On observables in a dark matter-clustering quintessence system

DOI10.1088/1475-7516/2019/05/033zbMath1481.83081arXiv1611.00542OpenAlexW2547292715WikidataQ64297242 ScholiaQ64297242MaRDI QIDQ5862951

Matteo Fasiello, Zvonimir Vlah

Publication date: 10 March 2022

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

Full work available at URL: https://arxiv.org/abs/1611.00542

zbMATH Keywords

power spectrummodified gravitydark energy theory

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (2)

Self-interacting dark matter in cosmology: accurate numerical implementation and observational constraints ⋮ Perturbative description of biased tracers using consistency relations of LSS

Uses Software

• CAMB
• CLASS

Cites Work

• Unnamed Item
• Consequences of symmetries and consistency relations in the large-scale structure of the universe for non-local bias and modified gravity
• Large-scale structure of the universe and cosmological perturbation theory
• The effective field theory of cosmological large scale structures
• Symmetries and consistency relations in the large scale structure of the universe
• High energy physics signatures from inflation and conformal symmetry of de Sitter
• An introduction to the Vainshtein mechanism
• CLASS

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