  This study deals with the formation and evolution of a strange star in the
Krori Barua Rainbow spacetime from collapsing charged stringy quark matter. The
dynamical variables are explored from the field equations, taking into account
the effects of particle's energy on the mass density, pressure, and string
tension. The electric field is also computed using the MIT Bag model. The real
time data of SAX J1808.4-3658 is used to analyzed the physical properties
including gradients, energy conditions, anisotropy, stability, Tolman
Oppenheimer Volkoff equation, mass function, compactness, and red-shift. The
graphical analysis has been made according to both the theories of rainbow
gravity and general relativity. The energy conditions and anisotropy are found
to be satisfied, indicating the physical existence of suggested model. Tolman
Oppenheimer Volkoff equation is satisfied indicating equilibrium of forces and
stability of the compact object. Overall, our model is consistent with the
observational information of SAX J1808.4-3658.
