Magnetic Field of a Compact Spherical Star under f(R,T) Gravity
arXiv:1812.02568 · doi:10.1088/0256-307X/35/9/099501
Abstract
We present the interior solutions of distributions of magnetised fluid inside a sphere in gravity. The magnetised sphere is embedded in an exterior Reissner-Nordström metric. We assume that all physical quantities are in static equilibrium. The perfect fluid matter is studied under a particular form of the Lagrangian density . The magnetic field profile in modified gravity is calculated. Observational data of neutron stars are used to plot suitable models of magnetised compact objects. We reveal the effect of gravity on the magnetic field profile, with application to neutron stars, especially highly magnetized neutron stars found in X-ray pulsar systems. Finally the effective potential and innermost stable circular orbits, arising out of motion of a test particle of negligible mass influenced by attraction or repulsion from the massive center, are discussed.
arXiv comment7 pages, 5 figures
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- Investigating the physical and geometrical parameters of the cosmological models with anisotropic background
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