Modeling relativistic contributions to the halo power spectrum dipole

DOI10.1088/1475-7516/2020/07/048zbMath1492.83018arXiv2004.08014OpenAlexW3098296683MaRDI QIDQ5070288

Enea Di Dio, Florian Beutler

Publication date: 11 April 2022

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

Full work available at URL: https://arxiv.org/abs/2004.08014

zbMATH Keywords

power spectrumcosmological simulationsredshift surveyscosmological parameters from LSS

Mathematics Subject Classification ID

Signal detection and filtering (aspects of stochastic processes) (60G35) Diffraction, scattering (78A45) Spectrum, resolvent (47A10) Electromagnetic fields in general relativity and gravitational theory (83C50) Galactic and stellar structure (85A15) (n)-body problems (70F10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Dark matter and dark energy (83C56) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (5)

Testing the equivalence principle on cosmological scales using the odd multipoles of galaxy cross-power spectrum and bispectrum ⋮ The relativistic galaxy number counts in the weak field approximation ⋮ Hybrid-basis inference for large-scale galaxy clustering: combining spherical and Cartesian Fourier analyses ⋮ Wide-angle effects in multi-tracer power spectra with Doppler corrections ⋮ BiGONLight: light propagation with bilocal operators in numerical relativity

Cites Work

• Large-scale galaxy bias
• Isolating relativistic effects in large-scale structure
• Testing the equivalence principle on cosmological scales
• Integral constraints in spectroscopic surveys
• The relativistic dipole and gravitational redshift on LSS

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