eprintid: 10194624
rev_number: 9
eprint_status: archive
userid: 699
dir: disk0/10/19/46/24
datestamp: 2024-07-16 14:07:04
lastmod: 2024-07-16 14:07:04
status_changed: 2024-07-16 14:07:04
type: article
metadata_visibility: show
sword_depositor: 699
creators_name: Bohmer, Christian G
creators_name: del Sordo, Antonio d'Alfonso
title: Cosmological fluids with boundary term couplings
ispublished: pub
divisions: UCL
divisions: B04
divisions: C06
divisions: F59
note: This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
abstract: Cosmological models can be studied effectively using dynamical systems techniques. Starting from Brown’s formulation of the variational principle for relativistic fluids, we introduce new types of couplings involving a perfect fluid, a scalar field, and boundary terms. We describe three different coupling models, one of which turns out to be particularly relevant for cosmology. Its behaviour is similar to that of models in which dark matter decays into dark energy. In particular, for a constant coupling, the model mimics well-known dynamical dark energy models while the non-constant couplings offer a rich dynamical structure, unseen before. We are able to achieve this richness whilst working in a two-dimensional phase space. This is a significant advantage which allows us to provide a clear physical interpretation of the key features and draw analogies with previously studied models.
date: 2024-06-18
date_type: published
publisher: SPRINGER/PLENUM PUBLISHERS
official_url: http://dx.doi.org/10.1007/s10714-024-03260-6
oa_status: green
full_text_type: pub
language: eng
primo: open
primo_central: open_green
verified: verified_manual
elements_id: 2290788
doi: 10.1007/s10714-024-03260-6
lyricists_name: Boehmer, Christian
lyricists_id: CGBOH42
actors_name: Boehmer, Christian
actors_id: CGBOH42
actors_role: owner
funding_acknowledgements: EP/R513143/1 [Engineering and Physical Sciences Research Council]; EP/T517793/1 [Engineering and Physical Sciences Research Council]; [Engineering and Physical Sciences Research Council]
full_text_status: public
publication: General Relativity and Gravitation
volume: 56
article_number: 75
pages: 33
issn: 0001-7701
citation:        Bohmer, Christian G;    del Sordo, Antonio d'Alfonso;      (2024)    Cosmological fluids with boundary term couplings.                   General Relativity and Gravitation , 56     , Article 75.  10.1007/s10714-024-03260-6 <https://doi.org/10.1007/s10714-024-03260-6>.       Green open access   
 
document_url: https://discovery.ucl.ac.uk/id/eprint/10194624/1/Boehmer_s10714-024-03260-6.pdf