Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
DOI10.1088/1475-7516/2021/05/069zbMath1485.85022arXiv2012.04637OpenAlexW3111826008MaRDI QIDQ5028156
Alexandre Barreira, Rodrigo Voivodic
Publication date: 8 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2012.04637
Classification and discrimination; cluster analysis (statistical aspects) (62H30) Relativistic cosmology (83F05) Gas dynamics (general theory) (76N15) Signal detection and filtering (aspects of stochastic processes) (60G35) Geometrodynamics and the holographic principle (83E05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Traveling wave solutions (35C07) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)
Related Items (2)
Uses Software
Cites Work
- Halo models of large scale structure
- Large-scale structure of the universe and cosmological perturbation theory
- Large-scale galaxy bias
- Natural Selection of Inflationary Vacuum Required by Infra-Red Regularity and Gauge-Invariance
- Responses in large-scale structure
- Cosmological simulation in tides: power spectra, halo shape responses, and shape assembly bias
- Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
- On the impact of galaxy bias uncertainties on primordial non-Gaussianity constraints
- Primordial non-Gaussianity from biased tracers: likelihood analysis of real-space power spectrum and bispectrum
- The Halo Void (Dust) Model of large scale structure
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