The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model

We present a dark fluid model described as a non-viscous, non-relativistic, rotating, and self-gravitating fluid. We assume that the system has spherical symmetry and that the matter can be described by the polytropic equation of state. The induced coupled nonlinear partial differential system of eq...

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Main Authors: Balázs Endre Szigeti, Imre Ferenc Barna, Gergely Gábor Barnaföldi
Format: Article
Language:English
Published: MDPI AG 2023-09-01
Series:Universe
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Online Access:https://www.mdpi.com/2218-1997/9/10/431
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author Balázs Endre Szigeti
Imre Ferenc Barna
Gergely Gábor Barnaföldi
author_facet Balázs Endre Szigeti
Imre Ferenc Barna
Gergely Gábor Barnaföldi
author_sort Balázs Endre Szigeti
collection DOAJ
description We present a dark fluid model described as a non-viscous, non-relativistic, rotating, and self-gravitating fluid. We assume that the system has spherical symmetry and that the matter can be described by the polytropic equation of state. The induced coupled nonlinear partial differential system of equations was solved using a self-similar time-dependent ansatz introduced by L. Sedov and G.I. Taylor. These kinds of solutions were successfully used to describe blast waves induced by an explosion following the Guderley–Landau–Stanyukovich problem. We show that the result of our quasi-analytic solutions are fully consistent with the Newtonian cosmological framework. We analyzed relevant quantities from the model, namely, the evolution of the Hubble parameter and the density parameter ratio, finding that our solutions can be applied to describe normal-to-dark energy on the cosmological scale.
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spelling doaj.art-09a1a938ad16474abc632de8d3627b162023-11-19T18:23:20ZengMDPI AGUniverse2218-19972023-09-0191043110.3390/universe9100431The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid ModelBalázs Endre Szigeti0Imre Ferenc Barna1Gergely Gábor Barnaföldi2Wigner Research Centre for Physics, Institute for Particle and Nuclear Physics, 1121 Budapest, HungaryWigner Research Centre for Physics, Institute for Particle and Nuclear Physics, 1121 Budapest, HungaryWigner Research Centre for Physics, Institute for Particle and Nuclear Physics, 1121 Budapest, HungaryWe present a dark fluid model described as a non-viscous, non-relativistic, rotating, and self-gravitating fluid. We assume that the system has spherical symmetry and that the matter can be described by the polytropic equation of state. The induced coupled nonlinear partial differential system of equations was solved using a self-similar time-dependent ansatz introduced by L. Sedov and G.I. Taylor. These kinds of solutions were successfully used to describe blast waves induced by an explosion following the Guderley–Landau–Stanyukovich problem. We show that the result of our quasi-analytic solutions are fully consistent with the Newtonian cosmological framework. We analyzed relevant quantities from the model, namely, the evolution of the Hubble parameter and the density parameter ratio, finding that our solutions can be applied to describe normal-to-dark energy on the cosmological scale.https://www.mdpi.com/2218-1997/9/10/431dark fluidSedov–Taylor Ansatzself-similarity
spellingShingle Balázs Endre Szigeti
Imre Ferenc Barna
Gergely Gábor Barnaföldi
The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model
Universe
dark fluid
Sedov–Taylor Ansatz
self-similarity
title The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model
title_full The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model
title_fullStr The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model
title_full_unstemmed The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model
title_short The Formulation of Scaling Expansion in an Euler-Poisson Dark-Fluid Model
title_sort formulation of scaling expansion in an euler poisson dark fluid model
topic dark fluid
Sedov–Taylor Ansatz
self-similarity
url https://www.mdpi.com/2218-1997/9/10/431
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