Clustering in massive neutrino cosmologies via Eulerian Perturbation Theory

DOI10.1088/1475-7516/2021/11/028zbMath1487.83050arXiv2106.13771OpenAlexW3175572355MaRDI QIDQ5062288

Zachary Slepian, Arka Banerjee, Alejandro Aviles, Gustavo Niz

Publication date: 15 March 2022

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

Full work available at URL: https://arxiv.org/abs/2106.13771

zbMATH Keywords

power spectrumdark matter theorycosmological neutrinos

Mathematics Subject Classification ID

Classification and discrimination; cluster analysis (statistical aspects) (62H30) Diffraction, scattering (78A45) Spectrum, resolvent (47A10) Quantum field theory on curved space or space-time backgrounds (81T20) Electromagnetic fields in general relativity and gravitational theory (83C50) Perturbations in context of PDEs (35B20) Weak interaction in quantum theory (81V15) Dark matter and dark energy (83C56) Effective quantum field theories (81T12) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)

Related Items (3)

Constraints on modified gravity from the BOSS galaxy survey ⋮ Neutrino mass and kinetic gravity braiding degeneracies ⋮ Fast computation of non-linear power spectrum in cosmologies with massive neutrinos

Uses Software

• emcee
• GetDist
• CONCEPT
• Quijote
• FAST-PT
• CAMB

Cites Work

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