Аннотации:
The existing analysis reports a reconstruction scheme of the newly proposed gravity say
f(Q) gravity through the scale factor of the form a(t) a0t
n 1
1+z by describing the powerlaw cosmology. The reconstructed f(Q) gravity models disclosed how this modified gravity
model is capable to replicate dissimilar epochs of the cosmological history. Also, the
reconstructed f(Q) gravity models are castoff to develop the expressions for density and
pressure and the equation of state parameter. We reconstruct two cases of interacting fluid
scenario ghost and pilgrim dark energy with pressureless dark matter. The physical
behavior of the models is talked over the evolution of the Universe is accelerated.
Moreover, the well-known cosmological planes i.e., (ωD − ωD′ ) and (r − s) constructed
for our models, also include a comparison of our findings of these dynamical parameters
with observational constraints. It is also quite interesting to mention here that the results of
the equation of state parameter, (ωD − ωD′ ) and (r − s)-planes coincide with the modern
observational data
