Dynamical analysis of charged anisotropic spherical star in f(r) gravity

dc.contributor.authorH. Rizwana Kausar
dc.contributor.authorIfra Noureen
dc.contributor.authorM. Umair Shahzad
dc.date.accessioned2015-11-13T11:54:56Z
dc.date.available2015-11-13T11:54:56Z
dc.date.issued2015
dc.description.abstractWe consider a modified gravity theory, f(R) = R + Rn − μ4 Rm , in the metric formulation and analyze the contribution of electromag- netic field on the range of dynamical instability of a star filled with anisotropic matter. The collapse equation is developed by applying conservation on anisotropic matter, Maxwell source and dark source terms arising due to f(R) gravity. Specific perturbation scheme is implemented and it is observed that the inclusion of Maxwell source slows down the collapse and makes system more stable in Newtonian regime. Also, we make comparison of our results with the existing literature.en_US
dc.identifier.citation9. Kausar, H. R., Noureen, I., & Shahzad, M. U. (2015). Dynamical analysis of charged anisotropic spherical star in f (R) gravity. The European Physical Journal Plus, 130(10), 1-10.en_US
dc.identifier.urihttps://escholar.umt.edu.pk/handle/123456789/1609
dc.publisherThe European Physical Journal Plusen_US
dc.titleDynamical analysis of charged anisotropic spherical star in f(r) gravityen_US
dc.typeArticleen_US
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