Full-sky bispectrum in redshift space for 21cm intensity maps
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Publication:5027064
DOI10.1088/1475-7516/2020/12/003zbMath1484.83108arXiv2008.02266OpenAlexW3047538035MaRDI QIDQ5027064
Roy Maartens, Francesco Montanari, Rahul Kothari, Ruth Durrer, Mona Jalilvand
Publication date: 3 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2008.02266
Relativistic cosmology (83F05) Diffraction, scattering (78A45) Atomic physics (81V45) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)
Related Items (4)
An estimator for the lensing potential from galaxy number counts ⋮ Testing general relativity with cosmological large scale structure ⋮ Local primordial non-Gaussianity in the relativistic galaxy bispectrum ⋮ Detecting the relativistic bispectrum in 21cm intensity maps
Cites Work
- Large-scale structure of the universe and cosmological perturbation theory
- Large-scale galaxy bias
- Imprints of local lightcone \ projection effects on the galaxy bispectrum. Part II
- Imprints of local lightcone projection effects on the galaxy bispectrum. Part III. Relativistic corrections from nonlinear dynamical evolution on large-scales
- Non-Gaussianities due to relativistic corrections to the observed galaxy bispectrum
- Higher order relativistic galaxy number counts: dominating terms
- A general relativistic signature in the galaxy bispectrum: the local effects of observing on the lightcone
- Detecting the relativistic galaxy bispectrum
- Multipoles of the relativistic galaxy bispectrum
- Imprints of local lightcone projection effects on the galaxy bispectrum IV: second-order vector and tensor contributions
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