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A non-exotic Morris-Thorne model of wormhole in the presence of a scalar field

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Abstract.

In this study, we derive the Einstein field equations for the Morris-Thorne wormhole geometry within the concepts of the scalar tensor theory in the presence of a scalar field which depends on the radial co-ordinate r . We analyze the non-exotic matter aspects via the null energy condition (NEC) and represent the requirements necessary for the ordinary matter or electromagnetic radiation formation of the wormhole by the way we represent a non-exotic model. In addition, we express particular example of that model satisfying those requirements and the equations of motion.

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Authors and Affiliations

  1. Department of Physics, Adnan Menderes University, Aydın, Turkey

    Onur Genç

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  1. Onur Genç
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Correspondence to Onur Genç.

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Genç, O. A non-exotic Morris-Thorne model of wormhole in the presence of a scalar field. Eur. Phys. J. Plus 134, 356 (2019). https://doi.org/10.1140/epjp/i2019-12825-5

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  • DOI: https://doi.org/10.1140/epjp/i2019-12825-5

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