TURKISH PHYSICAL SOCIETY 40TH INTERNATIONAL PHYSICS CONGRESS, Muğla, Türkiye, 2 - 06 Eylül 2024, ss.253
Our work focuses on thoroughly investigating the inner constitution of assorted
anisotropic massive compact objects like quark stars form, using the f(R, T, Q)
modified theory of gravity. These stars interact with an electromagnetic field because
of their charges. In this theory, we particularly examine a ordinary type of function
characterized by first degree of the Ricci scalar and the factor Q. To analyze the inner
constitution of intensive quark stars form, our approach employs a spherically
symmetric metric inclusive charge, which derived the corresponding field equations.
The solutions of these equations are obtained using specific metric potentials and the
Bag Model. We use observational informations certain the radius and masses of two
type quark stars, SMC X-4 and SAX J 1808.4-3658 to evaluate how charge and
altered adjustment expressions influence their dynamics. Additionally, we estimate
the physical significance of the acquired model by changing the revised model
parameter.