Testing effective dark energy models in gravitationally bound systems: The case of Non-local Gravity

Bouchè, F. (2024) Testing effective dark energy models in gravitationally bound systems: The case of Non-local Gravity. Il nuovo cimento C, 47 (3). pp. 1-6. ISSN 1826-9885

[img]
Preview
Text
ncc12912.pdf - Published Version

Download (143kB) | Preview
Official URL: https://www.sif.it/riviste/sif/ncc/econtents/2024/...

Abstract

The forthcoming generation of astrophysical and cosmological sur- veys are expected to generate an extensive and groundbreaking collection of data. The unmatched quantity and quality of these observations should boost our knowl- edge of the Universe, especially in regards to the dark sector. The true nature of the dark energy, either gravitational or related to fundamental fields, may therefore be unveiled in the next decades. Within this framework, the following contribution investigates the viability of a dark energy model based upon Non-local Gravity. The main cosmological features of the model are presented, and the impact of non-locality within the non-linear regime is analysed through astrophysical tests.

Item Type: Article
Subjects: 500 Scienze naturali e Matematica > 530 Fisica
Depositing User: Marina Spanti
Date Deposited: 07 Jun 2024 14:07
Last Modified: 07 Jun 2024 14:07
URI: http://eprints.bice.rm.cnr.it/id/eprint/22944

Actions (login required)

View Item View Item