Challenging f(R,T) theory with ΛCDM model through cosmographic parameters.

In this paper, we reconstruct a f (R , T) model where R and T are the curvature scalar and the trace of the stress-tensor, respectively, and confront it with Λ CDM model through the cosmographic parameters. The reconstructed f (R , T) model is fundamentally characterized by a input parameter β for which some suitable values are chosen. Our results show that for some values of these parameters the reconstructed f (R , T) fits very well with the Λ CDM regarding the evolution of the cosmographic parameters. [ABSTRACT FROM AUTHOR]