GALACTIC ANGULAR MOMENTA AND ANGULAR MOMENTUM CORRELATIONS IN THE COSMOLOGICAL LARGE-SCALE STRUCTURE

DOI10.1142/S0218271809014388zbMath1173.85002arXiv0808.0203OpenAlexW2125732909MaRDI QIDQ3636470

Björn Malte Schäfer

Publication date: 30 June 2009

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0808.0203

zbMATH Keywords

cosmologygravitational lensinglarge-scale structure

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Equations of motion in general relativity and gravitational theory (83C10) Astrophysical cosmology (85A40) Research exposition (monographs, survey articles) pertaining to astronomy and astrophysics (85-02)

Related Items (3)

Field-level inference of galaxy intrinsic alignment from the SDSS-III BOSS survey ⋮ The intrinsic alignment of galaxies and its impact on weak gravitational lensing in an era of precision cosmology ⋮ Environmental dependence of ellipticity correlation functions of intrinsic alignments

Cites Work

• Unnamed Item
• Newtonian cosmology in Lagrangian formulation: Foundations and perturbation theory
• Weak gravitational lensing
• Large-scale structure of the universe and cosmological perturbation theory
• A class of solutions for self-gravitating dust in Newtonian gravity
• Dynamical Friction. I. General Considerations: the Coefficient of Dynamical Friction.

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