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Wormholes in f(R, T) gravity with density-dependent B parameter in SQM

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Abstract

Wormhole solutions are obtained in the modified f(R, T) gravity with strange quark matter. The equation of state of the strange quark matter (SQM) is the phenomenological MIT Bag model. Both constant and density-dependent bag parameters (B) are considered in the framework of modified f(R, T) gravity. We have examined the possible construction of a stationary, spherically symmetric and spatially inhomogeneous wormhole spacetime supported by the SQM. It is shown that there are two types of wormhole solutions are permitted in the theory where null energy condition (NEC) is obeyed and in other case NEC is not satisfied with power law shape function. In the case of hybrid shape function, a new class of wormhole solutions are obtained satisfying all the energy conditions.

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Acknowledgements

BCP would like to thank IUCAA Centre for Astronomy Research and Development (ICARD), NBU for extending research facilities. The authors are thankful to the anonymous Referee for his constructive suggestion.

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Authors and Affiliations

  1. IUCAA Centre for Astronomy Research & Development (ICARD), University of North Bengal, Siliguri Dist., Darjeeling, 734013, India

    Rumi Deb

  2. Department of Physics, A. C. College, Jalpaiguri, West Bengal, 735102, India

    Priyanka Mandal

  3. Department of Physics, University of North Bengal, Siliguri, Dist, Darjeeling, 734 013, West Bengal, India

    Bikash Chandra Paul

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  1. Rumi Deb
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  2. Priyanka Mandal
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Correspondence to Bikash Chandra Paul.

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Deb, R., Mandal, P. & Paul, B.C. Wormholes in f(R, T) gravity with density-dependent B parameter in SQM. Eur. Phys. J. Plus 137, 481 (2022). https://doi.org/10.1140/epjp/s13360-022-02685-9

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