Cosmological simulation in tides: power spectra, halo shape responses, and shape assembly bias

DOI10.1088/1475-7516/2021/04/041zbMath1485.83109arXiv2011.06584OpenAlexW3153403168MaRDI QIDQ5026123

Yin Li, Kazuyuki Akitsu, Teppei Okumura

Publication date: 7 February 2022

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

Full work available at URL: https://arxiv.org/abs/2011.06584

zbMATH Keywords

power spectrumcosmological simulationscosmic webdark matter simulations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Perturbations in context of PDEs (35B20) Dark matter and dark energy (83C56) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (4)

Lagrangian approach to super-sample effects on biased tracers at field level: galaxy density fields and intrinsic alignments ⋮ Quadratic shape biases in three-dimensional halo intrinsic alignments ⋮ Synchronizing the consistency relation ⋮ Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias

Uses Software

• TreePM
• CLASS

Cites Work

• Complete super-sample lensing covariance in the response approach
• Galaxy imaging surveys as spin-sensitive detector for cosmological colliders

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