The relativistic galaxy number counts in the weak field approximation

DOI10.1088/1475-7516/2020/09/058zbMath1493.85004arXiv2004.07916OpenAlexW3103220611MaRDI QIDQ5070965

Enea Di Dio, Florian Beutler

Publication date: 14 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2004.07916

zbMATH Keywords

power spectrumcosmological perturbation theorygalaxy clusteringredshift surveys

Mathematics Subject Classification ID

Measures of association (correlation, canonical correlation, etc.) (62H20) Relativistic cosmology (83F05) Diffraction, scattering (78A45) Spectrum, resolvent (47A10) Symmetry breaking in quantum theory (81R40) Electromagnetic fields in general relativity and gravitational theory (83C50) Perturbations in context of PDEs (35B20) Galactic and stellar structure (85A15) Cluster sets, prime ends, boundary behavior (30D40)

Related Items (4)

Testing the equivalence principle on cosmological scales using the odd multipoles of galaxy cross-power spectrum and bispectrum ⋮ From matter to galaxies: general relativistic bias for the one-loop bispectrum ⋮ Wide-angle effects in multi-tracer power spectra with Doppler corrections ⋮ The observed galaxy power spectrum in General Relativity

Cites Work

• Weak gravitational lensing
• Lensing and time-delay contributions to galaxy correlations
• General relativistic weak-field limit and Newtonian N-body simulations
• Testing the equivalence principle on cosmological scales
• Lensing smoothing of BAO wiggles
• Relativistic cosmological large scale structures at one-loop
• Detecting the relativistic galaxy bispectrum
• Modeling relativistic contributions to the halo power spectrum dipole
• The relativistic dipole and gravitational redshift on LSS

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