Hydrodynamics of a gaseous system in massive brans-dicke gravity

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dc.contributor.authorRubab Manzoor
dc.date.accessioned2018-10-15T10:38:59Z
dc.date.available2018-10-15T10:38:59Z
dc.date.issued2016
dc.description.abstractThis 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.en_US
dc.identifier.citationSharif, M., & Manzoor, R. (2016). Hydrodynamics of a gaseous system in massive Brans-Dicke gravity. The European Physical Journal Plus, 131(64), 1-13. (Rubab Manzoor (Mathematics /SSC), JCR LISTED (IF:1:521))en_US
dc.identifier.urihttps://escholar.umt.edu.pk/handle/123456789/3246
dc.language.isoenen_US
dc.publisherThe European Physical Journal Plus, Springer Linken_US
dc.subjectMathematicsen_US
dc.subjectDark Energy Domain Wall Cosmic String Hydrostatic Equilibrium Pressure Gradient Forceen_US
dc.titleHydrodynamics of a gaseous system in massive brans-dicke gravityen_US
dc.typeArticleen_US
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