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Super Exponential Expansion for Dark Energy Model with Variable Λ in f (R, T) Gravity

Received: 28 March 2017     Accepted: 13 April 2017     Published: 2 June 2017
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Abstract

In this paper, we have studied Friedmann-Robertson-Walker (FRW) cosmological model with quadratic equation of state and cosmological constant in the presence of perfect fluid source in f (R, T) gravity. To obtain an exact solution of the field equations of the theory, we have used quadratic equation of state and time dependent deceleration parameter q (t). The physical and geometrical behavior of the model is also discussed.

Published in International Journal of Astrophysics and Space Science (Volume 5, Issue 3)
DOI 10.11648/j.ijass.20170503.11
Page(s) 41-46
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2017. Published by Science Publishing Group

Keywords

f (R, T) Gravity, Cosmological Model, Quadratic Equation of State, Cosmological Constant, Deceleration Parameter

References
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Cite This Article
  • APA Style

    Mohammad Moksud Alam, Mohammad Amjad Hossain, Mohammad Ashraful Islam. (2017). Super Exponential Expansion for Dark Energy Model with Variable Λ in f (R, T) Gravity. International Journal of Astrophysics and Space Science, 5(3), 41-46. https://doi.org/10.11648/j.ijass.20170503.11

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    ACS Style

    Mohammad Moksud Alam; Mohammad Amjad Hossain; Mohammad Ashraful Islam. Super Exponential Expansion for Dark Energy Model with Variable Λ in f (R, T) Gravity. Int. J. Astrophys. Space Sci. 2017, 5(3), 41-46. doi: 10.11648/j.ijass.20170503.11

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    AMA Style

    Mohammad Moksud Alam, Mohammad Amjad Hossain, Mohammad Ashraful Islam. Super Exponential Expansion for Dark Energy Model with Variable Λ in f (R, T) Gravity. Int J Astrophys Space Sci. 2017;5(3):41-46. doi: 10.11648/j.ijass.20170503.11

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  • @article{10.11648/j.ijass.20170503.11,
      author = {Mohammad Moksud Alam and Mohammad Amjad Hossain and Mohammad Ashraful Islam},
      title = {Super Exponential Expansion for Dark Energy Model with Variable Λ in f (R, T) Gravity},
      journal = {International Journal of Astrophysics and Space Science},
      volume = {5},
      number = {3},
      pages = {41-46},
      doi = {10.11648/j.ijass.20170503.11},
      url = {https://doi.org/10.11648/j.ijass.20170503.11},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20170503.11},
      abstract = {In this paper, we have studied Friedmann-Robertson-Walker (FRW) cosmological model with quadratic equation of state and cosmological constant in the presence of perfect fluid source in f (R, T) gravity. To obtain an exact solution of the field equations of the theory, we have used quadratic equation of state and time dependent deceleration parameter q (t). The physical and geometrical behavior of the model is also discussed.},
     year = {2017}
    }
    

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    T1  - Super Exponential Expansion for Dark Energy Model with Variable Λ in f (R, T) Gravity
    AU  - Mohammad Moksud Alam
    AU  - Mohammad Amjad Hossain
    AU  - Mohammad Ashraful Islam
    Y1  - 2017/06/02
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    DO  - 10.11648/j.ijass.20170503.11
    T2  - International Journal of Astrophysics and Space Science
    JF  - International Journal of Astrophysics and Space Science
    JO  - International Journal of Astrophysics and Space Science
    SP  - 41
    EP  - 46
    PB  - Science Publishing Group
    SN  - 2376-7022
    UR  - https://doi.org/10.11648/j.ijass.20170503.11
    AB  - In this paper, we have studied Friedmann-Robertson-Walker (FRW) cosmological model with quadratic equation of state and cosmological constant in the presence of perfect fluid source in f (R, T) gravity. To obtain an exact solution of the field equations of the theory, we have used quadratic equation of state and time dependent deceleration parameter q (t). The physical and geometrical behavior of the model is also discussed.
    VL  - 5
    IS  - 3
    ER  - 

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Author Information
  • Department of Mathematics, University of Chittagong, Chittagong, Bangladesh

  • Department of Mathematics, University of Chittagong, Chittagong, Bangladesh

  • Department of Mathematics, University of Chittagong, Chittagong, Bangladesh

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