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相关论文: Interacting extended Chaplygin gas cosmology in Ly…

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In this paper, we study interacting extended Chaplygin gas as dark matter and quintessence scalar field as dark energy with an effective $\Lambda$-term in Lyra manifold. As we know Chaplygin gas behaves as dark matter at the early universe…

广义相对论与量子宇宙学 · 物理学 2016-01-20 H. Saadat

We are interested by the study of several toy models of the Universe in presence of interacting quintessence DE models. Models are considered in the cosmology with an Effective varying $\Lambda$-Term in Lyra Manifold. The motivation of the…

广义相对论与量子宇宙学 · 物理学 2015-09-16 Martiros Khurshudyan

This thesis concentrates on the accelerated expansion of the Universe recently explored by measurements of redshift and luminosity-distance relations of type Ia Supernovae. We have considered a model of the universe filled with modified…

广义相对论与量子宇宙学 · 物理学 2011-05-06 Writambhara Chakraborty

In this paper, we attempt to explore the possibility of a obtaining a viable emergent universe scenario supported by a type of fluid known as the extended Chaplygin gas, which extends a modification to the equation of state of the well…

广义相对论与量子宇宙学 · 物理学 2025-08-13 Rikpratik Sengupta , Anirban Chanda , B C Paul , M Kalam

The cosmological model of the modified Chaplygin gas interacting with cold dark matter is studied. Our attention is focused on the final state of universe in the model. It turns out that there exists a stable scaling solution, which…

广义相对论与量子宇宙学 · 物理学 2009-12-04 Song Li , Yongge Ma , Yun Chen

We investigate a kind of interacting Chaplygin gas model in which the Chaplygin gas plays the role of dark energy and interacts with cold dark matter particles. We find that there exists a stable scaling solution at late times with the…

天体物理学 · 物理学 2009-11-13 Hongsheng Zhang , Zong-Hong Zhu

Modified Chaplygin gas as an exotic fluid has been introduced in [34]. Essential features of the modified Chaplygin gas as a cosmological model are discussed. Observational constraints on the parameters of the model have been included. The…

广义相对论与量子宇宙学 · 物理学 2012-11-16 H. B. Benaoum

This article motivated by the recent articles and results of two authors. Recently, J. Sadeghi and H. Farahani presented a work [1], where they include viscosity and analyze general model, by this way they extended models considered by M.…

广义相对论与量子宇宙学 · 物理学 2016-01-05 J. Sadeghi , M. Khurshudyan , H. Farahani

In this letter we consider two different models of our present universe. We choose the models which are consisting different sets of two seperate fluids. The first one of each set tries to justify the late time acceleration and the second…

综合物理 · 物理学 2019-03-27 Promila Biswas , Ritabrata Biswas

The goal of this paper is to discuss phase space analysis of some interacting Chaplygin gas models in General Relativity. Chaplygin gas is one of the fluids actively considered in modern cosmology due to the fact that it is a joint model of…

广义相对论与量子宇宙学 · 物理学 2015-09-09 M. Khurshudyan , R. Myrzakulov

In this work the modified Chaplygin gas is related to a cosmological scalar field. Analytical results, more general than the solutions previously shown in the literature, are presented for the case when the curvature is absent, and one…

广义相对论与量子宇宙学 · 物理学 2008-03-03 Sandro Silva e Costa

In this paper, we study two different models of dark energy based on Chaplygin gas equation of state. The first model is the variable modified Chaplygin gas while the second one is the extended Chaplygin gas. Both models are considered in…

广义相对论与量子宇宙学 · 物理学 2015-02-10 E. O. Kahya , M. Khurshudyan , B. Pourhassan , R. Myrzakulov , A. Pasqua

In this paper, we consider a universe dominated by the extended Chaplygin gas which recently proposed as the last version of Chaplygin gas models. Here, we only consider the second order term which recovers quadratic barotropic fluid…

广义相对论与量子宇宙学 · 物理学 2015-04-01 E. O. Kahya , B. Pourhassan

We consider a model of the Universe with variable G and {\Lambda}. Subject of our interest is a phenomenological model for {\Lambda} proposed and considered in this article first time (up to our knowledge). Modification based on an…

广义相对论与量子宇宙学 · 物理学 2015-01-13 M. Khurshudyan , J. Sadeghi , E. Chubaryan , H. Farahani

We consider a universe filled by a modified generalized Chaplygin gas together with a pressureless dark matter component. We get a thermodynamical interpretation for the modified generalized Chaplygin gas confined to the apparent horizon of…

广义相对论与量子宇宙学 · 物理学 2016-05-18 H. Ebadi , H. Moradpour

In this work interacting Umami Chaplygin gas has been studied in flat FRW model of universe in context of it's thermodynamic and dynamical behaviour. In particular, considering Umami fluid as dark energy interacting with dark matter,…

综合物理 · 物理学 2021-05-12 Sujay Kr. Biswas , Atreyee Biswas

In this paper, we consider three different models of dark energy in higher dimensional space-time and discuss about some cosmological parameters numerically. The first model is a single component universe including viscous varying modified…

广义相对论与量子宇宙学 · 物理学 2014-06-13 M. Khurshudyan , J. Sadeghi , M. Hakobyan , H. Farahani , R. Myrzakulov

Modified Chaplygin Gas has been successful in describing the cosmic history of the universe from radiation to $\Lambda$CDM in standard cosmology, while particle creation mechanism in nonlinear thermodynamics can be used to explain inflation…

广义相对论与量子宇宙学 · 物理学 2018-01-17 Subhra Bhattacharya , Shibaji Halder , Subenoy Chakraborty

This paper is devoted to the investigation of modified Chaplygin gas model in the context of solvable k-essence cosmologies. For this purpose, we construct equations of state parameter of this model for some particular values of the…

综合物理 · 物理学 2012-07-31 M. Sharif , K. R. Yesmakhanova , S. Rani , R. Myrzakulov

The goal of this paper is to study new cosmological models where the dark energy is a varying Chaplygin gas. This specific dark energy model with non-linear EoS had been often discussed in modern cosmology. Contrary to previous studies, we…

广义相对论与量子宇宙学 · 物理学 2021-05-04 M. Khurshudyan , R. Myrzakulov
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