  This paper explores a cosmological reconstruction scheme in the background of
f(Q) gravity theory from a Holographic perspective. The basic motivation for
this work is that the reconstruction is performed from a holographic origin,
which has its roots in the black hole thermodynamics and quantum gravity. Dark
energy models inspired by holographic prescription are used to reconstruct the
f(Q) gravity models. Two such models, namely the Granda-Oliveros holographic
dark energy model and its generalization, the Chen- Jing model are considered
for the study. Different scale factors are used and a thorough reconstruction
scheme is set up using the dark energy models. The observationally constrained
values of the free model parameters have been used to form the reconstructed
models. Finally, a thorough investigation of the energy conditions has been
performed to check the cosmological viability of the reconstructed f(Q) models.
As an outcome, we get some very promising and cosmologically viable f(Q) models
that present some interesting properties and demand further investigation.
