Non-perturbative probability distribution function for cosmological counts in cells

DOI10.1088/1475-7516/2019/03/009OpenAlexW2900951425WikidataQ128282709 ScholiaQ128282709MaRDI QIDQ5862111

Alexander A. Kaurov, Mikhail M. Ivanov, Sergey Sibiryakov

Publication date: 4 March 2022

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

Full work available at URL: https://arxiv.org/abs/1811.07913

zbMATH Keywords

power spectrumcosmic webcluster countsdark matter simulations

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (3)

AsPy ⋮ On the statistical evolution of the large-scale structure and the effective dynamics ⋮ Non-Gaussian CMB and LSS statistics beyond polyspectra

Uses Software

• DLMF
• GitHub
• FastPM
• nbodykit
• CLASS

Cites Work

• Unnamed Item
• Large-scale structure of the universe and cosmological perturbation theory
• The effective field theory of cosmological large scale structures
• NIST digital library of mathematical functions
• Symmetries and consistency relations in the large scale structure of the universe
• Dynamics of gravitational clustering
• Dynamics of gravitational clustering
• Divergence of perturbation theory in large scale structures
• CLASS

This page was built for publication: Non-perturbative probability distribution function for cosmological counts in cells