Analyzing clustering of astrophysical gravitational-wave sources: luminosity-distance space distortions

DOI10.1088/1475-7516/2021/01/036zbMath1484.85020arXiv2007.04359OpenAlexW3041420301MaRDI QIDQ5025283

Toshiya Namikawa

Publication date: 1 February 2022

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

Full work available at URL: https://arxiv.org/abs/2007.04359

zbMATH Keywords

power spectrumgalaxy clusteringredshift surveysgravitational waves/sources

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Galactic and stellar structure (85A15) Gravitational waves (83C35) Cluster sets, prime ends, boundary behavior (30D40) Rate-distortion theory in information and communication theory (94A34) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)

Related Items (1)

The observed number counts in luminosity distance space

Uses Software

• CAMB

Cites Work

• Weak gravitational lensing
• Anisotropies of gravitational wave backgrounds: a line of sight approach
• Mapping the gravitational-wave background
• Relativistic effect in galaxy clustering
• Cosmography with the Einstein Telescope
• The magnitude–redshift relation in a perturbed Friedmann universe

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