The plot of radial adiabatic index for H=0.3.

<div><p>In this article, a class of static configurations for stellar equilibrium in relativistic charged spheres with anisotropic fluid is studied. The Buchdahl ansatz is employed to solve the Einstein-Maxwell field equations, which govern the behavior of charged, relativistic stellar o...

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التفاصيل البيبلوغرافية
المؤلف الرئيسي:	A. Zahra (19484713) (author)
مؤلفون آخرون:	S. A. Mardan (19484716) (author), Sana Saleem (3551681) (author), Muhammad Bilal Riaz (14341552) (author), Tomas Kozubek (21395600) (author)
منشور في:	2025
الموضوعات:	Biophysics Biotechnology Evolutionary Biology Ecology Marine Biology Inorganic Chemistry Science Policy Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified necessary energy conditions modified chaplygin equation maxwell field equations matter distribution within several compact objects relativistic stellar objects hydrostatic equilibrium condition possibly exotic stars star &# 8217 relativistic charged spheres metric </ p buchdahl ansatz provides including neutron stars stellar equilibrium compact stars buchdahl ansatz xlink "> surface redshift static configurations results demonstrate realistic description psr j2215 psr j1614 psr j0952 psr j0740 psr j0030 pressure occur presented graphically physical viability maximum density gw 190814 gw 170817 electric charge charged sphere behaved throughout avoiding singularities anisotropic fluid adiabatic index 4u 1608
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The plot of radial adiabatic index for H=0.3.

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