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Role of Modified Chaplygin Gas in Accelerated Universe

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arxiv gr-qc/0411015 v1 pith:ZYMQQZSU submitted 2004-11-02 gr-qc

Ujjal Debnath , Asit Banerjee , Subenoy Chakraborty This is my paper · ORCID
classification gr-qc
keywords modelmodifieduniversechaplyginphaseroleacceleratedaccelerating
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abstract

In this paper we have considered a model of modified Chaplygin gas and its role in accelerating phase of the universe. We have assumed that the equation of state of this modified model is valid from the radiation era to $\Lambda$CDM model. We have used recently developed statefinder parameters in characterizing different phase of the universe diagrammatically.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Threshold Drop in Accretion Density if Dark Energy is Accreting onto a Supermassive Black Hole

    gr-qc 2019-08 conditional novelty 5.0 of 10

    Viscous, rotating accretion of modified Chaplygin gas dark energy onto a supermassive black hole produces a threshold drop in accretion density and a stronger wind.

  2. Black holes in Einstein-Gauss-Bonnet gravity with a background of modified Chaplygin gas

    gr-qc 2019-08 conditional novelty 4.0 of 10

    The authors obtain a static 5D Einstein-Gauss-Bonnet black hole solution surrounded by modified Chaplygin gas and analyze its thermodynamics, scalar tunneling, and perturbative stability.

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