A5102759291- Pulsars and Gravitational Waves Research
- Cosmology and Gravitation Theories
- Geophysics and Gravity Measurements
- Black Holes and Theoretical Physics
- Solar and Space Plasma Dynamics
- Astrophysical Phenomena and Observations
- Stellar, planetary, and galactic studies
- Astro and Planetary Science
- High-pressure geophysics and materials
BRAC University
2014-2019
Daffodil International University
2012-2014
In this work some families of relativistic anisotropic charged fluid spheres have been obtained by solving the Einstein–Maxwell field equations with a preferred form one metric potentials, and suitable forms electric charge distribution pressure anisotropy functions. The resulting equation state (EOS) matter has obtained. Physical analysis shows that stellar structure for considered in may reasonably model an electrically compact star whose energy density associated fields is on same order...
This work presents an algorithm for modeling a static spherically symmetric compact object satisfying the Eiesland condition (Eiesland in Am Math Soc 27:213, 1925), necessary and sufficient that general centro-symmetric space shall be of class 1. The model parameters are obtained accordingly by employing boundary conditions to interior solutions. equation state has been extracted from solution one found it is almost linear. These models free physical geometric singularities satisfy have...
In this work some families of relativistic anisotropic charged fluid spheres have been obtained by solving Einstein-Maxwell field equations with preferred form one the metric potentials, a suitable forms electric charge distribution and pressure anisotropy functions. The resulting equation state (EOS) matter has obtained. Physical analysis shows that stellar structure for in may reasonably model an electrically compact star whose energy density associated fields is on same order magnitude as...