Some New Models for Charged Anisotropic Relativistic Stars with a Linear and Quadratic Equation of State
Journal of Pharmaceutical Research International · pp. 1–19 · Published 13 Jan 2023
Abstract
Taking local anisotropy into consideration, in this paper, some new analytical models of relativistic anisotropic charged quark stars with a linear and quadratic equation of state have been developed. The Einstein-Maxwell field equations have been solved with a particular form of metric potential and electric field intensity. The plots generated show that physical variables such as metric potentials, radial pressure, energy density, charge density, anisotropy, radial speed sound are consistent with realistic stellar models. We obtained some models consistent with stellar objects as 4U 1538-52,Cyg X-2, OGLE-TR-122b and red dwarf Proxima Centauri.
Cited by 0
No indexed citations yet.
Related research
- Study of Compact Stars with Buchdahl Potential in 5-D Einstein-Gauss-Bonnet Gravity — shares topic coverage
Article metrics
Real usage data collected on this platform.
31
Page views
0
PDF downloads
4
Outbound clicks
0
Citations
Views over time
Views by country
Approximate, from request IP at view time — not citizenship or institution. Countries with fewer than 5 views are grouped as "Other".
Traffic sources
Referring site, by host.
Views and downloads exclude known bots/crawlers. Citations combines this platform's own DOI-resolved index with each external source's own reported total — see Cited by above for individually listed citing works. Last refreshed 0 seconds ago.