Cosmic Evolution of Viscous QCD Epoch in Causal Eckart Frame
It is conjectured that in cosmological applications the particle current is not modified but finite heat or energy flow. Therefore, comoving Eckart frame is a suitable choice, as it merely ceases the charge and particle diffusion and conserves charges and particles. The cosmic evolution of viscous h...
Main Authors: | , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-04-01
|
Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/7/5/112 |
id |
doaj-b8cd9d21f082444b875fb8215076cce2 |
---|---|
record_format |
Article |
spelling |
doaj-b8cd9d21f082444b875fb8215076cce22021-04-21T23:00:30ZengMDPI AGUniverse2218-19972021-04-01711211210.3390/universe7050112Cosmic Evolution of Viscous QCD Epoch in Causal Eckart FrameEman Abdel Hakk0Abdel Nasser Tawfik1Afaf Nada2Hayam Yassin3Physics Department, Faculty of Women for Arts, Science and Education, Ain Shams University, Cairo 11577, EgyptEgyptian Center for Theoretical Physics (ECTP), Juhayna Square of 26th-July-Corridor, Giza 12588, EgyptPhysics Department, Faculty of Women for Arts, Science and Education, Ain Shams University, Cairo 11577, EgyptPhysics Department, Faculty of Women for Arts, Science and Education, Ain Shams University, Cairo 11577, EgyptIt is conjectured that in cosmological applications the particle current is not modified but finite heat or energy flow. Therefore, comoving Eckart frame is a suitable choice, as it merely ceases the charge and particle diffusion and conserves charges and particles. The cosmic evolution of viscous hadron and parton epochs in casual and non-casual Eckart frame is analyzed. By proposing equations of state deduced from recent lattice QCD simulations including pressure <i>p</i>, energy density <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>ρ</mi></semantics></math></inline-formula>, and temperature <i>T</i>, the Friedmann equations are solved. We introduce expressions for the temporal evolution of the Hubble parameter <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>H</mi><mo>˙</mo></mover></semantics></math></inline-formula>, the cosmic energy density <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>ρ</mi><mo>˙</mo></mover></semantics></math></inline-formula>, and the share <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>η</mi><mo>˙</mo></mover></semantics></math></inline-formula> and the bulk viscous coefficient <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>ζ</mi><mo>˙</mo></mover></semantics></math></inline-formula>. We also suggest how the bulk viscous pressure <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Π</mi></semantics></math></inline-formula> could be related to <i>H</i>. We conclude that the relativistic theory of fluids, the Eckart frame, and the finite viscous coefficients play essential roles in the cosmic evolution, especially in the hadron and parton epochs.https://www.mdpi.com/2218-1997/7/5/112observational cosmologymathematical and relativistic aspects of cosmologyquark-gluon plasma |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Eman Abdel Hakk Abdel Nasser Tawfik Afaf Nada Hayam Yassin |
spellingShingle |
Eman Abdel Hakk Abdel Nasser Tawfik Afaf Nada Hayam Yassin Cosmic Evolution of Viscous QCD Epoch in Causal Eckart Frame Universe observational cosmology mathematical and relativistic aspects of cosmology quark-gluon plasma |
author_facet |
Eman Abdel Hakk Abdel Nasser Tawfik Afaf Nada Hayam Yassin |
author_sort |
Eman Abdel Hakk |
title |
Cosmic Evolution of Viscous QCD Epoch in Causal Eckart Frame |
title_short |
Cosmic Evolution of Viscous QCD Epoch in Causal Eckart Frame |
title_full |
Cosmic Evolution of Viscous QCD Epoch in Causal Eckart Frame |
title_fullStr |
Cosmic Evolution of Viscous QCD Epoch in Causal Eckart Frame |
title_full_unstemmed |
Cosmic Evolution of Viscous QCD Epoch in Causal Eckart Frame |
title_sort |
cosmic evolution of viscous qcd epoch in causal eckart frame |
publisher |
MDPI AG |
series |
Universe |
issn |
2218-1997 |
publishDate |
2021-04-01 |
description |
It is conjectured that in cosmological applications the particle current is not modified but finite heat or energy flow. Therefore, comoving Eckart frame is a suitable choice, as it merely ceases the charge and particle diffusion and conserves charges and particles. The cosmic evolution of viscous hadron and parton epochs in casual and non-casual Eckart frame is analyzed. By proposing equations of state deduced from recent lattice QCD simulations including pressure <i>p</i>, energy density <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi>ρ</mi></semantics></math></inline-formula>, and temperature <i>T</i>, the Friedmann equations are solved. We introduce expressions for the temporal evolution of the Hubble parameter <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>H</mi><mo>˙</mo></mover></semantics></math></inline-formula>, the cosmic energy density <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>ρ</mi><mo>˙</mo></mover></semantics></math></inline-formula>, and the share <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>η</mi><mo>˙</mo></mover></semantics></math></inline-formula> and the bulk viscous coefficient <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mover accent="true"><mi>ζ</mi><mo>˙</mo></mover></semantics></math></inline-formula>. We also suggest how the bulk viscous pressure <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Π</mi></semantics></math></inline-formula> could be related to <i>H</i>. We conclude that the relativistic theory of fluids, the Eckart frame, and the finite viscous coefficients play essential roles in the cosmic evolution, especially in the hadron and parton epochs. |
topic |
observational cosmology mathematical and relativistic aspects of cosmology quark-gluon plasma |
url |
https://www.mdpi.com/2218-1997/7/5/112 |
work_keys_str_mv |
AT emanabdelhakk cosmicevolutionofviscousqcdepochincausaleckartframe AT abdelnassertawfik cosmicevolutionofviscousqcdepochincausaleckartframe AT afafnada cosmicevolutionofviscousqcdepochincausaleckartframe AT hayamyassin cosmicevolutionofviscousqcdepochincausaleckartframe |
_version_ |
1721515533553106944 |