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cosmological model

by P. Pedram, S. Jalalzadeh, S. S. Gousheh , 2008
"... Schrödinger-Wheeler-DeWitt equation in chaplygin gas FRW ..."
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Schrödinger-Wheeler-DeWitt equation in chaplygin gas FRW

FRW cosmology with extended Chaplygin gas

by unknown authors , 2014
"... ar ..."
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Abstract not found

FRW Cosmological model with Modified Chaplygin Gas and

by Nairwita Mazumder, Ritabrata Biswas, Subenoy Chakraborty
"... ar ..."
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Abstract not found

Holographic Chaplygin gas model

by M. R. Setare , 704
"... In this paper we consider a correspondence between the holographic dark energy density and Chaplygin gas energy density in FRW universe. Then we reconstruct the potential and the dynamics of the scalar field which describe the Chaplygin cosmology. ..."
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In this paper we consider a correspondence between the holographic dark energy density and Chaplygin gas energy density in FRW universe. Then we reconstruct the potential and the dynamics of the scalar field which describe the Chaplygin cosmology.

Chaplygin

by Chao-jun Feng, Xin-zhou Li , 909
"... gas and the cosmological evolution of alpha ..."
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gas and the cosmological evolution of alpha

An Attempt for an Emergent Scenario with Modified Chaplygin Gas

by Sourav Dutta , Sudeshna Mukerji , Subenoy Chakraborty , Ahmed Farag , Ali
"... The present work is an attempt for emergent universe scenario with modified Chaplygin gas. The universe is chosen as spatially flat FRW space-time with modified Chaplygin gas as the only cosmic substratum. It is found that emergent scenario is possible for some specific (unrealistic) choice of the ..."
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The present work is an attempt for emergent universe scenario with modified Chaplygin gas. The universe is chosen as spatially flat FRW space-time with modified Chaplygin gas as the only cosmic substratum. It is found that emergent scenario is possible for some specific (unrealistic) choice

Chaplygin gas

by A J Hariton , 2007
"... Fermionic extension of the scalar Born-Infeld equation and its relation to the supersymmetric ..."
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Fermionic extension of the scalar Born-Infeld equation and its relation to the supersymmetric

Modified Chaplygin Gas as Scalar Field and Holographic Dark Energy Model

by P. Thakur, A. Saha
"... We study the correspondence between field theoretic and holographic dark energy density of the universe with the modified Chaplygin gas (MCG) respectively both in a flat and non-flat FRW universe. We present an equivalent representation of the MCG with a homogeneous minimally coupled scalar field by ..."
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We study the correspondence between field theoretic and holographic dark energy density of the universe with the modified Chaplygin gas (MCG) respectively both in a flat and non-flat FRW universe. We present an equivalent representation of the MCG with a homogeneous minimally coupled scalar field

Holographic Dark Energy Scenario and Variable Modified Chaplygin Gas

by Surajit Chattopadhyay, Ujjal Debnath , 2009
"... In this letter, we have considered that the universe is filled with normal matter and variable modified Chaplygin gas. Also we have considered the interaction between normal matter and variable modified Chaplygin gas in FRW universe. Then we have considered a correspondence between the holographic d ..."
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In this letter, we have considered that the universe is filled with normal matter and variable modified Chaplygin gas. Also we have considered the interaction between normal matter and variable modified Chaplygin gas in FRW universe. Then we have considered a correspondence between the holographic

Constraining the Parameters of Modified Chaplygin Gas in Einstein-Aether Gravity

by Ujjal Debnath
"... We have assumed FRW model of the universe in Einstein-Aether gravity filled with dark matter and modified Chaplygin gas (MCG) type dark energy. We present the Hubble parameter in terms of some unknown parameters and observational parameters with the redshift z. From observed Hubble data (OHD) set ( ..."
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We have assumed FRW model of the universe in Einstein-Aether gravity filled with dark matter and modified Chaplygin gas (MCG) type dark energy. We present the Hubble parameter in terms of some unknown parameters and observational parameters with the redshift z. From observed Hubble data (OHD) set
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