Assessing the foundation and applicability of some dark energy fluid models in the Dirac-Born-Infeld framework
Muhsin Aljaf, Daniele Gregoris, Martiros Khurshudyan

TL;DR
This paper investigates dark energy fluid models within the Dirac-Born-Infeld framework, analyzing their theoretical foundations, cosmological implications, and limitations in explaining galactic rotation curves, using both analytical and machine learning methods.
Contribution
It establishes the hydrodynamic realization of the Modified Berthelot fluid in the Dirac-Born-Infeld theory and explores the non-relativistic formulation of the Dieterici fluid, including their cosmological and galactic implications.
Findings
Modified Berthelot fluid corresponds to Dirac-Born-Infeld theory.
Dieterici fluid admits a non-relativistic k-essence formulation.
Dirac-Born-Infeld theory cannot explain flat galactic rotation curves.
Abstract
In this paper, we will deepen the understanding of some fluid models proposed by other authors for the description of dark energy. Specifically, we will show that the so-called (Modified) Berthelot fluid is the hydrodynamic realization of the free Dirac-Born-Infeld theory and that the Dieterici fluid admits a non-relativistic -essence formulation; for the former model the evolution of the scalar field will be written in terms of some cosmographic parameters. The latter model will also be tested using Machine Learning algorithms with respect to cosmic chronometers data, and results about the dynamics at a background level will be compared with those arising when other fluids (Generalized Chaplygin Gas and Anton-Schmidt) are considered. Due to some cosmic opacity effects, the background cosmology of universes filled by these inequivalent fluids, as they arise in physically different…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Computational Physics and Python Applications
