Kaluza-Klein cosmological model with strange-quark-matter in f(R,T) theory of gravity

This work deals with the Kaluza-Klein cosmological model with strange-quark-matter in f(R,T) theory of gravity, where R is the Ricci scalar and T is the trace of the energy-momentum tensor. To determine the solution of the field equation, we have assumed that scalar expansion theta is proportional to shear scalar sigma(2) which leads to R=Am, where R and A are metric potentials and m is constant. The cosmological parameters are investigated with the help of the equation of state strange-quark-matter (SQM) is p=rho-(4Bc)(3), where B-c is Bag constant. We have concentrated on the distances of cosmology such as the look-back time, proper distance, luminosity distance, angular-diameter distance and distance modulus which are presented graphically by using suitable data of H-0. The physical and geometrical properties of models are also discussed.