Cosmological Properties of the Cosmic Web
Author:
Affiliation:
1. Laboratory of Universe and Theories Observatoire de Paris, PSL research University, CNRS, 5 Place Jules Janssen, F-92190 Paris, France
Publisher
MDPI
Link
https://www.mdpi.com/2673-9984/7/1/53/pdf
Reference11 articles.
1. Imprints of dark energy on cosmic structure formation—I. Realistic quintessence models and the non-linear matter power spectrum;Alimi;Mon. Not. R. Astron. Soc.,2010
2. Cosmology with cosmic web environments;Bonnaire;Astron. Astrophys.,2022
3. Extracting cosmological parameters from N-body simulations using machine learning techniques;Lazanu;J. Cosmol. Astropart. Phy.,2021
4. Erwan Allys The quijote simulations;Hahn;Astrophys. J. Suppl. Ser.,2020
5. Alimi, J.-M., and Shalak, M. (2023). Pearson distribution as a phenomenological approach of non-linear cosmic matter field statistics, in preparation.
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1. Cosmological Properties of the Cosmic Web;The 2nd Electronic Conference on Universe;2023-02-16
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