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Hydrodynamics of a gaseous system in massive Brans-Dicke gravity

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Abstract.

This paper explores hydrodynamics and hydrostatic of a star in the post-Newtonian approximation of massive Brans-Dicke gravity. We study approximated solutions of the field equations up to \( O(c^{-4})\) and generalize Euler equations of motion. We then formulate equations governing the stability and instability of the system. Finally, we discuss spherically symmetric stars for a specific barotropic case like dust, cosmic string and domain wall in this scenario.

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Authors and Affiliations

  1. Department of Mathematics, University of the Punjab, Quaid-e-Azam Campus, 54590, Lahore, Pakistan

    M. Sharif & Rubab Manzoor

  2. Department of Mathematics, University of Management and Technology, Johar Town Campus, 54782, Lahore, Pakistan

    Rubab Manzoor

Authors
  1. M. Sharif
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  2. Rubab Manzoor
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Correspondence to M. Sharif.

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Sharif, M., Manzoor, R. Hydrodynamics of a gaseous system in massive Brans-Dicke gravity. Eur. Phys. J. Plus 131, 64 (2016). https://doi.org/10.1140/epjp/i2016-16064-0

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  • DOI: https://doi.org/10.1140/epjp/i2016-16064-0

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