On the viability of Planck scale cosmology with quartessence
Abstract Growing evidence as the observations of the CMB (cosmic microwave background), galaxy clustering and high-redshift supernovae address a stable dynamically universe dominated by the dark components. In this paper, using a qualitative theory of dynamical systems, we study the stability of a u...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
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SpringerOpen
2018-09-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-018-6191-4 |
| _version_ | 1828333960432713728 |
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| author | Mohsen Khodadi Kourosh Nozari Fazlollah Hajkarim |
| author_facet | Mohsen Khodadi Kourosh Nozari Fazlollah Hajkarim |
| author_sort | Mohsen Khodadi |
| collection | DOAJ |
| description | Abstract Growing evidence as the observations of the CMB (cosmic microwave background), galaxy clustering and high-redshift supernovae address a stable dynamically universe dominated by the dark components. In this paper, using a qualitative theory of dynamical systems, we study the stability of a unified dark matter-dark energy framework known as quartessence Chaplygin model (QCM) with three different equation-of-states within ultraviolet (UV) deformed Friedmann–Robertson–Walker (FRW) cosmologies without Big-Bang singularity. The UV deformation is inspired by the non-commutative (NC) Snyder spacetime approach in which by keeping the transformation groups and rotational symmetry there is a dimensionless, Planck scale characteristic parameter $$\mu _0$$ μ0 with dual implications dependent on its sign that addresses the required invariant cutoffs for length and momentum in nature, in a separate manner. Our stability analysis is done in the $$(H,\rho )$$ (H,ρ) phase space at a finite domain concerning the hyperbolic critical points. According to our analysis, due to constraints imposed on the signs of $$\mu _0$$ μ0 from the phenomenological parameters involved in quartessence models $$(\Omega _m^*, c_s^2, \rho _*)$$ (Ωm∗,cs2,ρ∗) , for an expanding and accelerating late universe, all three QCMs can be stable in the vicinity of the critical points. The requirement of stability for these quartessence models in case of admission of a minimum invariant length, can yield a flat as well as non-flat expanding and accelerating universe in which Big-Bang singularity is absent. This feedback also phenomenologically credits to braneworld-like framework versus loop quantum cosmology-like one as two possible scenarios which can be NC Snyder spacetime generators (correspond to $$\mu _0<0$$ μ0<0 and $$\mu _0>0$$ μ0>0 , respectively). As a result, our analysis show that between quartessence models with Chaplygin gas equation-of-states and accelerating FRW backgrounds occupied by a minimum invariant length, there is a possibility of viability. |
| first_indexed | 2024-04-13T21:26:54Z |
| format | Article |
| id | doaj.art-50ca27235b90444983ab674c6247b012 |
| institution | Directory Open Access Journal |
| issn | 1434-6044 1434-6052 |
| language | English |
| last_indexed | 2024-04-13T21:26:54Z |
| publishDate | 2018-09-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj.art-50ca27235b90444983ab674c6247b0122022-12-22T02:29:17ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-09-0178911210.1140/epjc/s10052-018-6191-4On the viability of Planck scale cosmology with quartessenceMohsen Khodadi0Kourosh Nozari1Fazlollah Hajkarim2Department of Physics, Faculty of Basic Sciences, University of MazandaranDepartment of Physics, Faculty of Basic Sciences, University of MazandaranBethe Center for Theoretical Physics and Physikalisches Institut, Universität BonnAbstract Growing evidence as the observations of the CMB (cosmic microwave background), galaxy clustering and high-redshift supernovae address a stable dynamically universe dominated by the dark components. In this paper, using a qualitative theory of dynamical systems, we study the stability of a unified dark matter-dark energy framework known as quartessence Chaplygin model (QCM) with three different equation-of-states within ultraviolet (UV) deformed Friedmann–Robertson–Walker (FRW) cosmologies without Big-Bang singularity. The UV deformation is inspired by the non-commutative (NC) Snyder spacetime approach in which by keeping the transformation groups and rotational symmetry there is a dimensionless, Planck scale characteristic parameter $$\mu _0$$ μ0 with dual implications dependent on its sign that addresses the required invariant cutoffs for length and momentum in nature, in a separate manner. Our stability analysis is done in the $$(H,\rho )$$ (H,ρ) phase space at a finite domain concerning the hyperbolic critical points. According to our analysis, due to constraints imposed on the signs of $$\mu _0$$ μ0 from the phenomenological parameters involved in quartessence models $$(\Omega _m^*, c_s^2, \rho _*)$$ (Ωm∗,cs2,ρ∗) , for an expanding and accelerating late universe, all three QCMs can be stable in the vicinity of the critical points. The requirement of stability for these quartessence models in case of admission of a minimum invariant length, can yield a flat as well as non-flat expanding and accelerating universe in which Big-Bang singularity is absent. This feedback also phenomenologically credits to braneworld-like framework versus loop quantum cosmology-like one as two possible scenarios which can be NC Snyder spacetime generators (correspond to $$\mu _0<0$$ μ0<0 and $$\mu _0>0$$ μ0>0 , respectively). As a result, our analysis show that between quartessence models with Chaplygin gas equation-of-states and accelerating FRW backgrounds occupied by a minimum invariant length, there is a possibility of viability.http://link.springer.com/article/10.1140/epjc/s10052-018-6191-4 |
| spellingShingle | Mohsen Khodadi Kourosh Nozari Fazlollah Hajkarim On the viability of Planck scale cosmology with quartessence European Physical Journal C: Particles and Fields |
| title | On the viability of Planck scale cosmology with quartessence |
| title_full | On the viability of Planck scale cosmology with quartessence |
| title_fullStr | On the viability of Planck scale cosmology with quartessence |
| title_full_unstemmed | On the viability of Planck scale cosmology with quartessence |
| title_short | On the viability of Planck scale cosmology with quartessence |
| title_sort | on the viability of planck scale cosmology with quartessence |
| url | http://link.springer.com/article/10.1140/epjc/s10052-018-6191-4 |
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