on the galaxy bispectrum IV: second-order vector and tensor contributions ⋮ Local primordial non-Gaussianity in the relativistic galaxy bispectrum ⋮ Full-sky bispectrum in redshift space for 21cm intensity maps ⋮ Detecting the relativistic bispectrum in 21cm intensity maps
Cites Work
- Large-scale structure of the universe and cosmological perturbation theory
- Observed galaxy number counts on the light cone up to second order: III. Magnification bias
- Imprints of local lightcone \ projection effects on the galaxy bispectrum. Part II
- 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
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