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Relativistic interacting fluids in cosmology

Iosifidis, D; Jensko, E; Koivisto, TS; (2024) Relativistic interacting fluids in cosmology. Journal of Cosmology and Astroparticle Physics , 2024 (11) , Article 043. 10.1088/1475-7516/2024/11/043. Green open access

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Abstract

Motivated by cosmological applications for interacting matters, an extension of the action functional for relativistic fluids is proposed to incorporate the physics of non-adiabatic processes and chemical reactions. The former are characterised by entropy growth, while the latter violate particle number conservation. The relevance of these physics is demonstrated in the contexts of self-interacting fluids, fluids interacting with scalar fields, and hyperhydrodynamical interactions with geometry. The possible cosmological applications range from early-universe phase transitions to astrophysical phenomena, and from matter creation inflationary alternatives to interacting dark sector alternatives to the ΛCDM model that aim to address its tensions. As an example of the latter, a single fluid model of a unified dark sector is presented. The simple action of the model features one field and one parameter, yet it can both reproduce the ΛCDM cosmology and predict new phenomenology.

Type: Article
Title: Relativistic interacting fluids in cosmology
Open access status: An open access version is available from UCL Discovery
DOI: 10.1088/1475-7516/2024/11/043
Publisher version: https://doi.org/10.1088/1475-7516/2024/11/043
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Mathematics
URI: https://discovery.ucl.ac.uk/id/eprint/10204196
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