Model of Charged Anisotropic Strange Stars in Minimally Coupled Gravity

Figure 20

Combined graphical behaviors with magnified images of the metric potentials ( and ) versus for compact object () SAX J 1808.4-3658 with their respective unknown arbitrary constant values given in Tables 1 and 2 for two viable models (a) and (b). From each plot of the metric potentials, the evolution is positive throughout the interior compact object and attains maximum position towards the boundary surface.

(a)

(b)