Abstract We perform a detailed physical analysis for
a class of exact solutions for the Einstein-Maxwell equations.
The linear equation of state consistent with
quark stars has been incorporated in the model. The
physical analysis of the exact solutions is performed
by considering the charged anisotropic stars for the
particular nonsingular exact model obtained by Maharaj,
Sunzu and Ray. In performing such an analysis
we regain masses obtained by previous researchers for
isotropic and anisotropic matter. It is also indicated
that other masses and radii may be generated which
are in acceptable ranges consistent with observed values
of stellar objects. A study of the mass-radius relation
indicates the effect of the electromagnetic field and
anisotropy on the mass of the relativistic star
Sunzu, J (2021). Charged Anisotropic Models For Quark Stars. Afribary. Retrieved from https://tracking.afribary.com/works/charged-anisotropic-models-for-quark-stars
Sunzu, Jefta "Charged Anisotropic Models For Quark Stars" Afribary. Afribary, 26 Apr. 2021, https://tracking.afribary.com/works/charged-anisotropic-models-for-quark-stars. Accessed 22 Nov. 2024.
Sunzu, Jefta . "Charged Anisotropic Models For Quark Stars". Afribary, Afribary, 26 Apr. 2021. Web. 22 Nov. 2024. < https://tracking.afribary.com/works/charged-anisotropic-models-for-quark-stars >.
Sunzu, Jefta . "Charged Anisotropic Models For Quark Stars" Afribary (2021). Accessed November 22, 2024. https://tracking.afribary.com/works/charged-anisotropic-models-for-quark-stars