General relativistic effects in the galaxy bias at second order
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Publication:5862940
DOI10.1088/1475-7516/2019/05/020zbMath1481.83121arXiv1901.07460OpenAlexW3103246984WikidataQ64297314 ScholiaQ64297314MaRDI QIDQ5862940
Chris Clarkson, Fabian Schmidt, Roy Maartens, Kazuya Koyama, Obinna Umeh
Publication date: 10 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1901.07460
Related Items (12)
The spatial gauge-dependence of single-field inflationary bispectra ⋮ Contributions from primordial non-Gaussianity and general relativity to the galaxy power spectrum ⋮ The galaxy bias at second order in general relativity with non-Gaussian initial conditions ⋮ Relativistic and non-Gaussianity contributions to the one-loop power spectrum ⋮ Multipoles of the relativistic galaxy bispectrum ⋮ 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 ⋮ Non-Gaussianity in the squeezed three-point correlation from the relativistic effects ⋮ Resilience of long modes in cosmological observables ⋮ Relativistic cosmological large scale structures at one-loop ⋮ Local primordial non-Gaussianity in the relativistic galaxy bispectrum ⋮ Optimal computation of anisotropic galaxy three point correlation function multipoles using 2DFFTLOG formalism
Uses Software
Cites Work
- Topology and cosmology
- Relativistic hydrodynamic cosmological perturbations
- Large-scale structure of the universe and cosmological perturbation theory
- Large-scale galaxy bias
- Symmetries and consistency relations in the large scale structure of the universe
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- Galaxy bias and gauges at second order in general relativity
- Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond
- General relativistic weak-field limit and Newtonian N-body simulations
- How Gaussian can our Universe be?
- Large-scale tides in general relativity
- A relativistic interpretation of bias in Newtonian simulations
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