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Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields

  • Regular Article - Theoretical Physics
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Abstract

In this paper, we investigate the Noether symmetries of F(T) cosmology involving matter and dark energy. In this model, the dark energy is represented by a canonical scalar field with a potential. Two special cases for dark energy are considered, including phantom energy and quintessence. We obtain F(T)∼T 3/4, and the scalar potential V(ϕ)∼ϕ 2 for both models of dark energy and discuss quantum picture of this model. Some astrophysical implications are also discussed.

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Acknowledgements

We would like to thank S.H. Hendi for useful communications and the anonymous reviewer for enlightening comments related to this work.

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Authors and Affiliations

  1. Center for Advanced Mathematics and Physics (CAMP), National University of Sciences and Technology (NUST), H-12, Islamabad, Pakistan

    Mubasher Jamil

  2. Eurasian International Center for Theoretical Physics, Eurasian National University, Astana, 010008, Kazakhstan

    Mubasher Jamil, D. Momeni & R. Myrzakulov

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  1. Mubasher Jamil
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  2. D. Momeni
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  3. R. Myrzakulov
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Correspondence to D. Momeni.

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Jamil, M., Momeni, D. & Myrzakulov, R. Noether symmetry of F(T) cosmology with quintessence and phantom scalar fields. Eur. Phys. J. C 72, 2137 (2012). https://doi.org/10.1140/epjc/s10052-012-2137-4

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  • DOI: https://doi.org/10.1140/epjc/s10052-012-2137-4

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