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Search Results: 1 - 10 of 859 matches for " Mubasher Jamil "
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Interacting new generalized Chaplygin gas
Mubasher Jamil
Physics , 2009, DOI: 10.1007/s10773-009-0178-8
Abstract: We have presented a model in which the new generalized Chaplygin gas interacts with matter. We find that there exists a stable scaling solution at late times in the evolution of the universe. Moreover, the phantom crossing scenario is observed in this model.
Evolution of a Schwarzschild Black Hole in Phantom-like Chaplygin gas Cosmologies
Mubasher Jamil
Physics , 2009, DOI: 10.1140/epjc/s10052-009-1051-x
Abstract: In the classical relativistic regime, the accretion of phantom energy onto a black hole reduces the mass of the black hole. In this context, we have investigated the evolution of a Schwarzschild black hole in the standard model of cosmology using the phantom-like modified variable Chaplygin gas and the viscous generalized Chaplygin gas. The corresponding expressions for accretion time scale and evolution of mass have been derived. Our results indicate that mass of the black hole will decrease if the accreting phantom Chaplygin gas violates the dominant energy condition and will increase in the opposite case. Thus our results are in agreement with the results of Babichev \textit{et al} \cite{Babi1} who first proposed this scenario.
Model of interacting dark energy in five-dimensional brane cosmology
Mubasher Jamil
Physics , 2008,
Abstract: We here investigate the model of interacting dark energy in the context of five dimensional brane cosmology. The effective equations of state of dark energy are evaluated for various choices of the variable time dependent cosmological constant. We have found that the interacting dark energy obeys the phantom divide/crossing scenario in this generalized model. It is also shown that interacting dark energy in this generalized model also resolves the cosmic coincidence problem.
Wormholes in Bulk Viscous Cosmology
Mubasher Jamil
Physics , 2008, DOI: 10.1393/ncb/i2008-10555-1
Abstract: We investigate the effects of the accretion of phantom energy with non-zero bulk viscosity onto a Morris-Thorne wormhole. We have found that if the bulk viscosity is large then the mass of wormhole increases rapidly as compared to small or zero bulk viscosity.
Variable G correction to statefinder parameters of dark energy
Mubasher Jamil
Physics , 2010, DOI: 10.1007/s10773-010-0475-2
Abstract: Motivated by several observational and theoretical developments concerning the variability of Newton's gravitational constant with time $G(t)$, we calculate the varying $G$ correction to the statefinder parameters for four models of dark energy namely interacting dark energy, holographic dark energy, new-agegraphic dark energy and generalized Chaplygin gas.
Primordial Black Holes in Phantom Cosmology
Mubasher Jamil,Asghar Qadir
Physics , 2009, DOI: 10.1007/s10714-010-0928-1
Abstract: We investigate the effects of accretion of phantom energy onto primordial black holes. Since Hawking radiation and phantom energy accretion contribute to a {\it decrease} of the mass of the black hole, the primordial black hole that would be expected to decay now due to the Hawking process would decay {\it earlier} due to the inclusion of the phantom energy. Equivalently, to have the primordial black hole decay now it would have to be more massive initially. We find that the effect of the phantom energy is substantial and the black holes decaying now would be {\it much} more massive -- over 10 orders of magnitude! This effect will be relevant for determining the time of production and hence the number of evaporating black holes expected in a universe accelerating due to phantom energy.
Generalized second law of thermodynamics for a phantom energy accreting BTZ black hole
Mubasher Jamil,M. Akbar
Physics , 2010, DOI: 10.1007/s10714-010-1024-2
Abstract: In this paper, we have studied the accretion of phantom energy on a (2+1)-dimensional stationary Banados-Teitelboim-Zanelli (BTZ) black hole. It has already been shown by Babichev et al that for the accretion of phantom energy onto a Schwarzschild black hole, the mass of black hole would decrease and the rate of change of mass would be dependent on the mass of the black hole. However, in the case of (2+1)-dimensional BTZ black hole, the mass evolution due to phantom accretion is independent of the mass of the black hole and is dependent only on the pressure and density of the phantom energy. We also study the generalized second law of thermodynamics at the event horizon and construct a condition that puts an lower bound on the pressure of the phantom energy.
Interacting entropy-corrected agegraphic-tachyon dark energy
Mubasher Jamil,Ahmad Sheykhi
Physics , 2010, DOI: 10.1007/s10773-010-0585-x
Abstract: Motivated by recent work of one of us [1], we generalize this work to agegraphic tachyon models of dark energy with entropy correction terms arising from loop quantum gravity. We establish a connection between the entropy-corrected agegraphic dark energy and the tachyon scalar field in a universe with spacial curvature and reconstruct the potential and the dynamics of the tachyon scalar field which describe the tachyon cosmology. The cosmological implications of the entropy-corrected agegraphic dark energy models are also discussed.
Gravitational collapse of radiation fluid in higher dimensions
Mubasher Jamil,Umar Farooq
Physics , 2008,
Abstract: We examine the problem of the gravitational collapse using higher dimensional Husain spacetime for the null fluid. The equations of state chosen to solve the field equations contain linear, quadratic and arbitrary powers of the radial parameter. The resulting mass evolution is discussed for each case.
On the resolution of cosmic coincidence problem and phantom crossing with triple interacting fluids
Mubasher Jamil,Farook Rahaman
Physics , 2008, DOI: 10.1140/epjc/s10052-009-1134-8
Abstract: We here investigate a cosmological model in which three fluids interact with each other involving certain coupling parameters and energy exchange rates. The motivation of the problem stems from the puzzling `triple coincidence problem' which naively asks why the cosmic energy densities of matter, radiation and dark energy are almost of the same order of magnitude at the present time. In our model, we determine the conditions under triple interacting fluids will cross the phantom divide.
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