We present a new class of singularity-free interior solutions for anisotropic compact stars with spherical symmetry. By prescribing a specific pressure anisotropy, exact solutions to Einstein’s field equations are obtained and matched smoothly to the Schwarzschild exterior metric. The model parameters are determined using the boundary condition of vanishing radial pressure. The physical viability of the model is demonstrated through an analysis of the pulsar 4U1820-30, characterized by a radius of 9. 1 km and mass M=1. 58M_.
Building similarity graph...
Analyzing shared references across papers
Loading...
Rinkal Patel (Sun,) studied this question.
www.synapsesocial.com/papers/69ba43884e9516ffd37a4ea7 — DOI: https://doi.org/10.1134/s0202289325700628
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:
Rinkal Patel
Gravitation and Cosmology
Building similarity graph...
Analyzing shared references across papers
Loading...